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Update 2 to #331.
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Ann Elisabet Wills - 298385 committed Jan 3, 2024
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8 changes: 4 additions & 4 deletions doc/sphinx/src/models.rst
Original file line number Diff line number Diff line change
Expand Up @@ -797,7 +797,7 @@ and we arrive at

.. math::
S(\rho,T) = S_0 - \Gamma(\rho_0)C_V \eta + {C_V} \ln \frac{T}{T_{ref}} ,
S(\rho,T) = S_0 - \Gamma(\rho_0)C_V \eta + {C_V} \ln \frac{T}{T_0} ,
where :math:`\eta` is a measure of compression given by
Expand All @@ -814,7 +814,7 @@ The pressure, energy, and temperature, on the Hugoniot are derived from the
shock jump conditions,

.. math::
\rho_0 U_s = \rho (U_s - u_p)
\rho_0 U_s = \rho (U_s - u_p) \\
P_H = \rho_0 U_s u_p ,
assuming a linear :math:`U_s`-:math:`u_p` relation,
Expand All @@ -830,7 +830,7 @@ so only this :math:`s` parameter is needed. The units for :math:`C_s` is velocit
:math:`s` is unitless. Note that the parameter :math:`s` is related to the
fundamental derivative of shock physics as shown by `Wills <WillsThermo_>`_.

The reference pressure along the Hugoniot is determined by
Solving the jump equations above gives that the reference pressure along the Hugoniot is determined by

.. math::
Expand All @@ -848,7 +848,7 @@ it is
.. math::
T_H(\rho) = T_0 e^{\Gammma(\rho_0) \eta} + \frac{e^{\Gammma(\rho_0) \eta}}{2 C_V \rho_0}
\int_0^\eta e^{-\gamma(\rho_0) z} z^2 \frac{d}{dz} \left( \frac{P_H}{z}\right) dz
\int_0^\eta e^{-\gamma(\rho_0) z} z^2 \frac{d}{dz} \left( \frac{P_H}{z}\right) dz \\
= T_0 e^{\Gammma(\rho_0) \eta} + \frac{C_s^2}}{2 C_V s^2}
\left[\frac{- s \eta}{(1 - s \eta)^2} + \left( \frac{\Gamma(\rho_0)}{s} - 3 \right)
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