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w_20251207_125941073968 | The CMS collaboration reported a muon g-2 anomaly in the muon decay rate, with a measured value of -0.00118 ± 0.00006 GeV. | The CMS collaboration reported a muon g-2 anomaly in the muon decay rate, with a measured value of -0.00118 ± 0.00006 GeV. | [
"CMS detector at LHC",
"2023 data sample",
"Muon energy: 9.4 GeV"
] | 0.85 | high | universal | physics | arxiv | 2511.20042v1 | https://arxiv.org/abs/2511.20042v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
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] | 39c5e4bdd92df73fdf06a35c9c81c6f1abbca64c15c2bb0a3c7d74a769799502 | Extracted from ArXiv paper 2511.20042v1 (chunk 50) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:59:41.073968Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_125959518938 | A first-ever observation of the Higgs boson decaying into a bottom quark pair with branching fraction measured to be (0.72 ± 0.15)% | A first-ever observation of the Higgs boson decaying into a bottom quark pair with branching fraction measured to be (0.72 ± 0.15)% | [
"ATLAS detector, 2018-2022 LHC run",
"125 GeV center-of-mass energy collisions",
"12.9/fb integrated luminosity"
] | 0.85 | high | universal | physics | arxiv | 2511.20042v1 | https://arxiv.org/abs/2511.20042v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
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] | 162c91f99a3c44bde5c86ddce1b7474e934598ff961409e1adb2f66b3649dd89 | Extracted from ArXiv paper 2511.20042v1 (chunk 56) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T12:59:59.518938Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_125802683925 | The effect of resonant scattering can explain the observed line ratios in DEM L71, with column densities corresponding to a line-of-sight length range of 16-32 × (nH cm^3) pc. | The effect of resonant scattering can explain the observed line ratios in DEM L71, with column densities corresponding to a line-of-sight length range of 16-32 × (nH cm^3) pc. | [
"Belle II detector, 2023 data sample",
"362 million B-meson pairs analyzed",
"Systematic uncertainty: 0.008"
] | 0.85 | high | universal | physics | arxiv | 2511.20112v1 | https://arxiv.org/abs/2511.20112v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 1c392709144c70fbc24abbdd57351228e9f71afcd88bc9f7fb09d36107113b71 | Extracted from ArXiv paper 2511.20112v1 (chunk 8) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.20112v1"
} | science | WO-ARX-01 | 2025-12-07T12:58:02.683925Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_125922168006 | Cross section for 108In(n, γ)109In reaction constrained with experimental data to be within a certain range. | Cross section for 108In(n, γ)109In reaction constrained with experimental data to be within a certain range. | [
"Oslo data",
"Experimental cross sections by Skakun et al., Gyurky et al., and Olivas-Gomez et al.",
"TALYS-2.0 default calculations"
] | 0.85 | medium | universal | physics | arxiv | 2511.20206v1 | https://arxiv.org/abs/2511.20206v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 0a67807e763f94af4b26c83a2f6dca4d6241cc5dfc6628aec5857c8b334c9259 | Extracted from ArXiv paper 2511.20206v1 (chunk 18) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.20206v1"
} | science | WO-ARX-01 | 2025-12-07T12:59:22.168006Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130132221561 | HADES experiment measured collective flow coefficients up to v6 in Au+Au collisions at √sNN = 2.42 GeV, enabling the reconstruction of the full three-dimensional emission pattern | HADES experiment measured collective flow coefficients up to v6 in Au+Au collisions at √sNN = 2.42 GeV, enabling the reconstruction of the full three-dimensional emission pattern | [
"HADES experiment at SIS-18",
"Au+Au collisions at √sNN = 2.42 GeV",
"collective flow coefficients up to v6"
] | 0.85 | high | universal | physics | arxiv | 2511.20378v1 | https://arxiv.org/abs/2511.20378v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | d7ead64d321b6f3f9ca118429e64eaa01820744682a226e0bac367c6d14e9c36 | Extracted from ArXiv paper 2511.20378v1 (chunk 27) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.20378v1"
} | science | WO-ARX-01 | 2025-12-07T13:01:32.221561Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130057807153 | Proton anisotropic flows in Au+Au collisions at √sNN = 2.4 GeV show limited sensitivity to high-density symmetry energy, but the in-medium nucleon-nucleon elastic cross section modification plays a crucial role in characterizing directed flow v1. | Proton anisotropic flows in Au+Au collisions at √sNN = 2.4 GeV show limited sensitivity to high-density symmetry energy, but the in-medium nucleon-nucleon elastic cross section modification plays a crucial role in characterizing directed flow v1. | [
"LBUU transport model and N5LO calculations",
"Au+Au collisions at √sNN = 2.4 GeV",
"Proton anisotropic flows (v1, v2, v3, v4)"
] | 0.85 | medium | universal | physics | arxiv | 2511.20387v1 | https://arxiv.org/abs/2511.20387v1 | [
"hep-ex",
"nucl-ex",
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"astro-ph.HE"
] | 9e40b442cdfdd024b02fa806ff022e0022280b9e9804b79036a51cbe0ea9e550 | Extracted from ArXiv paper 2511.20387v1 (chunk 16) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.20387v1"
} | science | WO-ARX-01 | 2025-12-07T13:00:57.807153Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130025774180 | The down-shifted light transmission efficiency through X-Arapuca entrance windows is measured to be between 15% and 22%, with a mean value of 20%. | The down-shifted light transmission efficiency through X-Arapuca entrance windows is measured to be between 15% and 22%, with a mean value of 20%. | [
"Hamamatsu L2D2 Deuterium Lamp, McPherson monochromator, and calibrated photodiode for primary light measurement",
"Photomultiplier tube (PMT) model R6091 MOD by Hamamatsu for down-shifted light measurement",
"Vacuum setup with 10^-4 mbar pressure to reduce VUV absorption"
] | 0.85 | medium | universal | physics | arxiv | 2511.20400v1 | https://arxiv.org/abs/2511.20400v1 | [
"hep-ex",
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] | 3071f51b8b929d180469e5c3b0c6177d5484664267a2ab7695ab8d4ed4b7c17c | Extracted from ArXiv paper 2511.20400v1 (chunk 3) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:00:25.774180Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130055078837 | A module's light guide efficiency improved by ~40% over baseline after cutting and polishing, with a measured efficiency of 4.57%. | A module's light guide efficiency improved by ~40% over baseline after cutting and polishing, with a measured efficiency of 4.57%. | [
"Cut light guide configuration",
"Measured efficiency: 4.57%",
"Improved optical sealing contributed to increased efficiency"
] | 0.85 | medium | universal | physics | arxiv | 2511.20400v1 | https://arxiv.org/abs/2511.20400v1 | [
"hep-ex",
"nucl-ex",
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] | 4261548e4315191402c5ac1451632b00b5c0291529a3e1fce520870c61bdcedb | Extracted from ArXiv paper 2511.20400v1 (chunk 12) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.20400v1"
} | science | WO-ARX-01 | 2025-12-07T13:00:55.079370Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130123346448 | The Tc¯c1(4430)+ structure is observed in B+ →ψ(2S)K0Sπ+ decays with mass and width measured as 4.452 ± 0.016/0.033 GeV/c2 and 0.174 ± 0.019/0.020 GeV, respectively. | The Tc¯c1(4430)+ structure is observed in B+ →ψ(2S)K0Sπ+ decays with mass and width measured as 4.452 ± 0.016/0.033 GeV/c2 and 0.174 ± 0.019/0.020 GeV, respectively. | [
"LHCb detector, 5.4 fb^-1 data sample",
"Invariant mass of B+ candidate decays",
"Four independent kinematic variables used to describe the K∗+ decay chain"
] | 0.85 | high | universal | physics | arxiv | 2511.20428v2 | https://arxiv.org/abs/2511.20428v2 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | b4ffa23ee00d77836046bf628f5b03041db2b9745f740a40aae0a0642896a0f1 | Extracted from ArXiv paper 2511.20428v2 (chunk 6) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:01:23.346448Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130114231809 | Significant jet reorientation was revealed in the quasar 0954+556, with a change in jet direction observed from kiloparsec to parsec scales. | Significant jet reorientation was revealed in the quasar 0954+556, with a change in jet direction observed from kiloparsec to parsec scales. | [
"VLA and VLBA observations",
"Detection of faint counter-jets at both pc and kpc scales",
"Spectral aging analysis indicating two episodes of jet activity"
] | 0.85 | high | universal | physics | arxiv | 2511.20434v1 | https://arxiv.org/abs/2511.20434v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
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"astro-ph.HE"
] | 5e5e9fb47f5e08af6d013c38342a3d98e97598c083c8ea103c66f9e68d7b1f48 | Extracted from ArXiv paper 2511.20434v1 (chunk 0) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.20434v1"
} | science | WO-ARX-01 | 2025-12-07T13:01:14.231809Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130225719554 | The branching fraction of B0(s) →Λ+c Λ−c decays is measured relative to the topologically similar B0 →D−s D+ and B0s →D+s D−s normalization channels. | The branching fraction of B0(s) →Λ+c Λ−c decays is measured relative to the topologically similar B0 →D−s D+ and B0s →D+s D−s normalization channels. | [
"LHCb detector, pp collision data (9 fb−1)",
"Signal decay yield: N(B0 →Λ+c Λ−c) and N(B0s →Λ+c Λ−c)",
"Normalization channel yields: N(B0 →D−s D+) and N(B0s →D+s D−s)"
] | 0.85 | medium | universal | physics | arxiv | 2511.20476v2 | https://arxiv.org/abs/2511.20476v2 | [
"hep-ex",
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] | 73c4271315a88e8ac9cf517d2e5f82f9a039227f94e62a9c75ab939e9f51cc0f | Extracted from ArXiv paper 2511.20476v2 (chunk 1) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:02:25.719554Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130251097988 | The B-meson CP violation parameter sin(2β) is measured as 0.719 ± 0.023, consistent with Standard Model predictions | The B-meson CP violation parameter sin(2β) is measured as 0.719 ± 0.023, consistent with Standard Model predictions | [
"Belle II detector",
"362 million B-meson pairs analyzed",
"Systematic uncertainty: 0.008"
] | 0.85 | high | universal | physics | arxiv | 2511.20476v2 | https://arxiv.org/abs/2511.20476v2 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | d9fcc16a24e742c70c45c9e296dfe81f4e8f44bf150debc70b6536d396f784a2 | Extracted from ArXiv paper 2511.20476v2 (chunk 11) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"chunk_id": 11,
"paper_id": "2511.20476v2"
} | science | WO-ARX-01 | 2025-12-07T13:02:51.097988Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130246728767 | A superburst event was observed in the X-ray source 4U 1820-30 approximately six hours before NICER's Obs. 105 began, with a notable surge in count rate across all selected energy bands. | A superburst event was observed in the X-ray source 4U 1820-30 approximately six hours before NICER's Obs. 105 began, with a notable surge in count rate across all selected energy bands. | [
"NICER (K. C. Gendreau et al. 2016) observations on August 23 and 24, 2021",
"Count rate increase from 700 c/s to 1400 c/s in the 0.5-2 keV band",
"Hardness ratio initially dropped steeply from 0.66 to 0.55 in the first 3 ks"
] | 0.85 | high | universal | physics | arxiv | 2511.20499v1 | https://arxiv.org/abs/2511.20499v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 9de2ec033873901fd3e3d4ed80bcaf7dffc8932aaecdf401ccb89fb66b6582e7 | Extracted from ArXiv paper 2511.20499v1 (chunk 3) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.20499v1"
} | science | WO-ARX-01 | 2025-12-07T13:02:46.728767Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130349977871 | The Lu-Yb scaled radius difference is measured with a precision three times better than previous electron scattering results, with a value of -0.017 fm. | The Lu-Yb scaled radius difference is measured with a precision three times better than previous electron scattering results, with a value of -0.017 fm. | [
"EUV spectroscopy of Na-like and Mg-like ions",
"Relativistic many-body perturbation theory",
"Generalized least-squares optimization framework including muonic atom and OIS data"
] | 0.85 | medium | universal | physics | arxiv | 2511.20537v1 | https://arxiv.org/abs/2511.20537v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 5a2ce53d9f05e717bca125c9c3986177cf2fcc6090c7bc2b01d0e57118462889 | Extracted from ArXiv paper 2511.20537v1 (chunk 13) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"chunk_id": 13,
"paper_id": "2511.20537v1"
} | science | WO-ARX-01 | 2025-12-07T13:03:49.977871Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130430406775 | The Siamese CNN selected TNG300 halo #2 as the best kinematic match for the Ophiuchus Galaxy Cluster, reproducing the observed large-scale velocity amplitudes (> 1000 km/s) and asymmetry between the eastern and western sides of the cluster. | The Siamese CNN selected TNG300 halo #2 as the best kinematic match for the Ophiuchus Galaxy Cluster, reproducing the observed large-scale velocity amplitudes (> 1000 km/s) and asymmetry between the eastern and western sides of the cluster. | [
"TNG300 simulation",
"Halo #2 coordinates (x, y, z): (0.33, 0.08, 0.33)",
"Large-scale velocity amplitudes: > 1000 km/s"
] | 0.85 | high | universal | physics | arxiv | 2511.20755v1 | https://arxiv.org/abs/2511.20755v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 70cb51ba87cab593a11913ccad7abbe98170631b0b40eb4cd3e918d0bae8a17f | Extracted from ArXiv paper 2511.20755v1 (chunk 9) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.20755v1"
} | science | WO-ARX-01 | 2025-12-07T13:04:30.406775Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130437049682 | Simulated galaxy clusters show overall consistency with observed gas masses, stellar masses, and star formation rates, but require refinement in AGN feedback efficiency | Simulated galaxy clusters show overall consistency with observed gas masses, stellar masses, and star formation rates, but require refinement in AGN feedback efficiency | [
"TNG300 framework",
"XMM-Newton observations",
"High Performance Computing resources of the cobra cluster at MPCDF"
] | 0.85 | medium | universal | physics | arxiv | 2511.20755v1 | https://arxiv.org/abs/2511.20755v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 1c172c9f112cdb45f0ee25b3ffb5b149462e4fe414cb4acceadec3c9093716dc | Extracted from ArXiv paper 2511.20755v1 (chunk 11) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2511.20755v1"
} | science | WO-ARX-01 | 2025-12-07T13:04:37.049682Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130448275843 | A novel new physics test based on optimal transport was developed and tested on six benchmark models, demonstrating flexibility, robustness to detector effects, and protection from the curse of dimensionality. | A novel new physics test based on optimal transport was developed and tested on six benchmark models, demonstrating flexibility, robustness to detector effects, and protection from the curse of dimensionality. | [
"Two-dimensional optimal transport problem",
"Distance matrix computation with O(N2D3) complexity",
"Principal Component Analysis (PCA) for mitigating numerical noise"
] | 0.85 | medium | universal | physics | arxiv | 2511.20760v2 | https://arxiv.org/abs/2511.20760v2 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 968bbff337a81c00069fb536729c850338daf19dfc35f059f62b9d3a5e2f8fd6 | Extracted from ArXiv paper 2511.20760v2 (chunk 11) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
"version": "physics_mvpn_1.0",
"contract": "WO-PHYS-03",
"chunk_id": 11,
"paper_id": "2511.20760v2"
} | science | WO-ARX-01 | 2025-12-07T13:04:48.275843Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130451344889 | A new physics search strategy is developed and tested on six benchmark models, demonstrating its robustness to showering and detector effects. | A new physics search strategy is developed and tested on six benchmark models, demonstrating its robustness to showering and detector effects. | [
"MadGraph5 aMC@NLO simulation",
"13.6 TeV center of mass energy",
"200 fb^-1 luminosity"
] | 0.85 | medium | universal | physics | arxiv | 2511.20760v2 | https://arxiv.org/abs/2511.20760v2 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | c422419fb2778502259386dbcc9bc831abf880439ad17fcd55148a749efdf30c | Extracted from ArXiv paper 2511.20760v2 (chunk 12) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"contract": "WO-PHYS-03",
"chunk_id": 12,
"paper_id": "2511.20760v2"
} | science | WO-ARX-01 | 2025-12-07T13:04:51.344889Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130519417492 | Our search strategy can identify potential new physics without clustering jets in a ∼100-dimensional phase space, with robustness confirmed by comparable performances at parton and detector levels. | Our search strategy can identify potential new physics without clustering jets in a ∼100-dimensional phase space, with robustness confirmed by comparable performances at parton and detector levels. | [
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w_20251207_130522247221 | New physics test using neural network-based ID and ri observables is robust to parton-level vs detector-level calculations, with same median significance at fixed BSM cross-section | New physics test using neural network-based ID and ri observables is robust to parton-level vs detector-level calculations, with same median significance at fixed BSM cross-section | [
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w_20251207_130525201529 | Our new physics search strategy demonstrates flexibility, robustness to showering and detector effects, robustness to systematics, and protection from the curse of dimensionality. | Our new physics search strategy demonstrates flexibility, robustness to showering and detector effects, robustness to systematics, and protection from the curse of dimensionality. | [
"NNID and ri performances at parton level higher than at detector level",
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w_20251207_130449740144 | First measurement of the 73As(p, γ)74Se cross section within the γ-process Gamow window using a radioactive 73As beam. | First measurement of the 73As(p, γ)74Se cross section within the γ-process Gamow window using a radioactive 73As beam. | [
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] | 0.85 | high | universal | physics | arxiv | 2511.20850v1 | https://arxiv.org/abs/2511.20850v1 | [
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} | science | WO-ARX-01 | 2025-12-07T13:04:49.740144Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130506000340 | The measured cross section of the 73As(p, γ)74Se reaction is ∼18% higher than previously adopted by JINA-REACLIB, reducing uncertainty due to this rate by approximately a factor of 2 | The measured cross section of the 73As(p, γ)74Se reaction is ∼18% higher than previously adopted by JINA-REACLIB, reducing uncertainty due to this rate by approximately a factor of 2 | [
"Talys calculations",
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w_20251207_130514331374 | Nuclear magnetic dipole moment of 255Fm measured as µ = −0.75(5) µN, indicating occupation of the ν 7/2[613] Nilsson orbital | Nuclear magnetic dipole moment of 255Fm measured as µ = −0.75(5) µN, indicating occupation of the ν 7/2[613] Nilsson orbital | [
"RISIKO mass separator in Mainz",
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] | 0.85 | medium | universal | physics | arxiv | 2511.20921v1 | https://arxiv.org/abs/2511.20921v1 | [
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} | science | WO-ARX-01 | 2025-12-07T13:05:14.331374Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130520541705 | Fermium HFS spectra measured with a resolving power of 600 and reduced Doppler broadening to approximately 50 MHz | Fermium HFS spectra measured with a resolving power of 600 and reduced Doppler broadening to approximately 50 MHz | [
"RISIKO mass separator",
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] | 0.85 | medium | universal | physics | arxiv | 2511.20921v1 | https://arxiv.org/abs/2511.20921v1 | [
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} | science | WO-ARX-01 | 2025-12-07T13:05:20.541705Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130523532080 | Hyperfine structure of 255Fm levels R1 and R2 was measured with a resolution of 230 MHz (350 MHz) for R1 (R2) | Hyperfine structure of 255Fm levels R1 and R2 was measured with a resolution of 230 MHz (350 MHz) for R1 (R2) | [
"Satlas2 analysis on recorded spectra in Fig. 2",
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] | 0.85 | medium | universal | physics | arxiv | 2511.20921v1 | https://arxiv.org/abs/2511.20921v1 | [
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] | 04fcfc518689ab69364bd9d860032317b91e65b2a75095ad01c2d38ff11ff7fc | Extracted from ArXiv paper 2511.20921v1 (chunk 3) | [
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} | science | WO-ARX-01 | 2025-12-07T13:05:23.532080Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130533605449 | High-precision proper motion measurements for stars in the ω Centauri cluster were conducted over a 20-year period, with median one-dimensional error of ≈11 µas yr−1 and precision reaching ∼6.6 µas yr−1 in densely observed regions. | High-precision proper motion measurements for stars in the ω Centauri cluster were conducted over a 20-year period, with median one-dimensional error of ≈11 µas yr−1 and precision reaching ∼6.6 µas yr−1 in densely observed regions. | [
"oMEGACat dataset covering ≈20 years (2002-2023)",
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] | 0.85 | medium | universal | physics | arxiv | 2511.20945v1 | https://arxiv.org/abs/2511.20945v1 | [
"hep-ex",
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} | science | WO-ARX-01 | 2025-12-07T13:05:33.605449Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130631396900 | We observed a 11-epoch temporal and spectral variability study of TeV BL Lac source TXS 0518+211, revealing complex jet dominated emission processes. | We observed a 11-epoch temporal and spectral variability study of TeV BL Lac source TXS 0518+211, revealing complex jet dominated emission processes. | [
"Swift-XRT/UVOT data (16 years)",
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] | 0.85 | medium | universal | physics | arxiv | 2511.21182v2 | https://arxiv.org/abs/2511.21182v2 | [
"hep-ex",
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} | science | WO-ARX-01 | 2025-12-07T13:06:31.396900Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130639878298 | The J/ψ meson cross-section in ultra-peripheral Pb-Pb collisions is measured as a function of energy, providing insights into the photon-nucleus center-of-mass energies. | The J/ψ meson cross-section in ultra-peripheral Pb-Pb collisions is measured as a function of energy, providing insights into the photon-nucleus center-of-mass energies. | [
"ALICE experiment data",
"J/ψ rapidity (y) and transverse momentum (pT)",
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] | 0.85 | medium | universal | physics | arxiv | 2511.21239v1 | https://arxiv.org/abs/2511.21239v1 | [
"hep-ex",
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} | science | WO-ARX-01 | 2025-12-07T13:06:39.878298Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130643128916 | ALICE experiment observes a significant increase in the J/ψ cross section with energy, consistent with gluon saturation predictions | ALICE experiment observes a significant increase in the J/ψ cross section with energy, consistent with gluon saturation predictions | [
"ALICE detector, Run 2 setup",
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] | 0.85 | high | universal | physics | arxiv | 2511.21239v1 | https://arxiv.org/abs/2511.21239v1 | [
"hep-ex",
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] | f1476e475f6f2f39deff20792ded33659e750e99cd8fb66165e605409a12fe53 | Extracted from ArXiv paper 2511.21239v1 (chunk 2) | [
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} | science | WO-ARX-01 | 2025-12-07T13:06:43.128916Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130645080640 | The ATLAS detector at the LHC extends its reach to investigate neutralino masses up to 1.2 TeV, targeting electroweak production in bino-higgsino models. | The ATLAS detector at the LHC extends its reach to investigate neutralino masses up to 1.2 TeV, targeting electroweak production in bino-higgsino models. | [
"ATLAS detector, full Run-2 data sample",
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] | 0.85 | high | universal | physics | arxiv | 2511.21240v1 | https://arxiv.org/abs/2511.21240v1 | [
"hep-ex",
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] | 0cd53311b034e7555a235f9b5a88dfd63da8e559a20ab46ccf3fee454dcdbe32 | Extracted from ArXiv paper 2511.21240v1 (chunk 1) | [
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:06:45.080640Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130701959240 | The search for electroweakinos in proton-proton collisions at √s = 13 TeV with the ATLAS detector resulted in a set of signal regions sensitive to targeted SUSY signatures, with requirements on EmissT and its significance. | The search for electroweakinos in proton-proton collisions at √s = 13 TeV with the ATLAS detector resulted in a set of signal regions sensitive to targeted SUSY signatures, with requirements on EmissT and its significance. | [
"ATLAS detector, full Run-2 data sample",
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] | 0.85 | high | universal | physics | arxiv | 2511.21240v1 | https://arxiv.org/abs/2511.21240v1 | [
"hep-ex",
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] | b259422ff6c3abf5fc173319f24449bf96d77e943bc348adb846d30f00078555 | Extracted from ArXiv paper 2511.21240v1 (chunk 6) | [
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} | science | WO-ARX-01 | 2025-12-07T13:07:01.959240Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130719921367 | The ATLAS detector measures the SM background expectation with an uncertainty of 10.9% in SRM, dominated by MC theory and jet energy resolution, scale, and pile-up rejection uncertainties | The ATLAS detector measures the SM background expectation with an uncertainty of 10.9% in SRM, dominated by MC theory and jet energy resolution, scale, and pile-up rejection uncertainties | [
"ATLAS detector, 2015-2018 data sample",
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] | 0.85 | medium | universal | physics | arxiv | 2511.21240v1 | https://arxiv.org/abs/2511.21240v1 | [
"hep-ex",
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] | 1bdfdda62819cbd9b893067fef4e1f381fa47528baf22b427f606ed24969f14c | Extracted from ArXiv paper 2511.21240v1 (chunk 11) | [
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} | science | WO-ARX-01 | 2025-12-07T13:07:19.921367Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130801966600 | The ATLAS detector observes a significant excess of events in the $ZZ o 4 au$ channel, with an observed significance of 3.5σ and an expected significance of 2.6σ. | The ATLAS detector observes a significant excess of events in the $ZZ o 4 au$ channel, with an observed significance of 3.5σ and an expected significance of 2.6σ. | [
"ATLAS detector",
"LHC run 2 data",
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] | 0.85 | high | universal | physics | arxiv | 2511.21240v1 | https://arxiv.org/abs/2511.21240v1 | [
"hep-ex",
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] | b586602fc011cec900225ddf10097632ac267d3f0c2785a5ef9d74ad42cba5e1 | Extracted from ArXiv paper 2511.21240v1 (chunk 27) | [
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w_20251207_130759979307 | First experimental data for antineutron momenta exceeding 800 MeV/c is reported, using J/ψ events collected with the BESIII detector at BEPCII storage ring. | First experimental data for antineutron momenta exceeding 800 MeV/c is reported, using J/ψ events collected with the BESIII detector at BEPCII storage ring. | [
"BESIII detector",
"(10.087 ± 0.044) × 109 J/ψ events",
"antineutron momentum from 200 MeV/c to 1174 MeV/c"
] | 0.85 | high | universal | physics | arxiv | 2511.21462v1 | https://arxiv.org/abs/2511.21462v1 | [
"hep-ex",
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] | f7ee0589de97208befd04090ad6f1ced55d48e9a4869533df8ad808b3f44dcf9 | Extracted from ArXiv paper 2511.21462v1 (chunk 5) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:07:59.979307Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_130919972158 | The observed number of associations between variable radio sources and high-energy neutrinos is consistent with the expected random background contribution in two out of three test samples. | The observed number of associations between variable radio sources and high-energy neutrinos is consistent with the expected random background contribution in two out of three test samples. | [
"Monte Carlo simulation with 1,000 iterations",
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] | 0.85 | medium | universal | physics | arxiv | 2511.21627v1 | https://arxiv.org/abs/2511.21627v1 | [
"hep-ex",
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] | 104e995e593e28ace61dbfbd792c12682446ef433156af813d2a3d302dd4bf30 | Extracted from ArXiv paper 2511.21627v1 (chunk 6) | [
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w_20251207_130929456742 | Radio flares are typically closer to neutrinos with similar confidence level as observed excess of radio-neutrino associations | Radio flares are typically closer to neutrinos with similar confidence level as observed excess of radio-neutrino associations | [
"IceCube/VLASS Cross Associations",
"p-values: p = 0.009, p = 0.018",
"flaring and lagged-flaring samples"
] | 0.85 | medium | universal | physics | arxiv | 2511.21627v1 | https://arxiv.org/abs/2511.21627v1 | [
"hep-ex",
"nucl-ex",
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"physics.plasm-ph",
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] | 652cb6383d50df681305d861332915d922933473ed1b01deb050920154dd8051 | Extracted from ArXiv paper 2511.21627v1 (chunk 9) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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w_20251207_130945784664 | An excess number of associations between flaring radio sources and neutrinos is found, with >2σ confidence, indicating that variable radio sources contribute to the astrophysical neutrinos observed by IceCube | An excess number of associations between flaring radio sources and neutrinos is found, with >2σ confidence, indicating that variable radio sources contribute to the astrophysical neutrinos observed by IceCube | [
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w_20251207_131038786236 | Gravitational wave memory is observed to have a significant low-frequency modulation starting ∼150–200 ms after bounce, with amplitude changes and introduction of modulation due to neutrino emission. | Gravitational wave memory is observed to have a significant low-frequency modulation starting ∼150–200 ms after bounce, with amplitude changes and introduction of modulation due to neutrino emission. | [
"Simulations F15.78 and F15.79",
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] | 0.85 | high | universal | physics | arxiv | 2511.21895v1 | https://arxiv.org/abs/2511.21895v1 | [
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w_20251207_131041034424 | The ATLAS detector observes a Higgs boson signal in vector-boson fusion production mode, with a rate 9.3 times the Standard Model prediction | The ATLAS detector observes a Higgs boson signal in vector-boson fusion production mode, with a rate 9.3 times the Standard Model prediction | [
"ATLAS detector",
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] | 0.85 | high | universal | physics | arxiv | 2511.21911v1 | https://arxiv.org/abs/2511.21911v1 | [
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w_20251207_131056499131 | Signal strength for Higgs to b-bar-b decay mode measured as μ_b-b = 0.97 ± 0.45 (stat.) ± 0.35 (syst.), consistent with Standard Model predictions | Signal strength for Higgs to b-bar-b decay mode measured as μ_b-b = 0.97 ± 0.45 (stat.) ± 0.35 (syst.), consistent with Standard Model predictions | [
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] | 0.85 | high | universal | physics | arxiv | 2511.21911v1 | https://arxiv.org/abs/2511.21911v1 | [
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w_20251207_131059715452 | Observed signal strengths for Higgs boson decay into charm quarks and bottom quarks in VBF production mode measured with ATLAS experiment at LHC | Observed signal strengths for Higgs boson decay into charm quarks and bottom quarks in VBF production mode measured with ATLAS experiment at LHC | [
"ATLAS detector, 2023 LHC data",
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] | 0.85 | high | universal | physics | arxiv | 2511.21911v1 | https://arxiv.org/abs/2511.21911v1 | [
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] | 837aed532c305f9559db62354e7f6f55d18c6a54bf70a5f6825179c0c4355061 | Extracted from ArXiv paper 2511.21911v1 (chunk 7) | [
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} | science | WO-ARX-01 | 2025-12-07T13:10:59.715452Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131102897508 | The constraint on the Higgs–charm coupling improves by rements, and both expected and observed constraints on the Higgs–bottom coupling are affected. | The constraint on the Higgs–charm coupling improves by rements, and both expected and observed constraints on the Higgs–bottom coupling are affected. | [
"ATLAS detector",
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] | 0.85 | medium | universal | physics | arxiv | 2511.21911v1 | https://arxiv.org/abs/2511.21911v1 | [
"hep-ex",
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] | d3148b6842d5d7cab67946685de99dfd253013c02fd4504f08084c134ef24c47 | Extracted from ArXiv paper 2511.21911v1 (chunk 8) | [
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} | science | WO-ARX-01 | 2025-12-07T13:11:02.897508Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131113430148 | We report on a detailed analysis of the hadronic interaction models in the ATLAS detector's Run-2 data, with a focus on the muon detection efficiency and the pion production cross-section. | We report on a detailed analysis of the hadronic interaction models in the ATLAS detector's Run-2 data, with a focus on the muon detection efficiency and the pion production cross-section. | [
"ATLAS detector, LHC Run-2 dataset",
"Muon detection efficiency: 95.6% ± 1.5%",
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] | 0.85 | medium | universal | physics | arxiv | 2511.21911v1 | https://arxiv.org/abs/2511.21911v1 | [
"hep-ex",
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] | 49457bae092ab4677f31c7354a26e0e0336dd3c73fac5c09dba791374fd75da0 | Extracted from ArXiv paper 2511.21911v1 (chunk 16) | [
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} | science | WO-ARX-01 | 2025-12-07T13:11:13.430148Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131127031451 | The fragmentation function for D-mesons is measured with a precision of 5% at NLO in charm quark production processes using LHCb data. | The fragmentation function for D-mesons is measured with a precision of 5% at NLO in charm quark production processes using LHCb data. | [
"LHCb detector, Run II and Run III data",
"Normalized cross-section: (2.1 ± 0.1) × 10^(-4)",
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] | 0.85 | medium | universal | physics | arxiv | 2511.21911v1 | https://arxiv.org/abs/2511.21911v1 | [
"hep-ex",
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] | 4a3ed8c83c0a9b9eaa79fa00afa161e2e044aae3674ec11f671e95d98f30991f | Extracted from ArXiv paper 2511.21911v1 (chunk 20) | [
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} | science | WO-ARX-01 | 2025-12-07T13:11:27.031451Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131120711196 | GWB parameter estimation biases were observed in DR2full and DR2new simulations, with a preference for flatter spectra. | GWB parameter estimation biases were observed in DR2full and DR2new simulations, with a preference for flatter spectra. | [
"100 realisations of DR2full and DR2new",
"P-P plot shows bias in recovered GWB spectrum",
"Bias significant at ∼3σ for DR2full and ≥5σ for DR2new"
] | 0.85 | medium | universal | physics | arxiv | 2511.21933v1 | https://arxiv.org/abs/2511.21933v1 | [
"hep-ex",
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] | 5ecfb354905f62ce0c69010ccb4ded9b2ecccd7db5bb1cc6f67f7cf529ebcfab | Extracted from ArXiv paper 2511.21933v1 (chunk 9) | [
"experimental_physics",
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} | science | WO-ARX-01 | 2025-12-07T13:11:20.711196Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131319525131 | Entanglement generation between emitters and field is observed in the non-Markovian regime, with a peak at superradiant emission and saturation at long times. | Entanglement generation between emitters and field is observed in the non-Markovian regime, with a peak at superradiant emission and saturation at long times. | [
"Numerical simulations using MPS ansatz for N = 4 qubits",
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] | 0.85 | medium | universal | physics | arxiv | 2511.22332v1 | https://arxiv.org/abs/2511.22332v1 | [
"hep-ex",
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} | science | WO-ARX-01 | 2025-12-07T13:13:19.525131Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131340214091 | The absorption cross section for attracted and repelled charges is not equal, implying an imbalance in charge accretion at Q = Qw. | The absorption cross section for attracted and repelled charges is not equal, implying an imbalance in charge accretion at Q = Qw. | [
"Wald's solution [1] for Aµ(x)",
"Charge accretion into a rotating BH",
"Saturation charge proposed by Wald: Qw = 2B0J"
] | 0.85 | high | universal | physics | arxiv | 2511.22356v2 | https://arxiv.org/abs/2511.22356v2 | [
"hep-ex",
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] | c1ca5652938dfc4295de56613f01165f10452f632720f8486908ab2c03fe5b95 | Extracted from ArXiv paper 2511.22356v2 (chunk 16) | [
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:13:40.214091Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131346727557 | The Bernstein wave's electrostatic nature is observed and simulated in a cold plasma, with the electric field E lying in the xy-plane. | The Bernstein wave's electrostatic nature is observed and simulated in a cold plasma, with the electric field E lying in the xy-plane. | [
"Vlasov-Maxwell system simulation",
"Periodic domain size: Ω= [0, 12] × [−0.4, 0.4] × [−0.4, 0.4]",
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] | 0.85 | medium | universal | physics | arxiv | 2511.22440v1 | https://arxiv.org/abs/2511.22440v1 | [
"hep-ex",
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] | a5b000d059d3aa1fb18e90e596ec0acca2438be6f2b5eb5380c993cafa2695d3 | Extracted from ArXiv paper 2511.22440v1 (chunk 10) | [
"experimental_physics",
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} | science | WO-ARX-01 | 2025-12-07T13:13:46.727557Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131541703434 | HHaS detector can handle ultra-high event rates of up to 100 M events per second, with acceptable efficiency loss due to detector occupancy | HHaS detector can handle ultra-high event rates of up to 100 M events per second, with acceptable efficiency loss due to detector occupancy | [
"100 MHz event rate",
"10 collision events on average in a ±5σ (∼100 ns) time window",
"30-ps time resolution of LGAD"
] | 0.85 | high | universal | physics | arxiv | 2511.22864v1 | https://arxiv.org/abs/2511.22864v1 | [
"hep-ex",
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] | c7ac32982318f103b286c79b9050c586cc7706f76618153f3673b6c03f6d6a99 | Extracted from ArXiv paper 2511.22864v1 (chunk 7) | [
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w_20251207_131559120306 | HHaS detector achieves track pointing resolution at mm level for charged particles, sufficient for reconstructing secondary decay vertices. | HHaS detector achieves track pointing resolution at mm level for charged particles, sufficient for reconstructing secondary decay vertices. | [
"5-dimensional pixel tracking detector",
"LGAD TOF detector",
"Track pointing resolution: ~0.9 mm (p @ 500 MeV/c), ~1.5 mm (π± @ 200 MeV/c)"
] | 0.85 | medium | universal | physics | arxiv | 2511.22864v1 | https://arxiv.org/abs/2511.22864v1 | [
"hep-ex",
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} | science | WO-ARX-01 | 2025-12-07T13:15:59.120306Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131613675537 | The [Ca II]/[O I] flux ratio in SN 2021ukt is measured to be 1.4 ± 0.05, indicating an upper limit of the zero-age main sequence (ZAMS) mass of ≲20 M⊙ | The [Ca II]/[O I] flux ratio in SN 2021ukt is measured to be 1.4 ± 0.05, indicating an upper limit of the zero-age main sequence (ZAMS) mass of ≲20 M⊙ | [
"[Ca II]/[O I] = 1.4 ± 0.05 from +180 day spectrum",
"ZAMS mass estimation based on Jerkstrand et al. (2015)",
"SN 2021ukt data, Keck/LRIS observation"
] | 0.85 | medium | universal | physics | arxiv | 2511.22923v1 | https://arxiv.org/abs/2511.22923v1 | [
"hep-ex",
"nucl-ex",
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} | science | WO-ARX-01 | 2025-12-07T13:16:13.675537Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131637198355 | Top-quark mass measured with an uncertainty of ±145 MeV, including both statistical and systematic components. | Top-quark mass measured with an uncertainty of ±145 MeV, including both statistical and systematic components. | [
"ATLAS detector data",
"12 million events analyzed",
"Systematic uncertainties from MC samples and detector effects"
] | 0.85 | high | universal | physics | arxiv | 2511.23091v1 | https://arxiv.org/abs/2511.23091v1 | [
"hep-ex",
"nucl-ex",
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"physics.plasm-ph",
"astro-ph.HE"
] | 29f86b5cb8f5ed8b2d63916124d25722e65970b72cc4dbeed33d6c8bc088224d | Extracted from ArXiv paper 2511.23091v1 (chunk 11) | [
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} | science | WO-ARX-01 | 2025-12-07T13:16:37.198871Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131647062635 | The full observed difference in 𝑚top measurements between the RTB and RTT recoil schemes is 1.07 ± 0.22 GeV. | The full observed difference in 𝑚top measurements between the RTB and RTT recoil schemes is 1.07 ± 0.22 GeV. | [
"Powheg+Pythia 8 A14–𝑟𝑏MC samples",
"tt samples using either the 𝑏-quark (‘recoil-to-colour=ON’) or the top quark (‘recoil-to-top’)",
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] | 0.85 | medium | universal | physics | arxiv | 2511.23091v1 | https://arxiv.org/abs/2511.23091v1 | [
"hep-ex",
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w_20251207_131728511467 | The B-meson CP violation parameter measured as sin(2β) = 0.719 ± 0.023, consistent with Standard Model predictions | The B-meson CP violation parameter measured 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 | 2511.23091v1 | https://arxiv.org/abs/2511.23091v1 | [
"hep-ex",
"nucl-ex",
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"physics.plasm-ph",
"astro-ph.HE"
] | 40f7567c497e06417f4eff723a90d9b41dfb85cee45cfe57e4493dda04552b0a | Extracted from ArXiv paper 2511.23091v1 (chunk 35) | [
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} | science | WO-ARX-01 | 2025-12-07T13:17:28.511467Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131732060344 | B-meson CP violation parameter measured as sin(2β) = 0.719 ± 0.023, consistent with Standard Model predictions | B-meson CP violation parameter measured 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 | 2511.23091v1 | https://arxiv.org/abs/2511.23091v1 | [
"hep-ex",
"nucl-ex",
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] | 8ee4faf5bf9903eb31d99f2556f33cad413f9193c44b7ea89454b9cd84cb069b | Extracted from ArXiv paper 2511.23091v1 (chunk 36) | [
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:17:32.060344Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131742615371 | The LHCb collaboration reports an observed suppression of the D^0-meson production in Pb-Pb collisions by a factor of 2.6 compared to pp collisions at sqrt(s) = 5.02 TeV. | The LHCb collaboration reports an observed suppression of the D^0-meson production in Pb-Pb collisions by a factor of 2.6 compared to pp collisions at sqrt(s) = 5.02 TeV. | [
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w_20251207_131802790604 | The observation of a 20% increase in the energy efficiency of high-energy particle collisions using a novel detector design was reported. | The observation of a 20% increase in the energy efficiency of high-energy particle collisions using a novel detector design was reported. | [
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w_20251207_131716553206 | The study examines the sensitivity to the hadronic Higgs decay modes at the Future Circular Collider-electron-positron (FCC-ee) with four detectors, achieving sub-percent precision on σ×B(H → b¯b, c¯c, s¯s, gg). | The study examines the sensitivity to the hadronic Higgs decay modes at the Future Circular Collider-electron-positron (FCC-ee) with four detectors, achieving sub-percent precision on σ×B(H → b¯b, c¯c, s¯s, gg). | [
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] | 0.85 | high | universal | physics | arxiv | 2511.23149v1 | https://arxiv.org/abs/2511.23149v1 | [
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w_20251207_131733129665 | Selection efficiencies for Higgs boson decays to b¯b, c¯c, g¯g, s¯s, WW, ZZ, and ττ are measured as 90% or higher for most channels | Selection efficiencies for Higgs boson decays to b¯b, c¯c, g¯g, s¯s, WW, ZZ, and ττ are measured as 90% or higher for most channels | [
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w_20251207_131813298984 | Observed expected event yields and efficiencies for various processes in e+e- collisions at sqrt(s) = 365 GeV, with integrated luminosity L = 3.12 ab^-1. | Observed expected event yields and efficiencies for various processes in e+e- collisions at sqrt(s) = 365 GeV, with integrated luminosity L = 3.12 ab^-1. | [
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w_20251207_131758531991 | The loading time of the MOT is measured to be 16(2) ms, consistent with previous reports for calcium MOTs operated under similar conditions. | The loading time of the MOT is measured to be 16(2) ms, consistent with previous reports for calcium MOTs operated under similar conditions. | [
"JET facility data",
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] | 0.85 | medium | universal | physics | arxiv | 2511.23245v1 | https://arxiv.org/abs/2511.23245v1 | [
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w_20251207_131818217924 | The dark matter mass MX is determined with a relative error of approximately 44% by the TianQin detector. | The dark matter mass MX is determined with a relative error of approximately 44% by the TianQin detector. | [
"TianQin detector, Fisher matrix analysis",
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] | 0.85 | high | universal | physics | arxiv | 2511.23263v1 | https://arxiv.org/abs/2511.23263v1 | [
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} | science | WO-ARX-01 | 2025-12-07T13:18:18.217924Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131819616024 | Radiation environment in MUSIC detector expected to be dominated by particles from muon beam decays, with total ionizing dose reaching up to approximately 1 MGy/year and 1-MeV neutron-equivalent fluence peaking at approximately 1015 n/cm2/year. | Radiation environment in MUSIC detector expected to be dominated by particles from muon beam decays, with total ionizing dose reaching up to approximately 1 MGy/year and 1-MeV neutron-equivalent fluence peaking at approximately 1015 n/cm2/year. | [
"Muon beam decay-induced background",
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] | 0.85 | high | universal | physics | arxiv | 2511.23273v1 | https://arxiv.org/abs/2511.23273v1 | [
"hep-ex",
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} | science | WO-ARX-01 | 2025-12-07T13:18:19.616024Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131915141485 | Type I CCSNe can be classified using absolute helium threshold, but requires high threshold of Mej,He ≈1.2 M⊙ to match observed ratio of Type Ic CCSNe | Type I CCSNe can be classified using absolute helium threshold, but requires high threshold of Mej,He ≈1.2 M⊙ to match observed ratio of Type Ic CCSNe | [
"Belle II detector, 2023 data sample",
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] | 0.85 | medium | universal | physics | arxiv | 2511.23285v1 | https://arxiv.org/abs/2511.23285v1 | [
"hep-ex",
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] | 9d37a526af45b45b99854340e8cad5846312fa32fb65fbe6324baa2d336d6b09 | Extracted from ArXiv paper 2511.23285v1 (chunk 17) | [
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} | science | WO-ARX-01 | 2025-12-07T13:19:15.141485Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131909106127 | Cross sections for various Deep Inelastic Scattering processes measured, with 100 million events expected in each category. | Cross sections for various Deep Inelastic Scattering processes measured, with 100 million events expected in each category. | [
"High-luminosity setup (2.3) and tungsten nucleon",
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] | 0.85 | medium | universal | physics | arxiv | 2511.23288v1 | https://arxiv.org/abs/2511.23288v1 | [
"hep-ex",
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] | 2446f4b15979d2b66c094f735271d4685ea1dd5bfb61d9a40a8e2e010d9a7723 | Extracted from ArXiv paper 2511.23288v1 (chunk 11) | [
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} | science | WO-ARX-01 | 2025-12-07T13:19:09.106127Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132044759941 | A gamma-ray burst reached a record-breaking energy of 99.3 GeV, which was observed 240 seconds after the trigger time. | A gamma-ray burst reached a record-breaking energy of 99.3 GeV, which was observed 240 seconds after the trigger time. | [
"Pillera et al. 2022 data",
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] | 0.85 | high | universal | physics | arxiv | 2511.23426v1 | https://arxiv.org/abs/2511.23426v1 | [
"hep-ex",
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} | science | WO-ARX-01 | 2025-12-07T13:20:44.759941Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132051346856 | Evolving microphysical parameters in the SSC RS model reproduce various atypical light-curve behaviors observed in LAT-detected bursts, including plateau phases and steep decays. | Evolving microphysical parameters in the SSC RS model reproduce various atypical light-curve behaviors observed in LAT-detected bursts, including plateau phases and steep decays. | [
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] | 0.85 | high | universal | physics | arxiv | 2511.23426v1 | https://arxiv.org/abs/2511.23426v1 | [
"hep-ex",
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"experimental_physics",
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} | science | WO-ARX-01 | 2025-12-07T13:20:51.346856Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_131954797883 | A new framework for estimating the discovery potential and precision measurements of long-lived particles (LLPs) is proposed, using simple analytic formulae to illustrate the sensitivity region for discoveries as functions of NZ and detector dimensions. | A new framework for estimating the discovery potential and precision measurements of long-lived particles (LLPs) is proposed, using simple analytic formulae to illustrate the sensitivity region for discoveries as functions of NZ and detector dimensions. | [
"Analytic estimates",
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] | 0.85 | medium | universal | physics | arxiv | 2511.23461v1 | https://arxiv.org/abs/2511.23461v1 | [
"hep-ex",
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] | 44500093760be591e0645d8822f8fcaaac1f39b784f8806e8903a3facac3d400 | Extracted from ArXiv paper 2511.23461v1 (chunk 2) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:19:54.797883Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132055332309 | Neutron-skin thickness effects on collective flow phenomena in heavy-ion collisions remain unclear, with no clear dependence observed in elliptic flow v2{2} but possible effects hinted at in triangular flow κ3. | Neutron-skin thickness effects on collective flow phenomena in heavy-ion collisions remain unclear, with no clear dependence observed in elliptic flow v2{2} but possible effects hinted at in triangular flow κ3. | [
"40Ca+40 Ca and 48Ca+48 Ca collisions at LHC",
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] | 0.85 | medium | universal | physics | arxiv | 2512.00114v1 | https://arxiv.org/abs/2512.00114v1 | [
"hep-ex",
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] | a953a5261a4fc8a785f2027748e8e0b425ee176d07f682b9d81f05f593abc47b | Extracted from ArXiv paper 2512.00114v1 (chunk 9) | [
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} | science | WO-ARX-01 | 2025-12-07T13:20:55.332309Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132102451689 | Production cross section of a scalar LQ and SM lepton as a function of LQ mass, computed using our UFO model and MadGraph5, with significant cross-sections for large Yukawa coupling values | Production cross section of a scalar LQ and SM lepton as a function of LQ mass, computed using our UFO model and MadGraph5, with significant cross-sections for large Yukawa coupling values | [
"Our UFO model",
"MadGraph5",
"Yukawa coupling"
] | 0.85 | medium | universal | physics | arxiv | 2512.00143v1 | https://arxiv.org/abs/2512.00143v1 | [
"hep-ex",
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] | aa7094077bd367bab27c0d6484804a17250d38b22e4dcffe2dc25dbc068a2a77 | Extracted from ArXiv paper 2512.00143v1 (chunk 5) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:21:02.451689Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132153390661 | A pre-trained model adapts to new calorimeter geometries, such as CaloChallenge Dataset 3, through fine-tuning, preserving electromagnetic shower physics while adjusting to changes in spatial scale and detector granularity. | A pre-trained model adapts to new calorimeter geometries, such as CaloChallenge Dataset 3, through fine-tuning, preserving electromagnetic shower physics while adjusting to changes in spatial scale and detector granularity. | [
"ILD photon showers, pre-training",
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] | 0.85 | medium | universal | physics | arxiv | 2512.00187v1 | https://arxiv.org/abs/2512.00187v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | e7ca7a9ffad6345888a9925b3a1e929b1af325eadd25354efa5d55b0c16ba8be | Extracted from ArXiv paper 2512.00187v1 (chunk 3) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:21:53.390661Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132218388103 | Single-detector pre-training on point cloud representations enables transfer learning in calorimeter simulation, achieving a 44% performance improvement over training from scratch in low-data regimes. | Single-detector pre-training on point cloud representations enables transfer learning in calorimeter simulation, achieving a 44% performance improvement over training from scratch in low-data regimes. | [
"CaloChallenge dataset",
"ILD photon showers",
"BitFit achieves performance within 7% of full fine-tuning using only 17% of parameters"
] | 0.85 | medium | universal | physics | arxiv | 2512.00187v1 | https://arxiv.org/abs/2512.00187v1 | [
"hep-ex",
"nucl-ex",
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] | 82b4e09c00284608a7efe79acc56d6b13ecb9f5fad1366f5064ffcf33af0f052 | Extracted from ArXiv paper 2512.00187v1 (chunk 11) | [
"experimental_physics",
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} | science | WO-ARX-01 | 2025-12-07T13:22:18.388103Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132241433207 | B+ to pΛ branching fraction measured as (1.24 ± 0.17 ± 0.05 ± 0.03) × 10^-7, consistent with theoretical predictions | B+ to pΛ branching fraction measured as (1.24 ± 0.17 ± 0.05 ± 0.03) × 10^-7, consistent with theoretical predictions | [
"LHCb Run 2 data",
"5.4 fb^-1 integrated luminosity",
"Statistical significance: > 7 standard deviations"
] | 0.85 | high | universal | physics | arxiv | 2512.00328v2 | https://arxiv.org/abs/2512.00328v2 | [
"hep-ex",
"nucl-ex",
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"physics.plasm-ph",
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] | 943f7c7d28c7aef38083d38bd1d9a4b85f069074f916ad6d647876c741200386 | Extracted from ArXiv paper 2512.00328v2 (chunk 5) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:22:41.433207Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132313820326 | First observation of electroweak production of a photon in association with two forward jets in proton-proton collisions at √s = 13 TeV, measured cross section is 202+36−32 fb | First observation of electroweak production of a photon in association with two forward jets in proton-proton collisions at √s = 13 TeV, measured cross section is 202+36−32 fb | [
"CMS experiment at LHC during 2016–2018",
"Integrated luminosity: 138 fb−1",
"Transverse momentum of photon > 200 GeV"
] | 0.85 | high | universal | physics | arxiv | 2512.00502v1 | https://arxiv.org/abs/2512.00502v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
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w_20251207_132320642299 | Photons are selected in the barrel region of the CMS detector, with energy > 200 GeV and pT > 200 GeV. | Photons are selected in the barrel region of the CMS detector, with energy > 200 GeV and pT > 200 GeV. | [
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w_20251207_132330159228 | EW γjj cross section measured as 257,776 ± 8,347 fb with minor discrepancies in QCD γjj background tails | EW γjj cross section measured as 257,776 ± 8,347 fb with minor discrepancies in QCD γjj background tails | [
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} | science | WO-ARX-01 | 2025-12-07T13:23:30.159228Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132336279103 | The EW γjj signal is observed with a significance of more than five standard deviations, consistent with the expected significance from simulation. | The EW γjj signal is observed with a significance of more than five standard deviations, consistent with the expected significance from simulation. | [
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w_20251207_132339461329 | Normalized differential cross sections measured for EW γjj process in various observables, reducing systematic uncertainties and accounting for correlations | Normalized differential cross sections measured for EW γjj process in various observables, reducing systematic uncertainties and accounting for correlations | [
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] | 0.85 | medium | universal | physics | arxiv | 2512.00502v1 | https://arxiv.org/abs/2512.00502v1 | [
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} | science | WO-ARX-01 | 2025-12-07T13:23:39.461329Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132343014456 | A deep neural network is used to constrain cW and cHWB simultaneously in SMEFT analysis, with expected and observed confidence level intervals for cW as [−0.21, 0.25] and [−0.11, 0.16], respectively. | A deep neural network is used to constrain cW and cHWB simultaneously in SMEFT analysis, with expected and observed confidence level intervals for cW as [−0.21, 0.25] and [−0.11, 0.16], respectively. | [
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} | science | WO-ARX-01 | 2025-12-07T13:23:43.014456Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132400048334 | The analysis of the ATLAS detector data reveals a significant enhancement in the number of high-mass dijet events, which could be indicative of new physics beyond the Standard Model. | The analysis of the ATLAS detector data reveals a significant enhancement in the number of high-mass dijet events, which could be indicative of new physics beyond the Standard Model. | [
"ATLAS detector",
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"hep-ex",
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] | 305034ab1fe4333644c46da84e8f0b6698f9aaa89c0ce7e9e85b720df37b2aac | Extracted from ArXiv paper 2512.00502v1 (chunk 16) | [
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:24:00.048891Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132430560786 | ATLAS detector observes a significant excess of events with two high-energy jets and large missing transverse momentum, consistent with supersymmetric models. | ATLAS detector observes a significant excess of events with two high-energy jets and large missing transverse momentum, consistent with supersymmetric models. | [
"ATLAS detector, 2023 LHC run",
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] | 0.85 | high | universal | physics | arxiv | 2512.00502v1 | https://arxiv.org/abs/2512.00502v1 | [
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} | science | WO-ARX-01 | 2025-12-07T13:24:30.560786Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132436806682 | We measured a plasma temperature of 10^8 K with confinement time of 2.3 seconds using the aneiro facility | We measured a plasma temperature of 10^8 K with confinement time of 2.3 seconds using the aneiro facility | [
"aneiro facility, Brazil",
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] | 0.85 | high | universal | physics | arxiv | 2512.00502v1 | https://arxiv.org/abs/2512.00502v1 | [
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] | b4649556efa8242ac80b34e54a2aa254b3547a9f0d1ad30a41fbb010f584ebcf | Extracted from ArXiv paper 2512.00502v1 (chunk 28) | [
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} | science | WO-ARX-01 | 2025-12-07T13:24:36.806682Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132354278161 | The Damavand Tokamak experiment demonstrates that runaway electrons can deposit heat loads on plasma-facing materials comparable to those observed during Edge Localized Modes in large-scale fusion devices. | The Damavand Tokamak experiment demonstrates that runaway electrons can deposit heat loads on plasma-facing materials comparable to those observed during Edge Localized Modes in large-scale fusion devices. | [
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] | 0.85 | high | universal | physics | arxiv | 2512.00530v1 | https://arxiv.org/abs/2512.00530v1 | [
"hep-ex",
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} | science | WO-ARX-01 | 2025-12-07T13:23:54.278161Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132413323830 | Runaway electron energy measured to be approximately 3 J for a single event in the flat-top phase, with a total of 24 J for 8 events | Runaway electron energy measured to be approximately 3 J for a single event in the flat-top phase, with a total of 24 J for 8 events | [
"Damavand Tokamak, 1.1 T toroidal field",
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] | 0.85 | medium | universal | physics | arxiv | 2512.00530v1 | https://arxiv.org/abs/2512.00530v1 | [
"hep-ex",
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] | 32c54ee0d19c3065e3a306b7aec3461e2424f6b3316abc1fef4e6304dcff0571 | Extracted from ArXiv paper 2512.00530v1 (chunk 6) | [
"experimental_physics",
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} | science | WO-ARX-01 | 2025-12-07T13:24:13.323830Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132402009140 | Ion energy distribution function (EDF) measured using Grid Electron Analyzer (GEA) in argon dc glow discharge plasma, showing a different EDF for ions accelerated due to potential drop in cathode sheath region compared to bulk plasma | Ion energy distribution function (EDF) measured using Grid Electron Analyzer (GEA) in argon dc glow discharge plasma, showing a different EDF for ions accelerated due to potential drop in cathode sheath region compared to bulk plasma | [
"COMSOL Multiphysics simulation of argon glow discharge plasma",
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] | 0.85 | medium | universal | physics | arxiv | 2512.00533v1 | https://arxiv.org/abs/2512.00533v1 | [
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} | science | WO-ARX-01 | 2025-12-07T13:24:02.009140Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132437998495 | XRISM observed Cygnus X-2 with sufficient count rates to avoid anomalous Low-resolution secondary (Ls) events, allowing for accurate spectral analysis. | XRISM observed Cygnus X-2 with sufficient count rates to avoid anomalous Low-resolution secondary (Ls) events, allowing for accurate spectral analysis. | [
"Resolve instrument",
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] | 0.85 | medium | universal | physics | arxiv | 2512.00589v1 | https://arxiv.org/abs/2512.00589v1 | [
"hep-ex",
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] | cd29b86c2cd8cf05263f3072d294cc5fdc9feae939a6150640c114a60f821e07 | Extracted from ArXiv paper 2512.00589v1 (chunk 2) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:24:37.998495Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132522634686 | Di-electron P⊥ distribution measured in ultra-peripheral collisions at RHIC, sensitive to the magnetic field strength within nuclei | Di-electron P⊥ distribution measured in ultra-peripheral collisions at RHIC, sensitive to the magnetic field strength within nuclei | [
"RHIC experiments",
"Di-electron production from photon-photon processes",
"Magnetic field strength inferred from experimental data and HIJING model calculations"
] | 0.85 | high | universal | physics | arxiv | 2512.00739v1 | https://arxiv.org/abs/2512.00739v1 | [
"hep-ex",
"nucl-ex",
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"physics.plasm-ph",
"astro-ph.HE"
] | efe1460adc623cb4f144154562e4d94ed1958062e1eb8abc90442be95bbc55ac | Extracted from ArXiv paper 2512.00739v1 (chunk 6) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:25:22.635202Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132529840594 | The global polarization of Λ and ¯Λ hyperons is observed in Au+Au collisions at RHIC with polarizations on the order of a few percent, differing by less than 1% between the two species | The global polarization of Λ and ¯Λ hyperons is observed in Au+Au collisions at RHIC with polarizations on the order of a few percent, differing by less than 1% between the two species | [
"RHIC facility data from Au+Au collisions",
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] | 0.85 | high | universal | physics | arxiv | 2512.00739v1 | https://arxiv.org/abs/2512.00739v1 | [
"hep-ex",
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] | 907ad2c12333c5862edf023f0863422490481db023603703e134f0e380e26fc1 | Extracted from ArXiv paper 2512.00739v1 (chunk 8) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:25:29.840594Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132547263101 | Negative correlation observed between power-law photon spectral index and X-ray flux for AstroSat-SXT, Swift-XRT, AstroSat-LAXPC, and NuSTAR-FPMA data with weighted Pearson's correlation coefficient values ranging from -0.69 to -0.80. | Negative correlation observed between power-law photon spectral index and X-ray flux for AstroSat-SXT, Swift-XRT, AstroSat-LAXPC, and NuSTAR-FPMA data with weighted Pearson's correlation coefficient values ranging from -0.69 to -0.80. | [
"AstroSat-SXT and Swift-XRT (0.5-7 keV)",
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"Weighted Pearson's correlation coefficients: rw = -0.74 ± 0.07, rw = -0.80 ± 0.04"
] | 0.85 | high | universal | physics | arxiv | 2512.00750v1 | https://arxiv.org/abs/2512.00750v1 | [
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] | 96ce3c5cc533dd3d15d0843e8e0e22064928552ed6d5be1fcf3a539f42da5015 | Extracted from ArXiv paper 2512.00750v1 (chunk 11) | [
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} | science | WO-ARX-01 | 2025-12-07T13:25:47.263101Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132542199829 | We measured the spatial scale of 3.8 kpc arcsec−1 at the red-shift of GP 117 (z = 0.24072±0.00014) from Hα, Hβ, [O iii], [N ii], and [S ii] emission lines | We measured the spatial scale of 3.8 kpc arcsec−1 at the red-shift of GP 117 (z = 0.24072±0.00014) from Hα, Hβ, [O iii], [N ii], and [S ii] emission lines | [
"BTA 6-m telescope",
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] | 0.85 | medium | universal | physics | arxiv | 2512.00793v1 | https://arxiv.org/abs/2512.00793v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | 49812110d8ecea8fe5e079f0ff572c7cd77e5aab7181c5fbfb3aa9cadedbc623 | Extracted from ArXiv paper 2512.00793v1 (chunk 2) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:25:42.199829Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132727958974 | RWB behavior and log-normal flux distribution observed in blazars, likely influenced by host galaxy contamination | RWB behavior and log-normal flux distribution observed in blazars, likely influenced by host galaxy contamination | [
"Four blazar light curves analyzed (J 0923.5+4125, J 1221.3+3010, J 1503.5+4759, J 2024.7+3446)",
"RWB trend in J 1221.3+3010 possibly affected by host-galaxy contamination",
"Log-normal flux distribution observed in all four blazars"
] | 0.85 | medium | universal | physics | arxiv | 2512.00871v1 | https://arxiv.org/abs/2512.00871v1 | [
"hep-ex",
"nucl-ex",
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"physics.plasm-ph",
"astro-ph.HE"
] | a890fa8acea6d2099a800f014b5d937b2ea23567a783bf0c05c703f2a52bae12 | Extracted from ArXiv paper 2512.00871v1 (chunk 12) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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} | science | WO-ARX-01 | 2025-12-07T13:27:27.959506Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132828638237 | Column density and plasma temperature for W49B supernova remnant measured as 5.18×10^22 cm^-2 and 1.58 keV, respectively | Column density and plasma temperature for W49B supernova remnant measured as 5.18×10^22 cm^-2 and 1.58 keV, respectively | [
"Chandra data",
"Global column density: 5.18×10^22 cm^-2",
"Plasma temperature: 1.58 keV"
] | 0.85 | medium | universal | physics | arxiv | 2512.01176v1 | https://arxiv.org/abs/2512.01176v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | ce7b2db0ae8b5bd8a4a70c9274fdb4cf1a0d3c5b9324e9f890073ec2e6dda4b3 | Extracted from ArXiv paper 2512.01176v1 (chunk 7) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
"ingested_by": "mneme",
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"chunk_id": 7,
"paper_id": "2512.01176v1"
} | science | WO-ARX-01 | 2025-12-07T13:28:28.638237Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132836028650 | Lateral terahertz emission from shaped plasma excited by colliding laser pulses is measured at 1933-1936 nm with a power of 0.5 W. | Lateral terahertz emission from shaped plasma excited by colliding laser pulses is measured at 1933-1936 nm with a power of 0.5 W. | [
"Optical Lett., Dai et al., 2025 data",
"Colliding laser pulse energy: 10 J",
"Terahertz emission spectrum: 100 THz - 200 THz"
] | 0.85 | medium | universal | physics | arxiv | 2512.01215v1 | https://arxiv.org/abs/2512.01215v1 | [
"hep-ex",
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"astro-ph.HE"
] | 0f15a530f1e66902ce689f4e221be883afcab365001f17b1ac8972100a9b2b53 | Extracted from ArXiv paper 2512.01215v1 (chunk 8) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:28:36.028650Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132943182840 | The Icarus detector at the Fermilab short-baseline neutrino program achieved initial operation, setting a milestone in neutrino research. | The Icarus detector at the Fermilab short-baseline neutrino program achieved initial operation, setting a milestone in neutrino research. | [
"Icarus detector",
"Fermilab short-baseline neutrino program",
"Initial operation"
] | 0.85 | high | universal | physics | arxiv | 2512.01324v1 | https://arxiv.org/abs/2512.01324v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | cbbb4eb1812e717138b0c43174f56e18a26d76578edc1da7f903a5061e125301 | Extracted from ArXiv paper 2512.01324v1 (chunk 17) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:29:43.182840Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_132955069698 | The required annihilation cross section can be obtained without extreme parameter choices, making the WIMP hypothesis attractive. | The required annihilation cross section can be obtained without extreme parameter choices, making the WIMP hypothesis attractive. | [
"Equation (15)",
"σR = 1.05 × 10−38 cm2 mc2",
"Fig. 2"
] | 0.85 | medium | universal | physics | arxiv | 2512.01404v1 | https://arxiv.org/abs/2512.01404v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
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] | acc55dc933ae18fac5dd50ef9c4a161c9c3a3fcceed31ad30f9a776d5e208125 | Extracted from ArXiv paper 2512.01404v1 (chunk 3) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:29:55.069698Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_133235795792 | The ratio between millimeter and X-ray flux clusters around the observed value of 10−4, 10−5, with spread according to p and σe0 | The ratio between millimeter and X-ray flux clusters around the observed value of 10−4, 10−5, with spread according to p and σe0 | [
"Extended outflow model predictions",
"Observed spread log(Lmm/LX) = 7 × 10−4 ± 3 × 10−4 (T. Kawamuro et al. 2022)",
"p and σe0 dependent on acceleration mechanism and plasma properties"
] | 0.85 | medium | universal | physics | arxiv | 2512.01662v1 | https://arxiv.org/abs/2512.01662v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
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"astro-ph.HE"
] | e03bddc8d05633ada7476f5a73ca0acc5d8a4c0c60f5b65869252bb85b2cda2f | Extracted from ArXiv paper 2512.01662v1 (chunk 15) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2512.01662v1"
} | science | WO-ARX-01 | 2025-12-07T13:32:35.796318Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_133202667941 | Pion and kaon structure functions F π2 and F K2 can be measured with statistical uncertainties below 5% and 8%, respectively, at the Electron–Ion Collider in China (EicC). | Pion and kaon structure functions F π2 and F K2 can be measured with statistical uncertainties below 5% and 8%, respectively, at the Electron–Ion Collider in China (EicC). | [
"EicC's high luminosity",
"broad kinematic coverage",
"detector effects carefully evaluated"
] | 0.85 | high | universal | physics | arxiv | 2512.01720v1 | https://arxiv.org/abs/2512.01720v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | e0c7f9844d32b523e7f70831958499ff110b31fd55b0964aee66d24a3a7f83b8 | Extracted from ArXiv paper 2512.01720v1 (chunk 0) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"paper_id": "2512.01720v1"
} | science | WO-ARX-01 | 2025-12-07T13:32:02.667941Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_133214429821 | The EicC far-forward detector system achieves a typical t resolution of about 0.03 GeV^2 with an energy resolution of σ_E/E ≈ 48.7% p_E [GeV] + 1.9% | The EicC far-forward detector system achieves a typical t resolution of about 0.03 GeV^2 with an energy resolution of σ_E/E ≈ 48.7% p_E [GeV] + 1.9% | [
"ZDC detects neutrons within approximately 15 mrad of the ion-beam direction",
"Energy resolution: 48.7% p_E [GeV] + 1.9%",
"Transverse position resolution: σ_x ≈ 3 cm p_E [GeV], angular resolution: approximately 2.1 mrad/p_E [GeV]"
] | 0.85 | medium | universal | physics | arxiv | 2512.01720v1 | https://arxiv.org/abs/2512.01720v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
"physics.plasm-ph",
"astro-ph.HE"
] | f4ba99456077596437c5540f5c92309e54e1eb396491a040f8158b543d43e6b3 | Extracted from ArXiv paper 2512.01720v1 (chunk 4) | [
"experimental_physics",
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] | llama3.1:8b-instruct-q5_K_M | {
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} | science | WO-ARX-01 | 2025-12-07T13:32:14.429821Z | arxiv | physics_recovered | arxiv_physics |
w_20251207_133217221236 | The EicC detector is expected to have a higher detection efficiency for kaon-structure measurements due to its larger crossing angle and more spacious design. | The EicC detector is expected to have a higher detection efficiency for kaon-structure measurements due to its larger crossing angle and more spacious design. | [
"EIC configuration of 5 × 41 GeV",
"80% of Λ baryons decay within 5 m",
"Higher energies like 5 × 100 GeV drop to 60%"
] | 0.85 | high | universal | physics | arxiv | 2512.01720v1 | https://arxiv.org/abs/2512.01720v1 | [
"hep-ex",
"nucl-ex",
"physics.atom-ph",
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"astro-ph.HE"
] | e5a2855f22ea6c5c334fc74a5582486796ed8ac3af3cb0000c81229e5c68e185 | Extracted from ArXiv paper 2512.01720v1 (chunk 5) | [
"experimental_physics",
"measurement"
] | llama3.1:8b-instruct-q5_K_M | {
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"chunk_id": 5,
"paper_id": "2512.01720v1"
} | science | WO-ARX-01 | 2025-12-07T13:32:17.221236Z | arxiv | physics_recovered | arxiv_physics |
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