|
SERiF v0.0.1a
Stellar Evolution and Rotation in Four Dimensions
|
A concept to determine if an EOS type can be used to compute pressure forces in the current SERiF system. This is satisfied for types that are valid EOS models, support the relation for computing pressure from specific enthalpy, and support the partial derivative of that relation with respect to specific enthalpy. More...
#include <concepts.hpp>
A concept to determine if an EOS type can be used to compute pressure forces in the current SERiF system. This is satisfied for types that are valid EOS models, support the relation for computing pressure from specific enthalpy, and support the partial derivative of that relation with respect to specific enthalpy.