/******************************************************************************* * This file is part of SWIFT. * Copyright (c) 2022 Matthieu Schaller (schaller@strw.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_NONE_MHD_IACT_H #define SWIFT_NONE_MHD_IACT_H /** * @brief MHD-Density interaction between two particles. * * @param r2 Comoving square distance between the two particles. * @param dx Comoving vector separating both particles (pi - pj). * @param hi Comoving smoothing-length of particle i. * @param hj Comoving smoothing-length of particle j. * @param pi First particle. * @param pj Second particle. * @param mu_0 The vaccuum permeability constant in internal units. * @param a Current scale factor. * @param H Current Hubble parameter. */ __attribute__((always_inline)) INLINE static void runner_iact_mhd_density( const float r2, const float dx[3], const float hi, const float hj, struct part *restrict pi, struct part *restrict pj, const double mu_0, const float a, const float H) {} /** * @brief MHD-Density interaction between two particles. (non-symmetric) * * @param r2 Comoving square distance between the two particles. * @param dx Comoving vector separating both particles (pi - pj). * @param hi Comoving smoothing-length of particle i. * @param hj Comoving smoothing-length of particle j. * @param pi First particle. * @param pj Second particle. * @param mu_0 The vaccuum permeability constant in internal units. * @param a Current scale factor. * @param H Current Hubble parameter. */ __attribute__((always_inline)) INLINE static void runner_iact_nonsym_mhd_density(const float r2, const float dx[3], const float hi, const float hj, struct part *restrict pi, const struct part *restrict pj, const double mu_0, const float a, const float H) {} /** * @brief Calculate the MHD-gradient interaction between particle i and particle * j * * This method wraps around hydro_gradients_collect, which can be an empty * method, in which case no gradients are used. * * @param r2 Comoving squared distance between particle i and particle j. * @param dx Comoving distance vector between the particles (dx = pi->x - * pj->x). * @param hi Comoving smoothing-length of particle i. * @param hj Comoving smoothing-length of particle j. * @param pi Particle i. * @param pj Particle j. * @param mu_0 The vaccuum permeability constant in internal units. * @param a Current scale factor. * @param H Current Hubble parameter. */ __attribute__((always_inline)) INLINE static void runner_iact_mhd_gradient( const float r2, const float dx[3], const float hi, const float hj, struct part *restrict pi, struct part *restrict pj, const double mu_0, const float a, const float H) {} /** * @brief Calculate the MHDgradient interaction between particle i and particle * j (non-symmetric) * * This method wraps around hydro_gradients_collect, which can be an empty * method, in which case no gradients are used. * * @param r2 Comoving squared distance between particle i and particle j. * @param dx Comoving distance vector between the particles (dx = pi->x - * pj->x). * @param hi Comoving smoothing-length of particle i. * @param hj Comoving smoothing-length of particle j. * @param pi Particle i. * @param pj Particle j. * @param mu_0 The vaccuum permeability constant in internal units. * @param a Current scale factor. * @param H Current Hubble parameter. */ __attribute__((always_inline)) INLINE static void runner_iact_nonsym_mhd_gradient(const float r2, const float dx[3], const float hi, const float hj, struct part *restrict pi, const struct part *restrict pj, const double mu_0, const float a, const float H) {} /** * @brief MHD-Force interaction between two particles. * * @param r2 Comoving square distance between the two particles. * @param dx Comoving vector separating both particles (pi - pj). * @param hi Comoving smoothing-length of particle i. * @param hj Comoving smoothing-length of particle j. * @param pi First particle. * @param pj Second particle. * @param mu_0 The vaccuum permeability constant in internal units. * @param a Current scale factor. * @param H Current Hubble parameter. */ __attribute__((always_inline)) INLINE static void runner_iact_mhd_force( const float r2, const float dx[3], const float hi, const float hj, struct part *restrict pi, struct part *restrict pj, const double mu_0, const float a, const float H) {} /** * @brief MHD-Force interaction between two particles. non-symmetric version. * * @param r2 Comoving square distance between the two particles. * @param dx Comoving vector separating both particles (pi - pj). * @param hi Comoving smoothing-length of particle i. * @param hj Comoving smoothing-length of particle j. * @param pi First particle. * @param pj Second particle. * @param mu_0 The vaccuum permeability constant in internal units. * @param a Current scale factor. * @param H Current Hubble parameter. */ __attribute__((always_inline)) INLINE static void runner_iact_nonsym_mhd_force( const float r2, const float dx[3], const float hi, const float hj, struct part *restrict pi, const struct part *restrict pj, const double mu_0, const float a, const float H) {} #endif /* SWIFT_NONE_MHD_H */