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w_20251207_115808493343 | ALICE detector at LHC records like- and unlike-sign pion, kaon, and proton correlations with high-statistics multiplicity classes | ALICE detector at LHC records like- and unlike-sign pion, kaon, and proton correlations with high-statistics multiplicity classes | [
"ALICE detector",
"13 TeV LHC collisions",
"high-statistics data sample"
] | 0.85 | medium | universal | physics | arxiv | 2511.10399v1 | https://arxiv.org/abs/2511.10399v1 | [
"hep-ex",
"nucl-ex",
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] | ad706c982765a1010bba5df7cca12085be8d9b7286df54c0bfbdef9ebe45e12c | Extracted from ArXiv paper 2511.10399v1 (chunk 12) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T11:58:08.493343Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_115844473033 | Two-particle angular correlations in pp collisions at √s = 13 TeV observed to have a significant impact on the event-by-event flow harmonics in ALICE Collaboration data | Two-particle angular correlations in pp collisions at √s = 13 TeV observed to have a significant impact on the event-by-event flow harmonics in ALICE Collaboration data | [
"ALICE detector, 2023 LHC run",
"Collision energy: 13 TeV",
"Event statistics: 10^9 events analyzed"
] | 0.85 | high | universal | physics | arxiv | 2511.10399v1 | https://arxiv.org/abs/2511.10399v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 3ecf1f8fe2cdc20efa45e0aed41093a8dcb375abfd6381282f25109df4fb0415 | Extracted from ArXiv paper 2511.10399v1 (chunk 25) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T11:58:44.473033Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_115732663456 | The probability to observe specific numbers of strange particles per event is measured in pp collisions at √s = 5.02 TeV, for the first time. | The probability to observe specific numbers of strange particles per event is measured in pp collisions at √s = 5.02 TeV, for the first time. | [
"ALICE detector",
"charged-particle multiplicity-density classes",
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] | 0.85 | high | universal | physics | arxiv | 2511.10413v1 | https://arxiv.org/abs/2511.10413v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
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] | 0b82dcad569c37379c5ed6e715cf410a2e3ab174c821e6a0f672d7437bbb1b65 | Extracted from ArXiv paper 2511.10413v1 (chunk 2) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T11:57:32.663976Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_115739290763 | Charged-particle multiplicity density at central pseudorapidity is measured to be 5.48 ± 0.07 per unit of η, across all event classes. | Charged-particle multiplicity density at central pseudorapidity is measured to be 5.48 ± 0.07 per unit of η, across all event classes. | [
"ALICE Collaboration detector",
"Event class: INEL > 0",
"Pseudorapidity range: |η| < 0.5"
] | 0.85 | medium | universal | physics | arxiv | 2511.10413v1 | https://arxiv.org/abs/2511.10413v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
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"astro-ph.HE"
] | bf1c2aefea1b438a24a053f88d06d39aaf534d4a178aca8e2caede890d57b7f8 | Extracted from ArXiv paper 2511.10413v1 (chunk 4) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T11:57:39.290763Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_115811059259 | A strangeness-induced charged-particle multiplicity bias effect is observed in pp collisions at √s = 5.02 TeV, with a relative shift in ⟨dNch/dη⟩ dependent on the number of strange particles requested and species under study. | A strangeness-induced charged-particle multiplicity bias effect is observed in pp collisions at √s = 5.02 TeV, with a relative shift in ⟨dNch/dη⟩ dependent on the number of strange particles requested and species under study. | [
"ALICE Collaboration data",
"PYTHIA 8 QCD-CR + Ropes simulation",
"Multi-strange hadron production"
] | 0.85 | high | universal | physics | arxiv | 2511.10413v1 | https://arxiv.org/abs/2511.10413v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
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"astro-ph.HE"
] | 1852486979394e5b071d8df884914e4080783d4fc15e3ca9a295d1dec293a6d0 | Extracted from ArXiv paper 2511.10413v1 (chunk 14) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T11:58:11.059259Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_115821501625 | Strangeness-enhancement is observed with a maximum unbalance of strange-quark content (∆S) of five for the first time in pp collisions at √s = 5.02 TeV. | Strangeness-enhancement is observed with a maximum unbalance of strange-quark content (∆S) of five for the first time in pp collisions at √s = 5.02 TeV. | [
"ALICE Collaboration experiment, data taken at LHC",
"Ratios between production yields of particles with different strangeness content",
"Up to ∆S=5 is achieved, corresponding to an unprecedented enhancement of two orders of magnitude"
] | 0.85 | high | universal | physics | arxiv | 2511.10413v1 | https://arxiv.org/abs/2511.10413v1 | [
"hep-ex",
"nucl-ex",
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] | 90548bafc39d89c5208402d065be25202320fac42fe040d7cd4ca763d3bd1bef | Extracted from ArXiv paper 2511.10413v1 (chunk 17) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T11:58:21.501625Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_115858530135 | Multiple strange hadrons are produced in proton-proton collisions at √s = 5.02 TeV, with a yield ratio between multi-strange to single strange baryons measured as 0.75 ± 0.03 | Multiple strange hadrons are produced in proton-proton collisions at √s = 5.02 TeV, with a yield ratio between multi-strange to single strange baryons measured as 0.75 ± 0.03 | [
"ALICE Collaboration",
"pp collision data at LHC",
"Integrated luminosity: 9.8 pb^(-1)"
] | 0.85 | high | universal | physics | arxiv | 2511.10413v1 | https://arxiv.org/abs/2511.10413v1 | [
"hep-ex",
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"astro-ph.HE"
] | 12edb4f736de30b369251407341e824ad656e0e78781df074500b173c276e95f | Extracted from ArXiv paper 2511.10413v1 (chunk 32) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T11:58:58.530135Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_115901380777 | Multiplicity and transverse momentum distributions of multi-strange hadrons are studied in proton-proton collisions at √s = 5.02 TeV, with the ALICE detector at the LHC. | Multiplicity and transverse momentum distributions of multi-strange hadrons are studied in proton-proton collisions at √s = 5.02 TeV, with the ALICE detector at the LHC. | [
"ALICE Collaboration",
"pp collisions at √s = 5.02 TeV",
"Multiplicity: 10^6 events recorded"
] | 0.85 | medium | universal | physics | arxiv | 2511.10413v1 | https://arxiv.org/abs/2511.10413v1 | [
"hep-ex",
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"astro-ph.HE"
] | f91f4ddc7a4500695c4006c5ab3f51f39d55a682ec186875603be59cc5cab745 | Extracted from ArXiv paper 2511.10413v1 (chunk 33) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T11:59:01.380777Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_115803282157 | We observed that the zonal-to-total kinetic energy ratio varies significantly across different turbulence models, with values ranging from 24.3% to 97.3%. | We observed that the zonal-to-total kinetic energy ratio varies significantly across different turbulence models, with values ranging from 24.3% to 97.3%. | [
"Table II: The Hasegawa-Wakatani model",
"Zonal-to-total kinetic energy ratio: 36.4 ± 1.0%",
"Two-layer quasi-geostrophic (QG) model"
] | 0.85 | medium | universal | physics | arxiv | 2511.10438v1 | https://arxiv.org/abs/2511.10438v1 | [
"hep-ex",
"nucl-ex",
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"astro-ph.HE"
] | d251555b2efe771323a69b4fcc76b9f976ac30af0698c030159ff169324d5796 | Extracted from ArXiv paper 2511.10438v1 (chunk 2) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T11:58:03.282157Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_115841959824 | The transition between 2D turbulence and zonal flows (ZFs) is observed with a sharp boundary at C/κ ≈0.1, featuring a hysteresis loop in the transition. | The transition between 2D turbulence and zonal flows (ZFs) is observed with a sharp boundary at C/κ ≈0.1, featuring a hysteresis loop in the transition. | [
"HW system simulation",
"Transition scale: 1/kβ",
"Rossby/drift wave frequency matched to inverse eddy turnover time"
] | 0.85 | high | universal | physics | arxiv | 2511.10438v1 | https://arxiv.org/abs/2511.10438v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 436d97d7baa025e36dde6a6838a78d570e0872e53dfed519f9d98f94cd72b647 | Extracted from ArXiv paper 2511.10438v1 (chunk 14) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T11:58:41.959824Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_115907349585 | The substructure of bottom quark jets in proton-proton collisions at 5.02 TeV is measured, showing a strong suppression of emissions at small soft-drop-groomed jet radius values compared to inclusive jets. | The substructure of bottom quark jets in proton-proton collisions at 5.02 TeV is measured, showing a strong suppression of emissions at small soft-drop-groomed jet radius values compared to inclusive jets. | [
"CMS experiment, 2017 data",
"301 pb−1 integrated luminosity",
"Soft-drop-groomed jet radius and momentum balance observables are used"
] | 0.85 | high | universal | physics | arxiv | 2511.10666v1 | https://arxiv.org/abs/2511.10666v1 | [
"hep-ex",
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"astro-ph.HE"
] | 1e2dd2564511134e5259301bd4d974c56cb10aa91eb596bdc7c9ef13ea59ca7e | Extracted from ArXiv paper 2511.10666v1 (chunk 0) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T11:59:07.349585Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120018632138 | Neutron capture cross sections for 88Y constrained with a narrow uncertainty of 7.6%-23.1% within neutron energy range of 0.01 to 3.0 MeV | Neutron capture cross sections for 88Y constrained with a narrow uncertainty of 7.6%-23.1% within neutron energy range of 0.01 to 3.0 MeV | [
"Bayesian optimization and Markov chain Monte Carlo method",
"Experimental data on gamma-decay probability and gamma-ray strength function",
"Comparison with measured data for the 88Sr(p,γ) reaction"
] | 0.85 | high | universal | physics | arxiv | 2511.10955v1 | https://arxiv.org/abs/2511.10955v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 13c36b7135dc256dec9321be2b3a55358cf758a7aaffaf94b99a69b251f18d3f | Extracted from ArXiv paper 2511.10955v1 (chunk 0) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:00:18.632662Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120025319241 | 88Y(n, γ) reaction cross sections extracted with reduced uncertainties using a joint optimization framework combining Bayesian optimization and Markov chain Monte Carlo method | 88Y(n, γ) reaction cross sections extracted with reduced uncertainties using a joint optimization framework combining Bayesian optimization and Markov chain Monte Carlo method | [
"proton inelastic scattering from 89Y target",
"coupled-channel reaction framework",
"experimental data of gamma-decay probability Pγ"
] | 0.85 | medium | universal | physics | arxiv | 2511.10955v1 | https://arxiv.org/abs/2511.10955v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 30c744ca53b4a1e8694a8824fee33a2a50c486b4351c33ac05f31a5ee61bd97d | Extracted from ArXiv paper 2511.10955v1 (chunk 2) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.10955v1"
} | science | WO-ARX-01 | 2025-12-07T12:00:25.319760Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120035275274 | The γ-decay probability for the 89Y*(p,p'γ) reaction has been measured as a function of excitation energy E*. | The γ-decay probability for the 89Y*(p,p'γ) reaction has been measured as a function of excitation energy E*. | [
"25 HPGe coaxial detectors and eight Clover detectors surrounding the target chamber",
"Total number of detected protons (Np) and coincidences between a proton and the γ-ray (Ng)",
"Energy resolution: 2.99 keV at 1.33 MeV"
] | 0.85 | medium | universal | physics | arxiv | 2511.10955v1 | https://arxiv.org/abs/2511.10955v1 | [
"hep-ex",
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] | 00da4618bb2b8b758f84818f983a49992566221762f28ca87a7622cb70b318fe | Extracted from ArXiv paper 2511.10955v1 (chunk 4) | [
"experimental_physics",
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} | science | WO-ARX-01 | 2025-12-07T12:00:35.275274Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120042883026 | 88Y(n, γ) cross sections predicted with the SRM have uncertainties between 7.6% at E_n=0.01 MeV and 23.1% at E_n=3.0 MeV | 88Y(n, γ) cross sections predicted with the SRM have uncertainties between 7.6% at E_n=0.01 MeV and 23.1% at E_n=3.0 MeV | [
"SRM prediction for 88Y(n, γ) cross sections",
"Uncertainty range: 7.6% to 23.1%",
"Experimentally constrained with Pγ(E*) and γSF data"
] | 0.85 | medium | universal | physics | arxiv | 2511.10955v1 | https://arxiv.org/abs/2511.10955v1 | [
"hep-ex",
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] | 03e4791f01e5f533140f1c92e569d649272de8176ea5ba790de892aff1527f03 | Extracted from ArXiv paper 2511.10955v1 (chunk 6) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:00:42.883026Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120042065066 | Electron density changes in dusty plasma measured using RF-compensated Langmuir probe after laser stimulated photodetachment. | Electron density changes in dusty plasma measured using RF-compensated Langmuir probe after laser stimulated photodetachment. | [
"RF compensated single Langmuir probe (10 mm length, 114.3 μm radius) biased by the bipolar amplifier and signal generator",
"Laser beam energy varied between 2-75 mJ at 355 nm (10 Hz, ~9 ns pulse width)",
"Current signals recorded with Siglent SDS 2354X HD oscilloscope through the 5.1 kΩ shunt resistor"
] | 0.85 | medium | universal | physics | arxiv | 2511.10956v1 | https://arxiv.org/abs/2511.10956v1 | [
"hep-ex",
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] | 0479117b483c3ff79dc4fbd4c74af3cfc1aa0b70df7af506e3e98a8c48a34d01 | Extracted from ArXiv paper 2511.10956v1 (chunk 4) | [
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w_20251207_120056592217 | We report the first search for flavor-changing neutral-current decays B →Xsν¯ν with no significant signal observed, setting upper limits on partial branching fractions at 90% confidence level. | We report the first search for flavor-changing neutral-current decays B →Xsν¯ν with no significant signal observed, setting upper limits on partial branching fractions at 90% confidence level. | [
"Belle II detector, 365 fb−1 integrated luminosity collected at Υ(4S) resonance",
"43 fb−1 integrated luminosity collected at center-of-mass energy 60 MeV below resonance for background estimation",
"30 Xs decay modes used in sum-of-exclusives approach"
] | 0.85 | high | universal | physics | arxiv | 2511.10980v1 | https://arxiv.org/abs/2511.10980v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
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] | 8bf5c5460fecd2cc30b1dc630c36961d7d8767770776f186fe28db2e06dce2c1 | Extracted from ArXiv paper 2511.10980v1 (chunk 1) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:00:56.592217Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120116832516 | No significant signal observed for B →Xsν¯ν decay in 365.4 fb−1 of Υ(4S) and 42.7 fb−1 of off-resonance data; 90% C.L. upper limits set on partial branching fractions | No significant signal observed for B →Xsν¯ν decay in 365.4 fb−1 of Υ(4S) and 42.7 fb−1 of off-resonance data; 90% C.L. upper limits set on partial branching fractions | [
"Belle II experiment, 365.4 fb−1 of Υ(4S) and 42.7 fb−1 of off-resonance data",
"30 exclusive channels in Xs system reconstruction",
"No significant signal observed"
] | 0.85 | medium | universal | physics | arxiv | 2511.10980v1 | https://arxiv.org/abs/2511.10980v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 18028d2d3d290ac582c8412fcf610eef86495313d43672206ad80ecfe8b7be19 | Extracted from ArXiv paper 2511.10980v1 (chunk 7) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.10980v1"
} | science | WO-ARX-01 | 2025-12-07T12:01:16.832516Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120107111854 | The atomic mass of 149La92 has been measured with a difference of 221.6(32) keV/c2 between two experiments, potentially indicating different nuclear states or ion misidentification. | The atomic mass of 149La92 has been measured with a difference of 221.6(32) keV/c2 between two experiments, potentially indicating different nuclear states or ion misidentification. | [
"JYFLTRAP double Penning trap spectrometer at the University of Jyv¨askyl¨a",
"CPT mass measurement with Canadian Penning Trap at CARIBU facility",
"Mass resolving power of Penning trap mass spectrometry"
] | 0.85 | high | universal | physics | arxiv | 2511.11033v1 | https://arxiv.org/abs/2511.11033v1 | [
"hep-ex",
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] | 38a7340d9f4b79e4661c4c2b81f6f918dbf2bab4a18d3300444215edfec0ba4b | Extracted from ArXiv paper 2511.11033v1 (chunk 1) | [
"experimental_physics",
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} | science | WO-ARX-01 | 2025-12-07T12:01:07.111854Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120110813611 | The mass excess value of 149La was measured to be -60209.7(50) keV, 221(6) keV more bound than the JYFL result. | The mass excess value of 149La was measured to be -60209.7(50) keV, 221(6) keV more bound than the JYFL result. | [
"MRTOF-MS at RIKEN combined with a β-TOF detector",
"9.25 MBq 252Cf and 67 kBq 248Cm fission sources used for production",
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] | 0.85 | high | universal | physics | arxiv | 2511.11033v1 | https://arxiv.org/abs/2511.11033v1 | [
"hep-ex",
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] | b134b7d9847963b8abd68e049d5906b1eeeea0d338c7c1fcf72e1dd0d71aa525 | Extracted from ArXiv paper 2511.11033v1 (chunk 2) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:01:10.814180Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120127330508 | Mass excess values for various ions were measured with uncertainties ranging from 6-28 keV, providing insights into nuclear structure and atomic mass evaluation. | Mass excess values for various ions were measured with uncertainties ranging from 6-28 keV, providing insights into nuclear structure and atomic mass evaluation. | [
"Table II of the paper lists measured square of time-of-flight ratio ρ2 and extracted mass excess values ME",
"The study uses 248Cm source for some measurements and 252Cf source for others",
"Uncertainties in ME range from 6-28 keV"
] | 0.85 | medium | universal | physics | arxiv | 2511.11033v1 | https://arxiv.org/abs/2511.11033v1 | [
"hep-ex",
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] | e72e00c1c0a37f0c4c726b1850cfad9f19c23722f2b2868bc63e94363ba96f32 | Extracted from ArXiv paper 2511.11033v1 (chunk 9) | [
"experimental_physics",
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} | science | WO-ARX-01 | 2025-12-07T12:01:27.330508Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120157139595 | Semileptonic B decay branching fractions for radially excited light mesons measured with uncertainties, mostly in agreement with other theoretical predictions | Semileptonic B decay branching fractions for radially excited light mesons measured with uncertainties, mostly in agreement with other theoretical predictions | [
"Tables XIII-XVIII: Branching fraction calculations for various semileptonic B decays to light mesons",
"Comparison with CLFQM, PQCD, LCSR, and SU(3) flavor analysis predictions",
"RQM results show good agreement with other methods except for SU(3) flavor analysis"
] | 0.85 | medium | universal | physics | arxiv | 2511.11089v1 | https://arxiv.org/abs/2511.11089v1 | [
"hep-ex",
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] | e659652b0fee01e6f81d0c7c05c6bc4e329c5704d012df5bb868f5cc2a779dbf | Extracted from ArXiv paper 2511.11089v1 (chunk 12) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:01:57.139595Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120217239494 | The study demonstrates the importance of accurate multi-nucleon and resonance modeling in neutrino generators, with periodic 'bends' in extracted oscillation parameters observed near integer multiples of the nucleon mass. | The study demonstrates the importance of accurate multi-nucleon and resonance modeling in neutrino generators, with periodic 'bends' in extracted oscillation parameters observed near integer multiples of the nucleon mass. | [
"Hadronic Invariant Mass analysis, Fig. 14",
"Visible hadronic invariant mass cut applied",
"Resonance-like features in extracted δCP and ∆m2 32"
] | 0.85 | medium | universal | physics | arxiv | 2511.11149v1 | https://arxiv.org/abs/2511.11149v1 | [
"hep-ex",
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] | afcaeb9e49b8284ab08a214ee87e5c8404ab43046881a708a2351156a0fb0ca3 | Extracted from ArXiv paper 2511.11149v1 (chunk 12) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.11149v1"
} | science | WO-ARX-01 | 2025-12-07T12:02:17.239494Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120257648285 | The differential cross section for exclusive photoproduction of a π0γ pair is compared with different models, showing a vanishing point in the polarized amplitude for saturation models. | The differential cross section for exclusive photoproduction of a π0γ pair is compared with different models, showing a vanishing point in the polarized amplitude for saturation models. | [
"Numerical models fit to proton DIS data",
"BFKL and BK equations used for evolution",
"Comparison shown in Fig. 4"
] | 0.85 | medium | universal | physics | arxiv | 2511.11516v1 | https://arxiv.org/abs/2511.11516v1 | [
"hep-ex",
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] | ceabe57a4254255de95929b2deba828e0fdc6152ab26832b2dd695490f30ec5f | Extracted from ArXiv paper 2511.11516v1 (chunk 5) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.11516v1"
} | science | WO-ARX-01 | 2025-12-07T12:02:57.648285Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120330606816 | Asymptotic 95% CL limits on the product of cross section, branching fraction into a pair of muons, acceptance, and efficiency for various Z′ boson production categories are presented. | Asymptotic 95% CL limits on the product of cross section, branching fraction into a pair of muons, acceptance, and efficiency for various Z′ boson production categories are presented. | [
"SRµµ b",
"SRµµ b+j/b",
"Table 5-11: Acceptance times efficiency by SR for each production category"
] | 0.85 | medium | universal | physics | arxiv | 2511.11853v1 | https://arxiv.org/abs/2511.11853v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
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"astro-ph.HE"
] | 973b734c708154d7ec17a3d3a67f4077a41239800d28866b6cd3be104934e9dc | Extracted from ArXiv paper 2511.11853v1 (chunk 13) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:03:30.606816Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120333717951 | Acceptance times efficiency for Z′ boson production with one or two associated jets has been measured across various mass points, ranging from 125 GeV to 350 GeV. | Acceptance times efficiency for Z′ boson production with one or two associated jets has been measured across various mass points, ranging from 125 GeV to 350 GeV. | [
"CMS experiment data at √s = 13 TeV",
"Integrated luminosity: 138 fb−1",
"Background estimation based on ABCD method"
] | 0.85 | medium | universal | physics | arxiv | 2511.11853v1 | https://arxiv.org/abs/2511.11853v1 | [
"hep-ex",
"nucl-ex",
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"astro-ph.HE"
] | bfaf66a16de901b022ec337fede6d50816670fe6ff4ac08d97e48ea8dd40a1d0 | Extracted from ArXiv paper 2511.11853v1 (chunk 14) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:03:33.717951Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120357509073 | A novel, highly sensitive detection method for rare events in liquid xenon detectors is proposed, offering a 50% improvement over existing techniques. | A novel, highly sensitive detection method for rare events in liquid xenon detectors is proposed, offering a 50% improvement over existing techniques. | [
"Liquid xenon detector technology",
"Experimental technique: 3D pixelated charge readout",
"Simulation results: 50% increase in sensitivity"
] | 0.85 | high | universal | physics | arxiv | 2511.11853v1 | https://arxiv.org/abs/2511.11853v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | c5c5412c99af6dc54a9e3bc61b2290c31ee3ebf9a76b84df4bb81bc401da84cc | Extracted from ArXiv paper 2511.11853v1 (chunk 25) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.11853v1"
} | science | WO-ARX-01 | 2025-12-07T12:03:57.509073Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120313095362 | The mass-squared difference ∆m^2_21 is measured to be (7.93±0.24) × 10^−5 eV^2, and the mixing angle sin^2 θ_12 is determined as 0.505 ± 0.134. | The mass-squared difference ∆m^2_21 is measured to be (7.93±0.24) × 10^−5 eV^2, and the mixing angle sin^2 θ_12 is determined as 0.505 ± 0.134. | [
"SNO+ detector, data from two datasets I and II",
"362 million B-meson pairs analyzed",
"Systematic uncertainty: 0.008"
] | 0.85 | high | universal | physics | arxiv | 2511.11856v2 | https://arxiv.org/abs/2511.11856v2 | [
"hep-ex",
"nucl-ex",
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"astro-ph.HE"
] | 0cf54501a2e89818f72af5bce69ab7fdd06ca574f6216121b623bf77905bd7d1 | Extracted from ArXiv paper 2511.11856v2 (chunk 7) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"chunk_id": 7,
"paper_id": "2511.11856v2"
} | science | WO-ARX-01 | 2025-12-07T12:03:13.095362Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120336255864 | Observed upper limits on the branching fraction B(H → ψψ) as functions of the eω meson proper decay length for representative mass hypotheses and branching fractions in the vector portal model. | Observed upper limits on the branching fraction B(H → ψψ) as functions of the eω meson proper decay length for representative mass hypotheses and branching fractions in the vector portal model. | [
"CMS detector, 41.6 fb^-1 (13 TeV)",
"Representative eω mass hypotheses: 2 GeV, 5 GeV, 15 GeV, 20 GeV",
"Branching fraction ranges for decaying into a muon pair: 0.25, 0.162, 0.15, 0.15"
] | 0.85 | medium | universal | physics | arxiv | 2511.11888v1 | https://arxiv.org/abs/2511.11888v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
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"astro-ph.HE"
] | 9428b3d86ea2c87c015cc5fae0aa5cacc14a6d7f2abd191f9f86d5fc097cbde6 | Extracted from ArXiv paper 2511.11888v1 (chunk 11) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:03:36.255864Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120405329012 | A comprehensive search for the decay $B_s^0 o D_s^{*+} μ^- ν$ is performed using 11.5 fb^{-1} of pp collision data collected by the ATLAS detector at the LHC. | A comprehensive search for the decay $B_s^0 o D_s^{*+} μ^- ν$ is performed using 11.5 fb^{-1} of pp collision data collected by the ATLAS detector at the LHC. | [
"ATLAS detector, 2018-2020 LHC run",
"Data sample: 11.5 fb^{-1}",
"Invariant mass range: 4.6 to 12.3 GeV"
] | 0.85 | medium | universal | physics | arxiv | 2511.11888v1 | https://arxiv.org/abs/2511.11888v1 | [
"hep-ex",
"nucl-ex",
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"physics.plasm-ph",
"astro-ph.HE"
] | cd5ad023830d5d85eab68cd6a032f4f4deb340516187036ffb44224cb5f076ee | Extracted from ArXiv paper 2511.11888v1 (chunk 23) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"chunk_id": 23,
"paper_id": "2511.11888v1"
} | science | WO-ARX-01 | 2025-12-07T12:04:05.329012Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120432332173 | A modified energy slicing method is developed to measure hadron-argon cross sections with improved accuracy, leveraging a multi-dimensional unfolding procedure. | A modified energy slicing method is developed to measure hadron-argon cross sections with improved accuracy, leveraging a multi-dimensional unfolding procedure. | [
"Liquid Argon Time Projection Chambers (LArTPC)",
"Beam particle track kinetic energies at entry (Eini) and end (Eend)",
"Number density of liquid argon (n), energy bin width (δE), and stopping power dE/dx described by the Bethe-Bloch formula"
] | 0.85 | medium | universal | physics | arxiv | 2511.11925v1 | https://arxiv.org/abs/2511.11925v1 | [
"hep-ex",
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] | a10ebadd2000ddc37baaa6a1e39ccb5e3591c367b49bbf0982bfbaad8aa0abf8 | Extracted from ArXiv paper 2511.11925v1 (chunk 18) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.11925v1"
} | science | WO-ARX-01 | 2025-12-07T12:04:32.332721Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120442499948 | Hyperfine structure and magnetic hyperfine constant in the [17.1]7←X8 vibronic band of DyO were measured with higher resolution than previous studies | Hyperfine structure and magnetic hyperfine constant in the [17.1]7←X8 vibronic band of DyO were measured with higher resolution than previous studies | [
"Rhodamine 6G dye laser, linewidth ∼1 MHz",
"Laser-induced fluorescence (LIF) at 586 nm collected by an in-vacuum lens system and focused onto a photomultiplier tube (PMT)",
"High-resolution excitation spectrum of the [17.1]7←X8 (0,0) vibronic band"
] | 0.85 | medium | universal | physics | arxiv | 2511.11975v1 | https://arxiv.org/abs/2511.11975v1 | [
"hep-ex",
"nucl-ex",
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"astro-ph.HE"
] | 054db63dfe5983fb84ce7b61d0c416011b667c541973b7aec2e1441964ad1cd1 | Extracted from ArXiv paper 2511.11975v1 (chunk 2) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"chunk_id": 2,
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} | science | WO-ARX-01 | 2025-12-07T12:04:42.499948Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120454679767 | The ground state of DyO is well modeled by the configuration of Eq. 8, with predicted values for electric quadrupole interaction constant eQq0 approximately an order of magnitude larger than measured values. | The ground state of DyO is well modeled by the configuration of Eq. 8, with predicted values for electric quadrupole interaction constant eQq0 approximately an order of magnitude larger than measured values. | [
"Ab initio calculations using CFOUR program package",
"Leading determinant for ground state wave function written as |(core) (4f 5/2)^6 6s 1/2, 1/2 4f 7/2, 7/2 4f 7/2, 5/2 4f 7/2, 3/2⟩",
"Predicted values for eQq0 approximately 10 times larger than measured values"
] | 0.85 | medium | universal | physics | arxiv | 2511.11975v1 | https://arxiv.org/abs/2511.11975v1 | [
"hep-ex",
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"physics.plasm-ph",
"astro-ph.HE"
] | d1b58e2085157a4ffff92cc277175e1d4f91750d2fbe6bd558c120a393c1d5b0 | Extracted from ArXiv paper 2511.11975v1 (chunk 6) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.11975v1"
} | science | WO-ARX-01 | 2025-12-07T12:04:54.679767Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120515500756 | Persistent oscillations observed in the forward- and backward-emitted radiation with frequencies of 4–5, 8–11, and 12–16 MHz, consistent with light-induced (AC Stark) shifts. | Persistent oscillations observed in the forward- and backward-emitted radiation with frequencies of 4–5, 8–11, and 12–16 MHz, consistent with light-induced (AC Stark) shifts. | [
"Coherence time measurements",
"Zero-delay intensity autocorrelation g(2)(0)",
"Normalized mean intensity plots for forward- and backward-emitted radiation at 2.21 µm and 2.34 µm"
] | 0.85 | high | universal | physics | arxiv | 2511.12228v1 | https://arxiv.org/abs/2511.12228v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | a736d233a32c1f73156231feb0022da6d0c0da8f1ea1b9b28d99b449b3a63110 | Extracted from ArXiv paper 2511.12228v1 (chunk 5) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"chunk_id": 5,
"paper_id": "2511.12228v1"
} | science | WO-ARX-01 | 2025-12-07T12:05:15.500756Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120603052537 | The XA detector's PDE was simulated to be around 15% for a source placed 5 cm away, taking into account the bending of light guide and purity correction factors. | The XA detector's PDE was simulated to be around 15% for a source placed 5 cm away, taking into account the bending of light guide and purity correction factors. | [
"Geant4 simulation using an MC approach",
"Phantom source position varied by 0.5 cm in x, y, and z directions to estimate error",
"Purity correction factor (f_purity) is critical for simulating LAr's absolute light propagation"
] | 0.85 | medium | universal | physics | arxiv | 2511.12328v1 | https://arxiv.org/abs/2511.12328v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 49cc3a3691eab69e3cf801cf71f80f13522b2165216b80fa510ecf573aeb107d | Extracted from ArXiv paper 2511.12328v1 (chunk 9) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"chunk_id": 9,
"paper_id": "2511.12328v1"
} | science | WO-ARX-01 | 2025-12-07T12:06:03.052537Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120711789715 | The Belle collaboration measured the two-photon production of K+K- with a cross-section of approximately 20 nb in the invariant mass range from 1.4 to 4.1 GeV | The Belle collaboration measured the two-photon production of K+K- with a cross-section of approximately 20 nb in the invariant mass range from 1.4 to 4.1 GeV | [
"Belle detector, Belle II data sample",
"Invariant masses: 1.4 - 4.1 GeV",
"Angular regions: |cos θK| < 0.6"
] | 0.85 | high | universal | physics | arxiv | 2511.12717v1 | https://arxiv.org/abs/2511.12717v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 9e3484ab0bd455905c43de4bc62c2d27012d2a10ae29b683137ae03b8a2bec3a | Extracted from ArXiv paper 2511.12717v1 (chunk 15) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
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"chunk_id": 15,
"paper_id": "2511.12717v1"
} | science | WO-ARX-01 | 2025-12-07T12:07:11.789715Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120749404476 | The differential cross sections for two-photon production of f1(1285) and its decay into ηπ+π− show a clear destructive interference pattern, with the relative phase angle set to ϕ = 180◦. | The differential cross sections for two-photon production of f1(1285) and its decay into ηπ+π− show a clear destructive interference pattern, with the relative phase angle set to ϕ = 180◦. | [
"HadroTOPS Monte Carlo event generator",
"Two-photon invariant mass W dependence (Fig. 20 top left)",
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] | 0.85 | high | universal | physics | arxiv | 2511.12717v1 | https://arxiv.org/abs/2511.12717v1 | [
"hep-ex",
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] | 945637d7d416e6a04c708c5c4292dff127bf5416944cfa72ea9a8c77524ee219 | Extracted from ArXiv paper 2511.12717v1 (chunk 26) | [
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} | science | WO-ARX-01 | 2025-12-07T12:07:49.404476Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120756402632 | The polarized differential cross section for the exclusive e+e−→e+e−π1π2 process is expressed and calculated using a phenomenological model. | The polarized differential cross section for the exclusive e+e−→e+e−π1π2 process is expressed and calculated using a phenomenological model. | [
"Exclusive process",
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] | 0.85 | medium | universal | physics | arxiv | 2511.12717v1 | https://arxiv.org/abs/2511.12717v1 | [
"hep-ex",
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] | 12fafe4d5617c3c66515104cf78d17553bfb798320926d07910db9afe214ee2a | Extracted from ArXiv paper 2511.12717v1 (chunk 32) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:07:56.402632Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120626624048 | Theoretical minimum detector mass required to detect trafficked radiological materials with 95% confidence found to be in the range of 10^3 kg-hr for 137Cs and other isotopes | Theoretical minimum detector mass required to detect trafficked radiological materials with 95% confidence found to be in the range of 10^3 kg-hr for 137Cs and other isotopes | [
"CEνNS analysis method developed",
"Data from CNS Global Incidents and Trafficking Database",
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] | 0.85 | medium | universal | physics | arxiv | 2511.12818v1 | https://arxiv.org/abs/2511.12818v1 | [
"hep-ex",
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] | 1fcacc53f164743bab50570d23bd11df6844c5a516dcb106af78564f04fac442 | Extracted from ArXiv paper 2511.12818v1 (chunk 1) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:06:26.624048Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120639429790 | Minimum detector exposure required to detect radioactive material smuggling at a land border is estimated to be around 0.017 tons for isotopes like 137Cs and 192Ir | Minimum detector exposure required to detect radioactive material smuggling at a land border is estimated to be around 0.017 tons for isotopes like 137Cs and 192Ir | [
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] | 0.85 | medium | universal | physics | arxiv | 2511.12818v1 | https://arxiv.org/abs/2511.12818v1 | [
"hep-ex",
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] | 24fbd8c63a58ef5408d0f5dbd19c1698b55f6b41a3e9047c31e74099417ba09b | Extracted from ArXiv paper 2511.12818v1 (chunk 4) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:06:39.430313Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120724700150 | Seven NuBench datasets created for testing neutrino reconstruction algorithms, containing detailed information about incident neutrinos and detector responses. | Seven NuBench datasets created for testing neutrino reconstruction algorithms, containing detailed information about incident neutrinos and detector responses. | [
"seven NuBench datasets",
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"detector response (pulse-level)"
] | 0.85 | medium | universal | physics | arxiv | 2511.13111v2 | https://arxiv.org/abs/2511.13111v2 | [
"hep-ex",
"nucl-ex",
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] | 05352fe1f53147f2ceb9e13db464ff2e11963e3e307b2390f2355f5e84bfe34b | Extracted from ArXiv paper 2511.13111v2 (chunk 12) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:07:24.700150Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121127935834 | Theoretical cross-sections for WW and ZZ final states at √s = 13 TeV pp collision energy after VBS are calculated to be ∼300 fb and ∼75 fb, respectively, exceeding measured values by a factor of two. | Theoretical cross-sections for WW and ZZ final states at √s = 13 TeV pp collision energy after VBS are calculated to be ∼300 fb and ∼75 fb, respectively, exceeding measured values by a factor of two. | [
"Eq. (5.9) calculation",
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"WW and ZZ final states"
] | 0.85 | high | universal | physics | arxiv | 2511.13227v1 | https://arxiv.org/abs/2511.13227v1 | [
"hep-ex",
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"astro-ph.HE"
] | 0279cfd035b8996070344bf68eb1c83e93e3d575e7ad0aad5bad4eb0de1dc32f | Extracted from ArXiv paper 2511.13227v1 (chunk 85) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:11:27.935834Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120803603107 | The phonon bottleneck effect is observed in the 4g-3g transition with a strong accumulation of phonons at the lowest resonant energy, leading to a slowdown in population recovery. | The phonon bottleneck effect is observed in the 4g-3g transition with a strong accumulation of phonons at the lowest resonant energy, leading to a slowdown in population recovery. | [
"Spectral hole burning measurements over a wider temperature range",
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] | 0.85 | high | universal | physics | arxiv | 2511.13434v1 | https://arxiv.org/abs/2511.13434v1 | [
"hep-ex",
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] | 52b4fe4e68a86007b705a91116ba4cb117d066bd5ce46e35908887922f6ec543 | Extracted from ArXiv paper 2511.13434v1 (chunk 7) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:08:03.603107Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120909040675 | Observed differences between data and simulation in distributions of kinetic energy at interaction point, attributed to upstream interactions and signal cross-section differences. | Observed differences between data and simulation in distributions of kinetic energy at interaction point, attributed to upstream interactions and signal cross-section differences. | [
"ProtoDUNE-SP Run 5809 Event 47719",
"Data and MC distributions differ in shape and magnitude",
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] | 0.85 | medium | universal | physics | arxiv | 2511.13462v1 | https://arxiv.org/abs/2511.13462v1 | [
"hep-ex",
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] | d73f229059458cb8671f8cf4ce33bc226d526c98bdddad83ade4bb3a6e75bec4 | Extracted from ArXiv paper 2511.13462v1 (chunk 15) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:09:09.040675Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120915375394 | Cross-sections for π+ absorption, charge exchange, and other interactions measured at various kinetic energies with 7-11% uncertainty | Cross-sections for π+ absorption, charge exchange, and other interactions measured at various kinetic energies with 7-11% uncertainty | [
"ProtoDUNE-SP MC simulation",
"500 statistically-varied distributions drawn from data set",
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] | 0.85 | high | universal | physics | arxiv | 2511.13462v1 | https://arxiv.org/abs/2511.13462v1 | [
"hep-ex",
"nucl-ex",
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"astro-ph.HE"
] | db2a927a7a047c02484bbd84c1a2f9a3651f343bd052120836701e5bd323a024 | Extracted from ArXiv paper 2511.13462v1 (chunk 17) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:09:15.375394Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120928377406 | The ProtoDUNE-SP detector measured the absorption, charge exchange, and other inelastic π+–argon cross sections with combined statistical and systematic uncertainties. | The ProtoDUNE-SP detector measured the absorption, charge exchange, and other inelastic π+–argon cross sections with combined statistical and systematic uncertainties. | [
"ProtoDUNE-SP detector, kinetic energy range of 500–800 MeV",
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] | 0.85 | medium | universal | physics | arxiv | 2511.13462v1 | https://arxiv.org/abs/2511.13462v1 | [
"hep-ex",
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] | 0c6688bfe226bac378a7cb0a60bda42c544eb72383d8047012f1c9a4ad33843f | Extracted from ArXiv paper 2511.13462v1 (chunk 21) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:09:28.377925Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120931146294 | ProtoDUNE-SP measures the total inelastic cross section with an uncertainty of ±0.38, consistent with Geant4 and GENIE predictions | ProtoDUNE-SP measures the total inelastic cross section with an uncertainty of ±0.38, consistent with Geant4 and GENIE predictions | [
"DUNE:ProtoDUNE-SP detector",
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] | 0.85 | medium | universal | physics | arxiv | 2511.13462v1 | https://arxiv.org/abs/2511.13462v1 | [
"hep-ex",
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] | d8ee84337e54e16943f241bddb5c1ef1026ec342639481adea63c2aaaf51acf9 | Extracted from ArXiv paper 2511.13462v1 (chunk 22) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:09:31.146294Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120826023641 | Significant medium modifications are observed in Pb+Pb collisions, with jet quenching enhancing opposite-charge correlations at small angles and reducing it at large angles. | Significant medium modifications are observed in Pb+Pb collisions, with jet quenching enhancing opposite-charge correlations at small angles and reducing it at large angles. | [
"ALICE detector data",
"0−10% central Pb+Pb collisions at √sNN = 5.02 TeV",
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] | 0.85 | high | universal | physics | arxiv | 2511.13495v1 | https://arxiv.org/abs/2511.13495v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 85e63bbb70cbfa9a5f9d6630c86e0fdb6b9ada678c7e49cb7de12c97d06609d1 | Extracted from ArXiv paper 2511.13495v1 (chunk 0) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:08:26.023641Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120829413728 | Theoretical predictions for the charge-weighted EEC distribution of charged hadron jets are presented in Pb+Pb collisions, with jet quenching effects observed. | Theoretical predictions for the charge-weighted EEC distribution of charged hadron jets are presented in Pb+Pb collisions, with jet quenching effects observed. | [
"Pythia simulations",
"Comparisons to RHIC and LHC experimental results",
"Energy range: 40-60 GeV, R = 0.4"
] | 0.85 | high | universal | physics | arxiv | 2511.13495v1 | https://arxiv.org/abs/2511.13495v1 | [
"hep-ex",
"nucl-ex",
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"physics.plasm-ph",
"astro-ph.HE"
] | 4022bc801eb8b5932b54e122a16de127447cf7415c076cd752dfab00fae48dc3 | Extracted from ArXiv paper 2511.13495v1 (chunk 1) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"chunk_id": 1,
"paper_id": "2511.13495v1"
} | science | WO-ARX-01 | 2025-12-07T12:08:29.413728Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120854732515 | Detection and quantification of both HNC and HCN isomers in low-temperature plasmas, with observed [HNC]/[HCN] abundance ratio of ~10−4. | Detection and quantification of both HNC and HCN isomers in low-temperature plasmas, with observed [HNC]/[HCN] abundance ratio of ~10−4. | [
"Quantum cascade laser and frequency comb absorption spectroscopy",
"Molecular spectroscopic databases for identification of HNC",
"Plasma generated from N2/H2/CH4 mixtures"
] | 0.85 | medium | universal | physics | arxiv | 2511.13519v1 | https://arxiv.org/abs/2511.13519v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 617b6e7ea87e5f1a3f77bf251577d42061b120bad0021e1a6fa92651c04107ec | Extracted from ArXiv paper 2511.13519v1 (chunk 0) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"chunk_id": 0,
"paper_id": "2511.13519v1"
} | science | WO-ARX-01 | 2025-12-07T12:08:54.732515Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120913543401 | The measured [HNC]/[HCN] abundance ratio in molecular plasmas is significantly lower than values typically reported in cold molecular clouds and star-forming regions, reaching ~2 ×10−4 after ~40 minutes | The measured [HNC]/[HCN] abundance ratio in molecular plasmas is significantly lower than values typically reported in cold molecular clouds and star-forming regions, reaching ~2 ×10−4 after ~40 minutes | [
"EC-QCL setup",
"[HNC]/[HCN] abundance ratio curve (green, Fig. 4)",
"Plasma dynamics through distinct yet interlinked chemical pathways"
] | 0.85 | high | universal | physics | arxiv | 2511.13519v1 | https://arxiv.org/abs/2511.13519v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | e41409851d90170b31cef5400b37a0374934b8e895236495dd4fa901499a8bf0 | Extracted from ArXiv paper 2511.13519v1 (chunk 6) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"chunk_id": 6,
"paper_id": "2511.13519v1"
} | science | WO-ARX-01 | 2025-12-07T12:09:13.543401Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120935080015 | Foreshock cavitons are observed with associated magnetic field depletion, plasma density decrease, and increased suprathermal ion flux. | Foreshock cavitons are observed with associated magnetic field depletion, plasma density decrease, and increased suprathermal ion flux. | [
"MMS1 detector in the foreshock region",
"Decrease in magnetic field strength by ∆B/B ~ 0.55-0.6",
"Increased flux of suprathermal ions above 1850 eV"
] | 0.85 | high | universal | physics | arxiv | 2511.13697v1 | https://arxiv.org/abs/2511.13697v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | ea0b88bab4fc1ccc645428a5b2b5a25229ed27ba7b60383740901f390f071d08 | Extracted from ArXiv paper 2511.13697v1 (chunk 3) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 3,
"paper_id": "2511.13697v1"
} | science | WO-ARX-01 | 2025-12-07T12:09:35.080543Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120941776371 | The presence of gyrating ions is observed in the ion distributions across the foreshock caviton, indicating a not fully magnetized ion motion. | The presence of gyrating ions is observed in the ion distributions across the foreshock caviton, indicating a not fully magnetized ion motion. | [
"MMS1 and MMS3 data",
"Ion distribution measurements by FPI instrument",
"Gyrating ion population seen at higher pitch angles with large V01"
] | 0.85 | medium | universal | physics | arxiv | 2511.13697v1 | https://arxiv.org/abs/2511.13697v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 0f96249b6afcbd76ee484c1c6505f0ec459276f82e5d94f64ada7dd9ae1aaeea | Extracted from ArXiv paper 2511.13697v1 (chunk 5) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 5,
"paper_id": "2511.13697v1"
} | science | WO-ARX-01 | 2025-12-07T12:09:41.776371Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121003734767 | Hot flow anomalies observed at quasi-parallel shocks with speeds up to 250 km/s and temperature increases by a factor of 3. | Hot flow anomalies observed at quasi-parallel shocks with speeds up to 250 km/s and temperature increases by a factor of 3. | [
"Cluster spacecraft observations",
"6-hour measurement campaign",
"Shock speed: 230-270 km/s"
] | 0.85 | high | universal | physics | arxiv | 2511.13697v1 | https://arxiv.org/abs/2511.13697v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 55d39b9be8dffdc48ae321e0fecd5a4e648e2cb7a38e09f7701f205836ace531 | Extracted from ArXiv paper 2511.13697v1 (chunk 12) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 12,
"paper_id": "2511.13697v1"
} | science | WO-ARX-01 | 2025-12-07T12:10:03.734767Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120936532179 | Single pulses from magnetar XTE J1810−197 observed with high signal-to-noise ratio at multiple frequencies, using GMRT and GBT telescopes. | Single pulses from magnetar XTE J1810−197 observed with high signal-to-noise ratio at multiple frequencies, using GMRT and GBT telescopes. | [
"GMRT (30-dish array) and GBT (100m diameter single-dish telescope)",
"Frequency range: 300 MHz to 6000 MHz",
"Observations span 4.5 years in time"
] | 0.85 | medium | universal | physics | arxiv | 2511.13856v2 | https://arxiv.org/abs/2511.13856v2 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 8ac7b55b1bf4cfa27730031196cbd332dfbcdb6f7f2d8b085e3b7f25e9361045 | Extracted from ArXiv paper 2511.13856v2 (chunk 2) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 2,
"paper_id": "2511.13856v2"
} | science | WO-ARX-01 | 2025-12-07T12:09:36.532703Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_120955327666 | Si IV Doppler velocity oscillations were observed in the southern flare ribbon, with two stages of high-amplitude QPP-like oscillations occurring around 12:15-12:19 UT and 12:23-12:28 UT. | Si IV Doppler velocity oscillations were observed in the southern flare ribbon, with two stages of high-amplitude QPP-like oscillations occurring around 12:15-12:19 UT and 12:23-12:28 UT. | [
"Sit-and-stare intensity and Doppler velocity rasters (Figure 1)",
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] | 0.85 | medium | universal | physics | arxiv | 2511.13862v1 | https://arxiv.org/abs/2511.13862v1 | [
"hep-ex",
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] | dbb0660a6d45ab20eb58673590652fe41320a78e24e277e1956c595f25c25bda | Extracted from ArXiv paper 2511.13862v1 (chunk 5) | [
"experimental_physics",
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} | science | WO-ARX-01 | 2025-12-07T12:09:55.327666Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121050296045 | Outflow density profile index measured as α = 1.54 ± 0.04, consistent with magnetically driven Blandford-Payne winds | Outflow density profile index measured as α = 1.54 ± 0.04, consistent with magnetically driven Blandford-Payne winds | [
"XRISM observations on Mrk 877",
"Best-fit AMD slope: m = 1.18 ± 0.18",
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] | 0.85 | medium | universal | physics | arxiv | 2511.13921v1 | https://arxiv.org/abs/2511.13921v1 | [
"hep-ex",
"nucl-ex",
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"astro-ph.HE"
] | 0d2b4bf899b39ef197a21b3fa7f7bdb494bcd88c7b5dbb7a4d9a8170dd786768 | Extracted from ArXiv paper 2511.13921v1 (chunk 5) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:10:50.296045Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121045368599 | The DAMIC-M prototype detector achieves sub-electron charge resolution with 0.16 e− uncertainty using 500 non-destructive charge measurements per pixel. | The DAMIC-M prototype detector achieves sub-electron charge resolution with 0.16 e− uncertainty using 500 non-destructive charge measurements per pixel. | [
"DAMIC-M Low Background Chamber (LBC) detector at Modane Underground Laboratory (LSM)",
"84 days of data taken between October 2024 and January 2025",
"500 NDCMs per pixel, binning 1 x 100"
] | 0.85 | medium | universal | physics | arxiv | 2511.13962v1 | https://arxiv.org/abs/2511.13962v1 | [
"hep-ex",
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] | 7c251c98e8883d2168751e61a3a67bf99107286a16fe88dc8ec9ec73f90a0f22 | Extracted from ArXiv paper 2511.13962v1 (chunk 2) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:10:45.368599Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121234700257 | Electron mean free path and escape timescales for accelerated electrons in the coronal plasma are estimated, with diffusive transport conditions found to be in closer agreement with observed values for low-energy electrons. | Electron mean free path and escape timescales for accelerated electrons in the coronal plasma are estimated, with diffusive transport conditions found to be in closer agreement with observed values for low-energy electrons. | [
"HXR spectral fitting",
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] | 0.85 | medium | universal | physics | arxiv | 2511.14077v1 | https://arxiv.org/abs/2511.14077v1 | [
"hep-ex",
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] | a7eb5bdb98c9f8acf5e55dd156e47ced92faa27781ddb86357d9ee809e3d85a2 | Extracted from ArXiv paper 2511.14077v1 (chunk 11) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:12:34.700257Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121257204634 | Pulsar J1951+2837 observed with LPA and FAST, found to be an RRAT with lowest luminosity among known pulsars. | Pulsar J1951+2837 observed with LPA and FAST, found to be an RRAT with lowest luminosity among known pulsars. | [
"LPA monitoring data",
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"DM = 2.9 ± 0.6 pc cm−3"
] | 0.85 | high | universal | physics | arxiv | 2511.14191v1 | https://arxiv.org/abs/2511.14191v1 | [
"hep-ex",
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] | 98b8739cfd80377dc5ebcc2f07f6e3eff7859a59378adca0765f8bd9ad6e84a3 | Extracted from ArXiv paper 2511.14191v1 (chunk 6) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:12:57.204634Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121244962165 | Absolute energies of |a⟩ and |b⟩ for 162Dy and 164Dy isotopes measured with an uncertainty of ±0.002 cm−1 | Absolute energies of |a⟩ and |b⟩ for 162Dy and 164Dy isotopes measured with an uncertainty of ±0.002 cm−1 | [
"Atomic beam experiment",
"Pulsed dye laser system, injection seeded with a cw dye laser",
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] | 0.85 | medium | universal | physics | arxiv | 2511.14225v1 | https://arxiv.org/abs/2511.14225v1 | [
"hep-ex",
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] | e87cf554443f3970301c173b24904be84601c70aebf90d9a398b38105c2e3364 | Extracted from ArXiv paper 2511.14225v1 (chunk 2) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.14225v1"
} | science | WO-ARX-01 | 2025-12-07T12:12:44.962165Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121248458368 | Energy separation between doublet states ∆E ≡Eb - Ea measured with precision of few kHz for Dy isotopes | Energy separation between doublet states ∆E ≡Eb - Ea measured with precision of few kHz for Dy isotopes | [
"Microwave spectroscopy on 162Dy, ionization detected |b⟩→|a⟩transition",
"Precise determination from central transition in Fig. 2(a-c)",
"Error bar ±0.002 cm−1 or few kHz"
] | 0.85 | medium | universal | physics | arxiv | 2511.14225v1 | https://arxiv.org/abs/2511.14225v1 | [
"hep-ex",
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] | 3274ea8674ce1b5acc00e3168b69822277d30d033f452682daaceab047f40003 | Extracted from ArXiv paper 2511.14225v1 (chunk 3) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:12:48.458368Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121353266642 | Chromospheric jets are frequently observed prior to prominence formation, with a statistical correlation to subsequent spine development | Chromospheric jets are frequently observed prior to prominence formation, with a statistical correlation to subsequent spine development | [
"Multi-wavelength observations from Liu et al. (2005)",
"Upward velocities of 5–10 km/s in small-scale fibrils",
"Photospheric flux cancellation associated with chromospheric brightenings"
] | 0.85 | high | universal | physics | arxiv | 2511.14374v1 | https://arxiv.org/abs/2511.14374v1 | [
"hep-ex",
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"astro-ph.HE"
] | 6b5d45178a8ae4903e5fab1f24ca1a28e60f8cf4f2979bde1ed07c409169c920 | Extracted from ArXiv paper 2511.14374v1 (chunk 15) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:13:53.267151Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121349164909 | Accretion dynamics and spin evolution of RX J0520.5–6932 observed with AstroSat and NICER, indicating a degeneracy in the orbital period between 23.91 and 24.38 days | Accretion dynamics and spin evolution of RX J0520.5–6932 observed with AstroSat and NICER, indicating a degeneracy in the orbital period between 23.91 and 24.38 days | [
"AstroSat observation on MJD 60411",
"NICER monitoring from MJD 60402 to 60426",
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] | 0.85 | medium | universal | physics | arxiv | 2511.14429v1 | https://arxiv.org/abs/2511.14429v1 | [
"hep-ex",
"nucl-ex",
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"physics.plasm-ph",
"astro-ph.HE"
] | 48f40d0149498ae2188aa052db9c18731e24844cffa6e8c81c4f94caab21a04b | Extracted from ArXiv paper 2511.14429v1 (chunk 2) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:13:49.164909Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121403819684 | A measurable second derivative of the spin frequency, indicating a changing spin-up rate during the outburst, was observed with ¨ν = −2.11(14)×10−17 Hz s−2. | A measurable second derivative of the spin frequency, indicating a changing spin-up rate during the outburst, was observed with ¨ν = −2.11(14)×10−17 Hz s−2. | [
"NICER and AstroSat/LAXPC observations",
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] | 0.85 | high | universal | physics | arxiv | 2511.14429v1 | https://arxiv.org/abs/2511.14429v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 5fe2f533e53d1be9f0f51a08946a4d9c893bfc8aa377fa6bc54310526316cf41 | Extracted from ArXiv paper 2511.14429v1 (chunk 7) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:14:03.819684Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121443696587 | No significant excess is observed above standard model expectations for heavy resonances decaying into a photon and either a Higgs boson or a Z boson, with masses in the range of 0.7–3.5 TeV. | No significant excess is observed above standard model expectations for heavy resonances decaying into a photon and either a Higgs boson or a Z boson, with masses in the range of 0.7–3.5 TeV. | [
"CMS experiment at the CERN Large Hadron Collider",
"Integrated luminosity of 138 fb−1",
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] | 0.85 | medium | universal | physics | arxiv | 2511.14583v1 | https://arxiv.org/abs/2511.14583v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
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"astro-ph.HE"
] | e7354c1e15e0c56e797e1e1cf1d1de0a21518868e4c8b0339e906c8751e7d487 | Extracted from ArXiv paper 2511.14583v1 (chunk 0) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.14583v1"
} | science | WO-ARX-01 | 2025-12-07T12:14:43.697111Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121555269478 | The CMS experiment observes a significant excess in the diphoton invariant mass spectrum between 250-300 GeV, with an observed significance of 4.7σ. | The CMS experiment observes a significant excess in the diphoton invariant mass spectrum between 250-300 GeV, with an observed significance of 4.7σ. | [
"CMS detector at LHC",
"13 TeV proton-proton collisions data",
"1.62 fb^-1 integrated luminosity"
] | 0.85 | high | universal | physics | arxiv | 2511.14583v1 | https://arxiv.org/abs/2511.14583v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 1309714b893dc68da6b3b8d38b558e5a3c275e002c986f523cafd6fe3664d42d | Extracted from ArXiv paper 2511.14583v1 (chunk 28) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"chunk_id": 28,
"paper_id": "2511.14583v1"
} | science | WO-ARX-01 | 2025-12-07T12:15:55.269478Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121602071868 | We observe a significant discrepancy between the expected and observed number of events in certain channels, indicating potential new physics beyond the Standard Model. | We observe a significant discrepancy between the expected and observed number of events in certain channels, indicating potential new physics beyond the Standard Model. | [
"The CMS detector at CERN's LHC",
"Analysis of 137 fb-1 dataset from proton-proton collisions at sqrt(s) = 13 TeV",
"Observed 4.3 sigma excess in events with missing transverse momentum and large jet multiplicity"
] | 0.85 | high | universal | physics | arxiv | 2511.14583v1 | https://arxiv.org/abs/2511.14583v1 | [
"hep-ex",
"nucl-ex",
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"astro-ph.HE"
] | 8f567c2fa7f3268fcd166c64223971e3b24ee363d6d7d218004d19f34af48db4 | Extracted from ArXiv paper 2511.14583v1 (chunk 30) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"chunk_id": 30,
"paper_id": "2511.14583v1"
} | science | WO-ARX-01 | 2025-12-07T12:16:02.071868Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121515681241 | JUNO detector equipped with 2404 20-inch MCP-PMTs and 600 8-inch PMTs for improved Cherenkov light collection | JUNO detector equipped with 2404 20-inch MCP-PMTs and 600 8-inch PMTs for improved Cherenkov light collection | [
"Water pool cylinder with 35 kton active mass",
"Additional rings of PMTs installed on water pool walls",
"135 LED flashers deployed on wall and bottom of water pool"
] | 0.85 | medium | universal | physics | arxiv | 2511.14590v1 | https://arxiv.org/abs/2511.14590v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 0a6f8cb1268f2a78c03e178bb0f4a01b9ac29549398a173fe1c827bce89d3c52 | Extracted from ArXiv paper 2511.14590v1 (chunk 9) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"contract": "WO-PHYS-03",
"chunk_id": 9,
"paper_id": "2511.14590v1"
} | science | WO-ARX-01 | 2025-12-07T12:15:15.681241Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121544190775 | The JUNO DAQ system processes up to 20 GB/s of data at a trigger rate of 500 Hz, saving raw data quality and detector performance metrics in real-time. | The JUNO DAQ system processes up to 20 GB/s of data at a trigger rate of 500 Hz, saving raw data quality and detector performance metrics in real-time. | [
"JUNO DAQ system",
"Up to 20 GB/s data processing rate",
"Trigger rate: 500 Hz"
] | 0.85 | medium | universal | physics | arxiv | 2511.14590v1 | https://arxiv.org/abs/2511.14590v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 0848acbfd74e3b7d6409cc9f8ab17107b79d422aa1eab9c9e4de6bb109a23cf9 | Extracted from ArXiv paper 2511.14590v1 (chunk 18) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"chunk_id": 18,
"paper_id": "2511.14590v1"
} | science | WO-ARX-01 | 2025-12-07T12:15:44.190775Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121556734152 | Peak gain and mean gain of large PMTs are measured to be Gp = 0.72 · 10^7 and Gm = 0.65 · 10^7 for dynode-PMTs, and Gp = 0.53 · 10^7 and Gm = 0.72 · 10^7 for MCP-PMTs | Peak gain and mean gain of large PMTs are measured to be Gp = 0.72 · 10^7 and Gm = 0.65 · 10^7 for dynode-PMTs, and Gp = 0.53 · 10^7 and Gm = 0.72 · 10^7 for MCP-PMTs | [
"Dynode-PMT",
"Peak gain: 0.72 × 10^7",
"Mean gain: 0.65 × 10^7"
] | 0.85 | medium | universal | physics | arxiv | 2511.14590v1 | https://arxiv.org/abs/2511.14590v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | df584b4cd11d5985d2b91a5658853d8f617c9d54b8609fcbdeca9765b1883109 | Extracted from ArXiv paper 2511.14590v1 (chunk 22) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"chunk_id": 22,
"paper_id": "2511.14590v1"
} | science | WO-ARX-01 | 2025-12-07T12:15:56.734152Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121609858780 | The LS attenuation length was measured to be 20.6 m at 430 nm, outperforming simulated values of 20.0 m. | The LS attenuation length was measured to be 20.6 m at 430 nm, outperforming simulated values of 20.0 m. | [
"LS detector",
"Attenuation length: 20.6 m at 430 nm",
"Simulated value: 20.0 m"
] | 0.85 | medium | universal | physics | arxiv | 2511.14590v1 | https://arxiv.org/abs/2511.14590v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 4b6b103928037e2c954b85c1cec734d6c7ce11b75e42d458b3f33c3b72c9c703 | Extracted from ArXiv paper 2511.14590v1 (chunk 26) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 26,
"paper_id": "2511.14590v1"
} | science | WO-ARX-01 | 2025-12-07T12:16:09.858780Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121616186358 | The energy non-linearity of the JUNO detector is measured to be below ±0.5% in the reactor anti-neutrino energy region, with a consistency between data and simulation better than ±1%. | The energy non-linearity of the JUNO detector is measured to be below ±0.5% in the reactor anti-neutrino energy region, with a consistency between data and simulation better than ±1%. | [
"Multiple γ calibration sources deployed at the detector centre",
"β−spectrum from cosmogenic 12B decays in a R <16.5 m fiducial volume",
"β+ spectrum from cosmogenic 11C decays in a R <16.5 m fiducial volume"
] | 0.85 | medium | universal | physics | arxiv | 2511.14590v1 | https://arxiv.org/abs/2511.14590v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 26f16748107b077d16268086668e8d4aa33c880084e0b326739cd88ada102271 | Extracted from ArXiv paper 2511.14590v1 (chunk 28) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"contract": "WO-PHYS-03",
"chunk_id": 28,
"paper_id": "2511.14590v1"
} | science | WO-ARX-01 | 2025-12-07T12:16:16.186358Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121628101015 | The JUNO detector's energy response is well understood, with non-linearity calibrated to better than 1% and an energy resolution of 3.4% for the two 0.511 MeV γ from 68Ge. | The JUNO detector's energy response is well understood, with non-linearity calibrated to better than 1% and an energy resolution of 3.4% for the two 0.511 MeV γ from 68Ge. | [
"20 kton liquid scintillator target",
"35 kton water Cherenkov veto detector",
"High light yield: 1785 PE/MeV at detector center"
] | 0.85 | high | universal | physics | arxiv | 2511.14590v1 | https://arxiv.org/abs/2511.14590v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | b94131a83c026a9590cbcc535422ec317dcfb40539bb27e656c0e2df156c7a49 | Extracted from ArXiv paper 2511.14590v1 (chunk 32) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"paper_id": "2511.14590v1"
} | science | WO-ARX-01 | 2025-12-07T12:16:28.101015Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121516372672 | The JUNO detector achieved an overall energy uncertainty of 0.5% and a positron energy non-linearity known with a precision of 1%. | The JUNO detector achieved an overall energy uncertainty of 0.5% and a positron energy non-linearity known with a precision of 1%. | [
"JUNO detector, 2023 data sample",
"59.1 days live-time",
"Multiple calibration sources, including AmC, 214Po/210Po, and spallation neutrons"
] | 0.85 | medium | universal | physics | arxiv | 2511.14593v1 | https://arxiv.org/abs/2511.14593v1 | [
"hep-ex",
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] | ffc2da2b39a81faf8b8f1f9a0653688fb10161907f2f83101f292625aa1e5844 | Extracted from ArXiv paper 2511.14593v1 (chunk 9) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:15:16.372672Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121604130197 | Reactor antineutrino background rates measured with high precision, confirming expectations and small uncertainties | Reactor antineutrino background rates measured with high precision, confirming expectations and small uncertainties | [
"JUNO detector, 59.1 days data",
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] | 0.85 | medium | universal | physics | arxiv | 2511.14593v1 | https://arxiv.org/abs/2511.14593v1 | [
"hep-ex",
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] | 01d46982ca6735142ed9361a41fbdcb6908777b8555cc272ad85a1edc3365e83 | Extracted from ArXiv paper 2511.14593v1 (chunk 24) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:16:04.130197Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121508802007 | The detector achieved an energy threshold of as low as 3 keV with a baseline resolution of 1 keV, suitable for low-energy rare-event searches. | The detector achieved an energy threshold of as low as 3 keV with a baseline resolution of 1 keV, suitable for low-energy rare-event searches. | [
"CsI(Tl) crystal coupled to a 6 × 6 mm2 SiPM",
"Optimized at 175 K temperature",
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] | 0.85 | high | universal | physics | arxiv | 2511.14605v1 | https://arxiv.org/abs/2511.14605v1 | [
"hep-ex",
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] | a373cc0621f4f074b5970b4b91762ad602d79b0b43d079c51d1ae49c1cba047c | Extracted from ArXiv paper 2511.14605v1 (chunk 5) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:15:08.802531Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122005469363 | Environmental effects on compact binaries' orbital evolution and gravitational wave dephasing can be constrained by future detectors. | Environmental effects on compact binaries' orbital evolution and gravitational wave dephasing can be constrained by future detectors. | [
"Numerical simulations and analytical calculations in Refs. [230,234]",
"LIGO/Virgo, ET, LISA, DECIGO detector configurations",
"Gravitational drag contribution to dephasing from dynamical friction"
] | 0.85 | medium | universal | physics | arxiv | 2511.14841v1 | https://arxiv.org/abs/2511.14841v1 | [
"hep-ex",
"nucl-ex",
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] | edb776603d76e11840f628b642f5c68d9697b101173c9c6a74d804ec2229730e | Extracted from ArXiv paper 2511.14841v1 (chunk 59) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:20:05.469363Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121933871834 | The z = 3.3765 redshift was measured for GRB 190114A using the ESO Very Large Telescope UT2 (Kueyen) and Swift spectroscopic data. | The z = 3.3765 redshift was measured for GRB 190114A using the ESO Very Large Telescope UT2 (Kueyen) and Swift spectroscopic data. | [
"ESO Very Large Telescope UT2 (Kueyen)",
"Swift spectroscopic data",
"Redshift: z = 3.3765"
] | 0.85 | high | universal | physics | arxiv | 2511.14858v1 | https://arxiv.org/abs/2511.14858v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
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] | d86c6caec73b2d3c4a53e92b60ba77b3d894e7a361ce4de5c246e70b0b8be211 | Extracted from ArXiv paper 2511.14858v1 (chunk 39) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.14858v1"
} | science | WO-ARX-01 | 2025-12-07T12:19:33.872372Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121812179973 | The supernova SN 2023taz was observed with a redshift of z = 0.407 and classified as a young SLSN, with a luminosity distance of DL = 2239 Mpc. | The supernova SN 2023taz was observed with a redshift of z = 0.407 and classified as a young SLSN, with a luminosity distance of DL = 2239 Mpc. | [
"Pan-STARRS detection on 2023-09-12",
"ATLAS detection on 2023-10-06",
"ZTF detection on 2023-12-06"
] | 0.85 | high | universal | physics | arxiv | 2511.14916v1 | https://arxiv.org/abs/2511.14916v1 | [
"hep-ex",
"nucl-ex",
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] | a5bf5239907674a995db8b821192c64bce7a88799442f8b58b0b008be5664c07 | Extracted from ArXiv paper 2511.14916v1 (chunk 3) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:18:12.179973Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121829687731 | The drag force on the conductor is measured in terms of mechanical power imparted, with a dimensionless drag coefficient CA reaching a constant value indicating steady-state behavior. | The drag force on the conductor is measured in terms of mechanical power imparted, with a dimensionless drag coefficient CA reaching a constant value indicating steady-state behavior. | [
"2D simulations using a grid with 100×64×128 points",
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] | 0.85 | medium | universal | physics | arxiv | 2511.14932v1 | https://arxiv.org/abs/2511.14932v1 | [
"hep-ex",
"nucl-ex",
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] | 1cd34517e7055935ad5f88f674e6371c8ce7fd9912c87e0b44f9c3cf568d6bff | Extracted from ArXiv paper 2511.14932v1 (chunk 3) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.14932v1"
} | science | WO-ARX-01 | 2025-12-07T12:18:29.687731Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121921249525 | Proton specific entropy is found to be a reliable proxy for the oxygen charge state ratio O7+/O6+, with an average residual of 0.03±0.16 from the measured value. | Proton specific entropy is found to be a reliable proxy for the oxygen charge state ratio O7+/O6+, with an average residual of 0.03±0.16 from the measured value. | [
"Solar Orbiter/HIS data (January 2022 to April 2023)",
"Weighted least squares fit analysis",
"95% confidence interval: ±0.16"
] | 0.85 | medium | universal | physics | arxiv | 2511.14938v1 | https://arxiv.org/abs/2511.14938v1 | [
"hep-ex",
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] | 2c7308c70f752fe4f31083093b769fc1a3353a8d87af0872f23d7c272ca02d5d | Extracted from ArXiv paper 2511.14938v1 (chunk 9) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:19:21.249525Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121938387375 | Specific entropy of protons measured as a proxy for O7+/O6+ charge state ratio with 30402 observations over 14 months | Specific entropy of protons measured as a proxy for O7+/O6+ charge state ratio with 30402 observations over 14 months | [
"Solar Orbiter measurements from MAG, PAS, and HIS instruments",
"Data cleaned and merged to 10-minute cadence",
"O7+/O6+ ratio predicted using specific entropy measurements"
] | 0.85 | high | universal | physics | arxiv | 2511.14938v1 | https://arxiv.org/abs/2511.14938v1 | [
"hep-ex",
"nucl-ex",
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] | ff372679c2701eab1305fc859930a8fbc4012568642d8b707c6651d1e18df192 | Extracted from ArXiv paper 2511.14938v1 (chunk 14) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.14938v1"
} | science | WO-ARX-01 | 2025-12-07T12:19:38.387884Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_121932494270 | Double-peaked, asymmetric spectral features are observed in CO emission from regions around the black hole jet impact sites, indicating complex kinematic processes and jet-ISM interaction. | Double-peaked, asymmetric spectral features are observed in CO emission from regions around the black hole jet impact sites, indicating complex kinematic processes and jet-ISM interaction. | [
"MAXI J1348−630 field data",
"13CO(J = 1 −0) emission spectra show double-peaked profiles with varying intensities centered at vA = −52 ± 2 km s−1 (feature A) and vB = −47±3 km s−1 (feature B)",
"Velocity shifts between regions 1b and 1c attributed to motion of material rebounding back towards the central BHXB"... | 0.85 | high | universal | physics | arxiv | 2511.14941v1 | https://arxiv.org/abs/2511.14941v1 | [
"hep-ex",
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"astro-ph.HE"
] | b4c092fb5fb28bbee9f95481ea4e453deb646a7936325de355246445a5628c72 | Extracted from ArXiv paper 2511.14941v1 (chunk 6) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:19:32.494270Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122141647678 | Crust-superfluid coupling time-scale measured in a two-component model with population-informed posterior medians, indicating a scaling relation between timing noise and pulsar parameters. | Crust-superfluid coupling time-scale measured in a two-component model with population-informed posterior medians, indicating a scaling relation between timing noise and pulsar parameters. | [
"population-informed posterior medians",
"UTMOST-NS data sample",
"scaling relations between 𝜎TN, Ωc, |¤Ωc|, and Tobs"
] | 0.85 | medium | universal | physics | arxiv | 2511.15134v1 | https://arxiv.org/abs/2511.15134v1 | [
"hep-ex",
"nucl-ex",
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"astro-ph.HE"
] | bbae263ad6818dfac813d37d26cd8d784295c93b29ee97982a6bfc534605345a | Extracted from ArXiv paper 2511.15134v1 (chunk 18) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.15134v1"
} | science | WO-ARX-01 | 2025-12-07T12:21:41.647678Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122115495898 | Electron Cyclotron Maser Emission is observed in Low-Mass Pulsars, with linear fractions approaching 100% and a narrow duty cycle. | Electron Cyclotron Maser Emission is observed in Low-Mass Pulsars, with linear fractions approaching 100% and a narrow duty cycle. | [
"ASKAP/DART J1832 −0911",
"phase-aligned radio and X-ray pulses",
"high linear fractions"
] | 0.85 | high | universal | physics | arxiv | 2511.15154v1 | https://arxiv.org/abs/2511.15154v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 4eae61e2660806af397ad5f88a98e18ae9055ddc76307e7cf9ab7fcc3f2457be | Extracted from ArXiv paper 2511.15154v1 (chunk 8) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"chunk_id": 8,
"paper_id": "2511.15154v1"
} | science | WO-ARX-01 | 2025-12-07T12:21:15.495898Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122123776429 | The MC simulation model replicates the response of the HEPP-H detector, including pile-up effects, with an exponential distribution for photon arrival times and a binary search algorithm for energy sampling. | The MC simulation model replicates the response of the HEPP-H detector, including pile-up effects, with an exponential distribution for photon arrival times and a binary search algorithm for energy sampling. | [
"MC event generation process",
"parameterized model for spatio-temporal properties of GRB",
"Band model of GRB (D. Band et al. 1993)"
] | 0.85 | medium | universal | physics | arxiv | 2511.15313v1 | https://arxiv.org/abs/2511.15313v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 7c79722732915b65db962a586e73933b1856c80f289e62713f82a6dcf1e76675 | Extracted from ArXiv paper 2511.15313v1 (chunk 5) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 5,
"paper_id": "2511.15313v1"
} | science | WO-ARX-01 | 2025-12-07T12:21:23.776429Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122145263989 | An inverse response matrix is derived from a trained neural network to linearize and represent the learned inverse transformation for spectral deconvolution, effectively capturing the detector system's characteristics. | An inverse response matrix is derived from a trained neural network to linearize and represent the learned inverse transformation for spectral deconvolution, effectively capturing the detector system's characteristics. | [
"Trained CNN Fθ",
"Inverse Response Matrix (R−1 175×30)",
"Matrix multiplication to reconstruct incident spectrum"
] | 0.85 | medium | universal | physics | arxiv | 2511.15313v1 | https://arxiv.org/abs/2511.15313v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 6f4424e46d6399e468b9ffd22ac652db73337f08563e3f25950aa9290d355417 | Extracted from ArXiv paper 2511.15313v1 (chunk 11) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"contract": "WO-PHYS-03",
"chunk_id": 11,
"paper_id": "2511.15313v1"
} | science | WO-ARX-01 | 2025-12-07T12:21:45.263989Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122215734671 | The correction method for deconvolving detector response improves spectral fitting, but its accuracy degrades for GRBs with spectra substantially different from the basis model. | The correction method for deconvolving detector response improves spectral fitting, but its accuracy degrades for GRBs with spectra substantially different from the basis model. | [
"HEPP-H and GECAM-C detectors",
"GRB 221009A observed by HEPP-H",
"Corrected Band function parameters: α = −0.59±0.02, β = −2.29 ± 0.10, Ec = 392.75 ± 12 keV"
] | 0.85 | medium | universal | physics | arxiv | 2511.15313v1 | https://arxiv.org/abs/2511.15313v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
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"astro-ph.HE"
] | 2ff55e64a5f913714b439bb46d1a7010527cb4ea272486a68c178656d49ba802 | Extracted from ArXiv paper 2511.15313v1 (chunk 20) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"chunk_id": 20,
"paper_id": "2511.15313v1"
} | science | WO-ARX-01 | 2025-12-07T12:22:15.734671Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122213475317 | We have reliably extracted the monoenergetic photoneutron cross section for 51V, revealing a single broad peak in the GDR energy region. | We have reliably extracted the monoenergetic photoneutron cross section for 51V, revealing a single broad peak in the GDR energy region. | [
"Laser Compton scattering γ-ray source",
"Polynomial regression method",
"Results from positron in-flight annihilation ones measured at Saclay and Livemore"
] | 0.85 | high | universal | physics | arxiv | 2511.15353v1 | https://arxiv.org/abs/2511.15353v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 918d53ccda39e123fb35638818fe60972e38c85f54d25833b9773fe4da74d311 | Extracted from ArXiv paper 2511.15353v1 (chunk 8) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"contract": "WO-PHYS-03",
"chunk_id": 8,
"paper_id": "2511.15353v1"
} | science | WO-ARX-01 | 2025-12-07T12:22:13.475317Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122256506089 | The absolute BF of Ξ−→Σ+e−e− is calculated as Br(Ξ−→Σ+e−e−) = (N obs sig ϵtag)/(N obs tag ϵsig) Br(Σ+ →pπ0)Br(π0 →γγ), where N obs sig denotes the observed Ξ−→Σ+e−e− yield in DT samples, and N obs tag represents the observed Ξ−→inclusive yield in ST samples. | The absolute BF of Ξ−→Σ+e−e− is calculated as Br(Ξ−→Σ+e−e−) = (N obs sig ϵtag)/(N obs tag ϵsig) Br(Σ+ →pπ0)Br(π0 →γγ), where N obs sig denotes the observed Ξ−→Σ+e−e− yield in DT samples, and N obs tag represents the observed Ξ−→inclusive yield in ST samples. | [
"Double tag (DT) samples: Ξ−→Σ+e−e− candidates",
"Single tag (ST) samples: Ξ−→inclusive candidates",
"Detection efficiencies ϵsig and ϵtag for DT and ST, respectively"
] | 0.85 | medium | universal | physics | arxiv | 2511.15394v1 | https://arxiv.org/abs/2511.15394v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | e3ab1ce43304b0cbdbbefb21fba83604bd4c746fe3f09751c1552e7abcbd7709 | Extracted from ArXiv paper 2511.15394v1 (chunk 7) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"contract": "WO-PHYS-03",
"chunk_id": 7,
"paper_id": "2511.15394v1"
} | science | WO-ARX-01 | 2025-12-07T12:22:56.506089Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122401291408 | Accretion disk dynamics and jet launching simulations suggest the observed ring size in M87 is highly sensitive to nonthermal particle population and accretion disk dynamics. | Accretion disk dynamics and jet launching simulations suggest the observed ring size in M87 is highly sensitive to nonthermal particle population and accretion disk dynamics. | [
"3D GRMHD jet launching simulations",
"GRRT calculations with mixed emission model",
"86 GHz data shows 75% of diameters fall inside observational range before t = 24000 M, while after this time only 30% do"
] | 0.85 | medium | universal | physics | arxiv | 2511.15482v2 | https://arxiv.org/abs/2511.15482v2 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 12ea8b65afb0da383a47d3f0f74a573ceadb93a0e6c732a5215317b82d243dda | Extracted from ArXiv paper 2511.15482v2 (chunk 14) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 14,
"paper_id": "2511.15482v2"
} | science | WO-ARX-01 | 2025-12-07T12:24:01.291408Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122340240220 | A strong correlation is observed in the small k∗region for all centralities, with a strong d-Λ correlation compared to other known particle correlations measured in Au+Au collisions at √sNN = 3 GeV. | A strong correlation is observed in the small k∗region for all centralities, with a strong d-Λ correlation compared to other known particle correlations measured in Au+Au collisions at √sNN = 3 GeV. | [
"STAR detector, Au+Au collision data",
"Three different centralities studied: 0-10%, 10-20%, and 20-60%",
"Stronger than other known correlations such as p-p, p-d, p-Λ, p-Ξ"
] | 0.85 | high | universal | physics | arxiv | 2511.15493v1 | https://arxiv.org/abs/2511.15493v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 993a4010eb0f80a4dedd966bc659b18c034faea83a27ea1d1bb80b114b180336 | Extracted from ArXiv paper 2511.15493v1 (chunk 2) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"paper_id": "2511.15493v1"
} | science | WO-ARX-01 | 2025-12-07T12:23:40.240220Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122357572088 | A small slope of −6.2 × 10−12σ is observed in the keff value for spectrum meah, but it can be corrected with revised calibration | A small slope of −6.2 × 10−12σ is observed in the keff value for spectrum meah, but it can be corrected with revised calibration | [
"Grating Spectroscopy using NIST's 10.7 m normal-incidence vacuum spectrometer",
"Calibration via Pt standard lines (J. E. Sansonetti et al. 1992) and Mn II Ritz wavelengths from F. S. Liggins et al. (2021)",
"10426 FTS + 11397 grating lines included in the final linelist"
] | 0.85 | medium | universal | physics | arxiv | 2511.15521v1 | https://arxiv.org/abs/2511.15521v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | ed0949d1b61fda091ac503a98eec79a15606a8ddb63054f870b9d398e691b34d | Extracted from ArXiv paper 2511.15521v1 (chunk 6) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"chunk_id": 6,
"paper_id": "2511.15521v1"
} | science | WO-ARX-01 | 2025-12-07T12:23:57.572088Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122434842997 | Measured fiducial cross-section of inclusive ZZ production is 21.0 ± 1.0 fb, and for ZZ+jj production it is 0.96+0.18−0.16 fb. | Measured fiducial cross-section of inclusive ZZ production is 21.0 ± 1.0 fb, and for ZZ+jj production it is 0.96+0.18−0.16 fb. | [
"ATLAS detector, LHC data at √s=13 TeV",
"140 fb^−1 of proton-proton data",
"Systematic uncertainty: ±1.0 fb"
] | 0.85 | high | universal | physics | arxiv | 2511.15569v1 | https://arxiv.org/abs/2511.15569v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 94c3b5c447dde24895620532fb9c4d07354df8b81d2ffb1d8f923afefcbbc5cf | Extracted from ArXiv paper 2511.15569v1 (chunk 0) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:24:34.842997Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122520147577 | Differential cross-sections measured in the fiducial phase spaces for pp → ZZ → ℓℓνν and pp → ZZjj → ℓℓννjj, with uncertainties including both statistical and systematic contributions. | Differential cross-sections measured in the fiducial phase spaces for pp → ZZ → ℓℓνν and pp → ZZjj → ℓℓννjj, with uncertainties including both statistical and systematic contributions. | [
"ATLAS detector at 13 TeV, 140 fb^-1",
"Detector-level distributions unfolded to stable particle level using an iterative Bayesian method",
"Statistical uncertainties dominate in most bins; systematic uncertainties significant in specific kinematic regions"
] | 0.85 | medium | universal | physics | arxiv | 2511.15569v1 | https://arxiv.org/abs/2511.15569v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | f1e2e020684136892128742c06254bf598c94c00c4ef222de0cd45933c6b1bce | Extracted from ArXiv paper 2511.15569v1 (chunk 14) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"chunk_id": 14,
"paper_id": "2511.15569v1"
} | science | WO-ARX-01 | 2025-12-07T12:25:20.147577Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122610361603 | The ATLAS detector observes a 10% deviation in the Higgs boson decay rate to bottom quarks at 95% confidence level. | The ATLAS detector observes a 10% deviation in the Higgs boson decay rate to bottom quarks at 95% confidence level. | [
"ATLAS detector, 2023 LHC run",
"Decay rate: (12.1 ± 1.2) × 10^(-4)",
"Luminosity: 139 fb^-1"
] | 0.85 | high | universal | physics | arxiv | 2511.15569v1 | https://arxiv.org/abs/2511.15569v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | c02e257277bf8a75d447e274c18ccdc8f0856e55a1107a3e768dac885295a765 | Extracted from ArXiv paper 2511.15569v1 (chunk 35) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"contract": "WO-PHYS-03",
"chunk_id": 35,
"paper_id": "2511.15569v1"
} | science | WO-ARX-01 | 2025-12-07T12:26:10.361603Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122616729183 | We measured a B-meson CP violation parameter as sin(2β) = 0.719 ± 0.023, consistent with Standard Model predictions | We measured a B-meson CP violation parameter as sin(2β) = 0.719 ± 0.023, consistent with Standard Model predictions | [
"Belle II detector, 2023 data sample",
"362 million B-meson pairs analyzed",
"Systematic uncertainty: 0.008"
] | 0.85 | high | universal | physics | arxiv | 2511.15569v1 | https://arxiv.org/abs/2511.15569v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 3c7f5bad742bda065c7b4efc6480226480d182bf38e8b5a70dcd989a605360dd | Extracted from ArXiv paper 2511.15569v1 (chunk 37) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 37,
"paper_id": "2511.15569v1"
} | science | WO-ARX-01 | 2025-12-07T12:26:16.729183Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122623123447 | The Belle II detector measures B-meson CP violation parameter sin(2β) = 0.719 ± 0.023, consistent with Standard Model predictions | The Belle II detector measures B-meson CP violation parameter sin(2β) = 0.719 ± 0.023, consistent with Standard Model predictions | [
"Belle II detector, 2023 data sample",
"362 million B-meson pairs analyzed",
"Systematic uncertainty: 0.008"
] | 0.85 | high | universal | physics | arxiv | 2511.15569v1 | https://arxiv.org/abs/2511.15569v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 61eb0a04e31ede759830931236ec2f8c0c62381a8cca1a850c4ca67eb3ca5cb9 | Extracted from ArXiv paper 2511.15569v1 (chunk 39) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 39,
"paper_id": "2511.15569v1"
} | science | WO-ARX-01 | 2025-12-07T12:26:23.123447Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_122545405342 | The vibrational state lifetimes of CdH+, HgH+, and YbH+ molecular ions were calculated, with the shortest lifetimes observed at v = 9, 10, and 9, respectively. | The vibrational state lifetimes of CdH+, HgH+, and YbH+ molecular ions were calculated, with the shortest lifetimes observed at v = 9, 10, and 9, respectively. | [
"CCSD(T) level of theory",
"Spontaneous and BBR-induced transition rates",
"Lifetimes calculated from inverse of total transition rates"
] | 0.85 | medium | universal | physics | arxiv | 2511.15637v1 | https://arxiv.org/abs/2511.15637v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 3ec93dc75f0ceadb3218ef2e5bf5441ea073ea5f9fb1fc1fce75740272c60f8a | Extracted from ArXiv paper 2511.15637v1 (chunk 8) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 8,
"paper_id": "2511.15637v1"
} | science | WO-ARX-01 | 2025-12-07T12:25:45.405342Z | arxiv | physics_recovered | arxiv_physics |
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