old_contents: # coding=utf-8
  """
  Base Library (:mod:`ibei`)
  ==========================
  
  The Bose-Einstein integral appears when calculating quantities
  pertaining to photons. It is used to derive the Stefan-Boltzmann law,
  and it also appears when calculating the detailed balance limit of a
  solar cell and other devices.
  
  The :mod:`ibei` module provides functionality to calculate various
  forms of the Bose-Einstein integral, along with well-known models of
  photovoltaic devices. The :class:`BEI` class implements the
  full, upper-incomplete, and lower-incomplete Bose-Einstein integrals
  and is the main feature of this module.
  
  
  Notes
  -----
  Arguments passed to the constructor of the :class:`BEI` class
  correspond to symbols in the expressions given below. The
  correspondence is noted in the "Parameters" section of the class
  docstring.
  
  
  The (full) Bose-Einstein integral is denoted by :math:`G_{m} (T, \mu)`
  and given by
  
  .. math::
      G_{m}(T, \mu) = \\frac{2 \pi}{h^{3} c^{2}} \int_{0}^{\infty} E^{m} \\frac{1}{\exp(\\frac{E-\mu}{kT}) - 1} dE
  
  (a glossary of symbols is given at the end of the docstring). The full
  Bose-Einstein integral can be expressed as a sum of an
  upper-incomplete (denoted :math:`G_{m} (E_{g}, T, \mu)`) and
  lower-incomplete integral (denoted :math:`g_{m} (E_{g}, T, \mu)`)
  
  .. math::
      G_{m} (T, \mu) = G_{m} (E_{g}, T, \mu) + g_{m} (E_{g}, T, \mu)
  
  where
  
  .. math::
      G_{m} (E_{g}, T, \mu) = \\frac{2 \pi}{h^{3} c^{2}} \int_{E_{g}}^{\infty} E^{m} \\frac{1}{\exp(\\frac{E-\mu}{kT}) - 1} dE
  
  and
  
  .. math::
      g_{m} (E_{g}, T, \mu) = \\frac{2 \pi}{h^{3} c^{2}} \int_{0}^{E_{g}} E^{m} \\frac{1}{\exp(\\frac{E-\mu}{kT}) - 1} dE
  
  This module provides functionality to compute each integral given
  above via the :class:`BEI` class.
  
  Symbols used in the above equations are given as follows.
  
  * :math:`h`: Planck's constant
  * :math:`c`: Speed of light
  * :math:`\mu`: Chemical potential of photons
  * :math:`E`: Energy of photons
  * :math:`T`: Absolute temperature of the radiator
  * :math:`k`: Boltzmann's constant
  """
  
  from .models import BEI, SQSolarcell, DeVosSolarcell
  
  try:
      from ._version import __version__
  except ModuleNotFoundError:
      __version__ = ""
  
new_contents: # coding=utf-8
  """
  Base Library (:mod:`ibei`)
  ==========================
  
  The Bose-Einstein integral appears when calculating quantities
  pertaining to photons. It is used to derive the Stefan-Boltzmann law,
  and it also appears when calculating the detailed balance limit of a
  solar cell and other devices.
  
  The :mod:`ibei` module provides functionality to calculate various
  forms of the Bose-Einstein integral, along with well-known models of
  photovoltaic devices. The :class:`BEI` class implements the
  full, upper-incomplete, and lower-incomplete Bose-Einstein integrals
  and is the main feature of this module.
  
  
  Notes
  -----
  Arguments passed to the constructor of the :class:`BEI` class
  correspond to symbols in the expressions given below. The
  correspondence is noted in the "Parameters" section of the class
  docstring.
  
  
  The (full) Bose-Einstein integral is denoted by :math:`G_{m} (T, \mu)`
  and given by
  
  .. math::
      G_{m}(T, \mu) = \\frac{2 \pi}{h^{3} c^{2}} \int_{0}^{\infty} E^{m} \\frac{1}{\exp(\\frac{E-\mu}{kT}) - 1} dE
  
  (a glossary of symbols is given at the end of the docstring). The full
  Bose-Einstein integral can be expressed as a sum of an
  upper-incomplete (denoted :math:`G_{m} (E_{g}, T, \mu)`) and
  lower-incomplete integral (denoted :math:`g_{m} (E_{g}, T, \mu)`)
  
  .. math::
      G_{m} (T, \mu) = G_{m} (E_{g}, T, \mu) + g_{m} (E_{g}, T, \mu)
  
  where
  
  .. math::
      G_{m} (E_{g}, T, \mu) = \\frac{2 \pi}{h^{3} c^{2}} \int_{E_{g}}^{\infty} E^{m} \\frac{1}{\exp(\\frac{E-\mu}{kT}) - 1} dE
  
  and
  
  .. math::
      g_{m} (E_{g}, T, \mu) = \\frac{2 \pi}{h^{3} c^{2}} \int_{0}^{E_{g}} E^{m} \\frac{1}{\exp(\\frac{E-\mu}{kT}) - 1} dE
  
  This module provides functionality to compute each integral given
  above via the :class:`BEI` class.
  
  Symbols used in the above equations are given as follows.
  
  .. glossary::
  
      :math:`h`: Planck's constant
      :math:`c`: Speed of light
      :math:`\mu`: Chemical potential of photons
      :math:`E`: Energy of photons
      :math:`T`: Absolute temperature of the radiator
      :math:`k`: Boltzmann's constant
  """
  
  from .models import BEI, SQSolarcell, DeVosSolarcell
  
  try:
      from ._version import __version__
  except ModuleNotFoundError:
      __version__ = ""
  
subject: Convert unordered list to glossary