/*******************************************************************************
* This file is part of SWIFT.
* Copyright (c) 2023 Orestis Karapiperis (karapiperis@lorentz.leidenuniv.nl).
*
* This program is free software: you can redistribute it and/or modify
* it under the terms of the GNU Lesser General Public License as published
* by the Free Software Foundation, either version 3 of the License, or
* (at your option) any later version.
*
* This program is distributed in the hope that it will be useful,
* but WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
* GNU General Public License for more details.
*
* You should have received a copy of the GNU Lesser General Public License
* along with this program. If not, see .
*
******************************************************************************/
#ifndef SWIFT_BAROTROPIC_GAS_EQUATION_OF_STATE_H
#define SWIFT_BAROTROPIC_GAS_EQUATION_OF_STATE_H
/* Some standard headers. */
#include
/* Local headers. */
#include "adiabatic_index.h"
#include "common_io.h"
#include "inline.h"
#include "physical_constants.h"
extern struct eos_parameters eos;
/**
* @brief The parameters of the equation of state for the gas.
*
* Barotropic equation of state from Hennebelle et al., 2008, A&A, 477, 9
* reimplemented following Pakmor et al., 2011, MNRAS, 418, 1392
*/
struct eos_parameters {
/*! Square of barotropic sound speed in vacuum */
float vacuum_sound_speed2;
/*! Inverse of the core density */
float inverse_core_density;
};
/**
* @brief Returns the internal energy given density and entropy
*
* Since we are using a barotropic EoS, the entropy value is ignored.
* Computes \f$u = c_0^2 \frac{1 + \left(\frac{\rho}{\rho_c}\right)^\gamma
* }{\gamma - 1}\f$.
*
* @param density The density \f$\rho\f$.
* @param entropy The entropy \f$A\f$.
*/
__attribute__((always_inline, const)) INLINE static float
gas_internal_energy_from_entropy(float density, float entropy) {
const float density_frac = density * eos.inverse_core_density;
const float density_factor = pow_gamma(density_frac);
return eos.vacuum_sound_speed2 * sqrtf(1.0f + density_factor) *
hydro_one_over_gamma_minus_one;
}
/**
* @brief Returns the pressure given density and entropy
*
* Since we are using a barotropic EoS, the entropy value is ignored.
* Computes \f$P = c_0^2 \left(1 +
* \left(\frac{\rho}{\rho_c}\right)^\gamma\right)\f$.
*
* @param density The density \f$\rho\f$.
* @param entropy The entropy \f$A\f$.
*/
__attribute__((always_inline, const)) INLINE static float
gas_pressure_from_entropy(float density, float entropy) {
const float density_frac = density * eos.inverse_core_density;
const float density_factor = pow_gamma(density_frac);
return eos.vacuum_sound_speed2 * density * sqrtf(1.0f + density_factor);
}
/**
* @brief Returns the entropy given density and pressure.
*
* Since we are using a barotropic EoS, the pressure value is ignored.
* Computes \f$A = \rho^{1-\gamma}c_0^2 \left(1 +
* \left(\frac{\rho}{\rho_c}\right)^\gamma\right)\f$.
*
* @param density The density \f$\rho\f$.
* @param pressure The pressure \f$P\f$.
* @return The entropy \f$A\f$.
*/
__attribute__((always_inline, const)) INLINE static float
gas_entropy_from_pressure(float density, float pressure) {
const float density_frac = density * eos.inverse_core_density;
const float density_factor = pow_gamma(density_frac);
return eos.vacuum_sound_speed2 * pow_minus_gamma_minus_one(density) *
sqrtf(1.0f + density_factor);
}
/**
* @brief Returns the sound speed given density and entropy
*
* Since we are using a barotropic EoS, the entropy is ignored.
* Computes \f$c = \sqrt{c_0^2 \left(1 +
* \left(\frac{\rho}{\rho_c}\right)^\gamma\right)}\f$.
*
* @param density The density \f$\rho\f$.
* @param entropy The entropy \f$A\f$.
*/
__attribute__((always_inline, const)) INLINE static float
gas_soundspeed_from_entropy(float density, float entropy) {
const float density_frac = density * eos.inverse_core_density;
const float density_factor = pow_gamma(density_frac);
return sqrtf(eos.vacuum_sound_speed2 * sqrtf(1.0f + density_factor));
}
/**
* @brief Returns the entropy given density and internal energy
*
* Since we are using a barotropic EoS, the internal energy value is ignored.
* Computes \f$A = \rho^{1-\gamma}c_0^2 \left(1 +
* \left(\frac{\rho}{\rho_c}\right)^\gamma\right)\f$.
*
* @param density The density \f$\rho\f$
* @param u The internal energy \f$u\f$
*/
__attribute__((always_inline, const)) INLINE static float
gas_entropy_from_internal_energy(float density, float u) {
const float density_frac = density * eos.inverse_core_density;
const float density_factor = pow_gamma(density_frac);
return eos.vacuum_sound_speed2 * pow_minus_gamma_minus_one(density) *
sqrtf(1.0f + density_factor);
}
/**
* @brief Returns the pressure given density and internal energy
*
* Since we are using a barotropic EoS, the internal energy value is ignored.
* Computes \f$P = c_0^2 \left(1 +
* \left(\frac{\rho}{\rho_c}\right)^\gamma\right)\f$.
*
* @param density The density \f$\rho\f$
* @param u The internal energy \f$u\f$
*/
__attribute__((always_inline, const)) INLINE static float
gas_pressure_from_internal_energy(float density, float u) {
const float density_frac = density * eos.inverse_core_density;
const float density_factor = pow_gamma(density_frac);
return eos.vacuum_sound_speed2 * density * sqrtf(1.0f + density_factor);
}
/**
* @brief Returns the internal energy given density and pressure.
*
* Since we are using a barotropic EoS, the pressure value is ignored.
* Computes \f$u = c_0^2 \frac{1 + \left(\frac{\rho}{\rho_c}\right)^\gamma
* }{\gamma - 1}\f$.
*
* @param density The density \f$\rho\f$.
* @param pressure The pressure \f$P\f$.
* @return The internal energy \f$u\f$.
*/
__attribute__((always_inline, const)) INLINE static float
gas_internal_energy_from_pressure(float density, float pressure) {
const float density_frac = density * eos.inverse_core_density;
const float density_factor = pow_gamma(density_frac);
return eos.vacuum_sound_speed2 * sqrtf(1.0f + density_factor) *
hydro_one_over_gamma_minus_one;
}
/**
* @brief Returns the sound speed given density and internal energy
*
* Since we are using a barotropic EoS, the internal energy value is ignored.
* Computes \f$c = \sqrt{c_0^2 \left(1 +
* \left(\frac{\rho}{\rho_c}\right)^\gamma\right)}\f$.
*
* @param density The density \f$\rho\f$
* @param u The internal energy \f$u\f$
*/
__attribute__((always_inline, const)) INLINE static float
gas_soundspeed_from_internal_energy(float density, float u) {
const float density_frac = density * eos.inverse_core_density;
const float density_factor = pow_gamma(density_frac);
return sqrtf(eos.vacuum_sound_speed2 * sqrtf(1.0f + density_factor));
}
/**
* @brief Returns the sound speed given density and pressure
*
* Since we are using a barotropic EoS, the pressure value is ignored.
* Computes \f$c = \sqrt{c_0^2 \left(1 +
* \left(\frac{\rho}{\rho_c}\right)^\gamma\right)}\f$.
*
* @param density The density \f$\rho\f$
* @param P The pressure \f$P\f$
*/
__attribute__((always_inline, const)) INLINE static float
gas_soundspeed_from_pressure(float density, float P) {
const float density_frac = density * eos.inverse_core_density;
const float density_factor = pow_gamma(density_frac);
return sqrtf(eos.vacuum_sound_speed2 * sqrtf(1.0f + density_factor));
}
/**
* @brief Initialize the eos parameters
*
* Read the vacuum sound speed and core density from the parameter file.
*
* @param e The #eos_parameters.
* @param phys_const The physical constants in the internal unit system.
* @param us The internal unit system.
* @param params The parsed parameters.
*/
INLINE static void eos_init(struct eos_parameters *e,
const struct phys_const *phys_const,
const struct unit_system *us,
struct swift_params *params) {
const float vacuum_sound_speed =
parser_get_param_float(params, "EoS:barotropic_vacuum_sound_speed");
e->vacuum_sound_speed2 = vacuum_sound_speed * vacuum_sound_speed;
e->inverse_core_density =
1. / parser_get_param_float(params, "EoS:barotropic_core_density");
}
/**
* @brief Print the equation of state
*
* @param e The #eos_parameters
*/
INLINE static void eos_print(const struct eos_parameters *e) {
message(
"Equation of state: Barotropic gas with vacuum sound speed set to %f and "
"core density set to %f.",
sqrtf(e->vacuum_sound_speed2), 1. / e->inverse_core_density);
message("Adiabatic index gamma: %f.", hydro_gamma);
}
#if defined(HAVE_HDF5)
/**
* @brief Write equation of state information to the snapshot
*
* @param h_grpsph The HDF5 group in which to write
* @param e The #eos_parameters
*/
INLINE static void eos_print_snapshot(hid_t h_grpsph,
const struct eos_parameters *e) {
io_write_attribute_f(h_grpsph, "Adiabatic index", hydro_gamma);
io_write_attribute_s(h_grpsph, "Equation of state", "Barotropic gas");
}
#endif
#endif /* SWIFT_BAROTROPIC_GAS_EQUATION_OF_STATE_H */