/******************************************************************************* * This file is part of SWIFT. * Copyright (c) 2016 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_PRESSURE_ENTROPY_HYDRO_IACT_H #define SWIFT_PRESSURE_ENTROPY_HYDRO_IACT_H #include "adaptive_softening_iact.h" #include "hydro_parameters.h" #include "signal_velocity.h" /** * @file PressureEntropy/hydro_iact.h * @brief Pressure-Entropy implementation of SPH (Particle interactions) * * The thermal variable is the entropy (S) and the entropy is smoothed over * contact discontinuities to prevent spurious surface tension. * * Follows eqautions (19), (21) and (22) of Hopkins, P., MNRAS, 2013, * Volume 428, Issue 4, pp. 2840-2856 with a simple Balsara viscosity term. */ /** * @brief 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 a Current scale factor. * @param H Current Hubble parameter. */ __attribute__((always_inline)) INLINE static void runner_iact_density( const float r2, const float dx[3], const float hi, const float hj, struct part *restrict pi, struct part *restrict pj, const float a, const float H) { float wi, wi_dx; float wj, wj_dx; float dv[3], curlvr[3]; /* Get the masses. */ const float mi = pi->mass; const float mj = pj->mass; /* Get r and 1/r. */ const float r = sqrtf(r2); const float r_inv = r ? 1.0f / r : 0.0f; /* Compute the kernel function for pi */ const float hi_inv = 1.f / hi; const float ui = r * hi_inv; kernel_deval(ui, &wi, &wi_dx); /* Compute contribution to the density */ pi->rho += mj * wi; pi->density.rho_dh -= mj * (hydro_dimension * wi + ui * wi_dx); /* Compute contribution to the number of neighbours */ pi->density.wcount += wi; pi->density.wcount_dh -= (hydro_dimension * wi + ui * wi_dx); /* Compute contribution to the weighted density */ pi->rho_bar += mj * pj->entropy_one_over_gamma * wi; pi->density.pressure_dh -= mj * pj->entropy_one_over_gamma * (hydro_dimension * wi + ui * wi_dx); /* Compute contribution to the adpative softening correction */ adaptive_softening_add_correction_term(pi, ui, hi_inv, mj); /* Compute the kernel function for pj */ const float hj_inv = 1.f / hj; const float uj = r * hj_inv; kernel_deval(uj, &wj, &wj_dx); /* Compute contribution to the density */ pj->rho += mi * wj; pj->density.rho_dh -= mi * (hydro_dimension * wj + uj * wj_dx); /* Compute contribution to the number of neighbours */ pj->density.wcount += wj; pj->density.wcount_dh -= (hydro_dimension * wj + uj * wj_dx); /* Compute contribution to the weighted density */ pj->rho_bar += mi * pi->entropy_one_over_gamma * wj; pj->density.pressure_dh -= mi * pi->entropy_one_over_gamma * (hydro_dimension * wj + uj * wj_dx); /* Compute contribution to the adpative softening correction */ adaptive_softening_add_correction_term(pj, uj, hj_inv, mi); const float faci = mj * wi_dx * r_inv; const float facj = mi * wj_dx * r_inv; /* Compute dv dot r */ dv[0] = pi->v[0] - pj->v[0]; dv[1] = pi->v[1] - pj->v[1]; dv[2] = pi->v[2] - pj->v[2]; const float dvdr = dv[0] * dx[0] + dv[1] * dx[1] + dv[2] * dx[2]; pi->density.div_v -= faci * dvdr; pj->density.div_v -= facj * dvdr; /* Compute dv cross r */ curlvr[0] = dv[1] * dx[2] - dv[2] * dx[1]; curlvr[1] = dv[2] * dx[0] - dv[0] * dx[2]; curlvr[2] = dv[0] * dx[1] - dv[1] * dx[0]; pi->density.rot_v[0] += faci * curlvr[0]; pi->density.rot_v[1] += faci * curlvr[1]; pi->density.rot_v[2] += faci * curlvr[2]; pj->density.rot_v[0] += facj * curlvr[0]; pj->density.rot_v[1] += facj * curlvr[1]; pj->density.rot_v[2] += facj * curlvr[2]; } /** * @brief 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 (not updated). * @param a Current scale factor. * @param H Current Hubble parameter. */ __attribute__((always_inline)) INLINE static void runner_iact_nonsym_density( const float r2, const float dx[3], const float hi, const float hj, struct part *restrict pi, const struct part *restrict pj, const float a, const float H) { float wi, wi_dx; float dv[3], curlvr[3]; /* Get the masses. */ const float mj = pj->mass; /* Get r and 1/r. */ const float r = sqrtf(r2); const float r_inv = r ? 1.0f / r : 0.0f; /* Compute the kernel function */ const float h_inv = 1.0f / hi; const float ui = r * h_inv; kernel_deval(ui, &wi, &wi_dx); /* Compute contribution to the density */ pi->rho += mj * wi; pi->density.rho_dh -= mj * (hydro_dimension * wi + ui * wi_dx); /* Compute contribution to the number of neighbours */ pi->density.wcount += wi; pi->density.wcount_dh -= (hydro_dimension * wi + ui * wi_dx); /* Compute contribution to the weighted density */ pi->rho_bar += mj * pj->entropy_one_over_gamma * wi; pi->density.pressure_dh -= mj * pj->entropy_one_over_gamma * (hydro_dimension * wi + ui * wi_dx); /* Compute contribution to the adpative softening correction */ adaptive_softening_add_correction_term(pi, ui, h_inv, mj); const float fac = mj * wi_dx * r_inv; /* Compute dv dot r */ dv[0] = pi->v[0] - pj->v[0]; dv[1] = pi->v[1] - pj->v[1]; dv[2] = pi->v[2] - pj->v[2]; const float dvdr = dv[0] * dx[0] + dv[1] * dx[1] + dv[2] * dx[2]; pi->density.div_v -= fac * dvdr; /* Compute dv cross r */ curlvr[0] = dv[1] * dx[2] - dv[2] * dx[1]; curlvr[1] = dv[2] * dx[0] - dv[0] * dx[2]; curlvr[2] = dv[0] * dx[1] - dv[1] * dx[0]; pi->density.rot_v[0] += fac * curlvr[0]; pi->density.rot_v[1] += fac * curlvr[1]; pi->density.rot_v[2] += fac * curlvr[2]; } /** * @brief Calculate the gradient interaction between particle i and particle j * * Nothing to do here in this scheme. * * @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 a Current scale factor. * @param H Current Hubble parameter. */ __attribute__((always_inline)) INLINE static void runner_iact_gradient( const float r2, const float dx[3], const float hi, const float hj, struct part *restrict pi, struct part *restrict pj, const float a, const float H) {} /** * @brief Calculate the gradient interaction between particle i and particle j: * non-symmetric version * * Nothing to do here in this scheme. * * @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 a Current scale factor. * @param H Current Hubble parameter. */ __attribute__((always_inline)) INLINE static void runner_iact_nonsym_gradient( const float r2, const float dx[3], const float hi, const float hj, struct part *restrict pi, struct part *restrict pj, const float a, const float H) {} /** * @brief 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 a Current scale factor. * @param H Current Hubble parameter. */ __attribute__((always_inline)) INLINE static void runner_iact_force( const float r2, const float dx[3], const float hi, const float hj, struct part *restrict pi, struct part *restrict pj, const float a, const float H) { float wi, wj, wi_dx, wj_dx; /* Cosmological factors entering the EoMs */ const float fac_mu = pow_three_gamma_minus_five_over_two(a); const float a2_Hubble = a * a * H; /* Get r and 1/r. */ const float r = sqrtf(r2); const float r_inv = r ? 1.0f / r : 0.0f; /* Get some values in local variables. */ const float mi = pi->mass; const float mj = pj->mass; const float rhoi = pi->rho; const float rhoj = pj->rho; /* Get the kernel for hi. */ const float hi_inv = 1.0f / hi; const float hid_inv = pow_dimension_plus_one(hi_inv); /* 1/h^(d+1) */ const float ui = r * hi_inv; kernel_deval(ui, &wi, &wi_dx); const float wi_dr = hid_inv * wi_dx; /* Get the kernel for hj. */ const float hj_inv = 1.0f / hj; const float hjd_inv = pow_dimension_plus_one(hj_inv); /* 1/h^(d+1) */ const float xj = r * hj_inv; kernel_deval(xj, &wj, &wj_dx); const float wj_dr = hjd_inv * wj_dx; /* Compute gradient terms */ const float f_i = pi->force.f; const float f_j = pj->force.f; /* Compute Pressure terms */ const float P_over_rho2_i = pi->force.P_over_rho2; const float P_over_rho2_j = pj->force.P_over_rho2; /* Compute entropy terms */ const float S_gamma_i = pi->entropy_one_over_gamma; const float S_gamma_j = pj->entropy_one_over_gamma; /* Compute dv dot r. */ const float dvdr = (pi->v[0] - pj->v[0]) * dx[0] + (pi->v[1] - pj->v[1]) * dx[1] + (pi->v[2] - pj->v[2]) * dx[2] + a2_Hubble * r2; /* Balsara term */ const float balsara_i = pi->force.balsara; const float balsara_j = pj->force.balsara; /* Are the particles moving towards each others ? */ const float omega_ij = fminf(dvdr, 0.f); const float mu_ij = fac_mu * r_inv * omega_ij; /* This is 0 or negative */ /* Signal velocity */ const float v_sig = signal_velocity(dx, pi, pj, mu_ij, const_viscosity_beta); /* Now construct the full viscosity term */ const float rho_ij = 0.5f * (rhoi + rhoj); const float visc = -0.25f * v_sig * mu_ij * (balsara_i + balsara_j) / rho_ij; /* Now, convolve with the kernel */ const float visc_term = 0.5f * visc * (wi_dr + wj_dr); const float sph_term = (S_gamma_j / S_gamma_i - f_i / S_gamma_i) * P_over_rho2_i * wi_dr + (S_gamma_i / S_gamma_j - f_j / S_gamma_j) * P_over_rho2_j * wj_dr; /* Adaptive softening acceleration term */ const float adapt_soft_acc_term = adaptive_softening_get_acc_term(pi, pj, wi_dr, wj_dr, f_i, f_j, r_inv); /* Eventually got the acceleration */ const float acc = (visc_term + sph_term) * r_inv + adapt_soft_acc_term; /* Use the force Luke ! */ pi->a_hydro[0] -= mj * acc * dx[0]; pi->a_hydro[1] -= mj * acc * dx[1]; pi->a_hydro[2] -= mj * acc * dx[2]; pj->a_hydro[0] += mi * acc * dx[0]; pj->a_hydro[1] += mi * acc * dx[1]; pj->a_hydro[2] += mi * acc * dx[2]; /* Get the time derivative for h. */ pi->force.h_dt -= mj * dvdr * r_inv / rhoj * wi_dr; pj->force.h_dt -= mi * dvdr * r_inv / rhoi * wj_dr; /* Update the signal velocity. */ pi->force.v_sig = fmaxf(pi->force.v_sig, v_sig); pj->force.v_sig = fmaxf(pj->force.v_sig, v_sig); /* Change in entropy */ pi->entropy_dt += mj * visc_term * r_inv * dvdr; pj->entropy_dt += mi * visc_term * r_inv * dvdr; } /** * @brief Force 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 (not updated). * @param a Current scale factor. * @param H Current Hubble parameter. */ __attribute__((always_inline)) INLINE static void runner_iact_nonsym_force( const float r2, const float dx[3], const float hi, const float hj, struct part *restrict pi, const struct part *restrict pj, const float a, const float H) { float wi, wj, wi_dx, wj_dx; /* Cosmological factors entering the EoMs */ const float fac_mu = pow_three_gamma_minus_five_over_two(a); const float a2_Hubble = a * a * H; /* Get r and 1/r. */ const float r = sqrtf(r2); const float r_inv = r ? 1.0f / r : 0.0f; /* Get some values in local variables. */ // const float mi = pi->mass; const float mj = pj->mass; const float rhoi = pi->rho; const float rhoj = pj->rho; /* Get the kernel for hi. */ const float hi_inv = 1.0f / hi; const float hid_inv = pow_dimension_plus_one(hi_inv); /* 1/h^(d+1) */ const float ui = r * hi_inv; kernel_deval(ui, &wi, &wi_dx); const float wi_dr = hid_inv * wi_dx; /* Get the kernel for hj. */ const float hj_inv = 1.0f / hj; const float hjd_inv = pow_dimension_plus_one(hj_inv); /* 1/h^(d+1) */ const float xj = r * hj_inv; kernel_deval(xj, &wj, &wj_dx); const float wj_dr = hjd_inv * wj_dx; /* Compute gradient terms */ const float f_i = pi->force.f; const float f_j = pj->force.f; /* Compute Pressure terms */ const float P_over_rho2_i = pi->force.P_over_rho2; const float P_over_rho2_j = pj->force.P_over_rho2; /* Compute entropy terms */ const float S_gamma_i = pi->entropy_one_over_gamma; const float S_gamma_j = pj->entropy_one_over_gamma; /* Compute dv dot r. */ const float dvdr = (pi->v[0] - pj->v[0]) * dx[0] + (pi->v[1] - pj->v[1]) * dx[1] + (pi->v[2] - pj->v[2]) * dx[2] + a2_Hubble * r2; /* Balsara term */ const float balsara_i = pi->force.balsara; const float balsara_j = pj->force.balsara; /* Are the particles moving towards each others ? */ const float omega_ij = fminf(dvdr, 0.f); const float mu_ij = fac_mu * r_inv * omega_ij; /* This is 0 or negative */ /* Signal velocity */ const float v_sig = signal_velocity(dx, pi, pj, mu_ij, const_viscosity_beta); /* Now construct the full viscosity term */ const float rho_ij = 0.5f * (rhoi + rhoj); const float visc = -0.25f * v_sig * mu_ij * (balsara_i + balsara_j) / rho_ij; /* Now, convolve with the kernel */ const float visc_term = 0.5f * visc * (wi_dr + wj_dr); const float sph_term = (S_gamma_j / S_gamma_i - f_i / S_gamma_i) * P_over_rho2_i * wi_dr + (S_gamma_i / S_gamma_j - f_j / S_gamma_j) * P_over_rho2_j * wj_dr; /* Adaptive softening acceleration term */ const float adapt_soft_acc_term = adaptive_softening_get_acc_term(pi, pj, wi_dr, wj_dr, f_i, f_j, r_inv); /* Eventually got the acceleration */ const float acc = (visc_term + sph_term) * r_inv + adapt_soft_acc_term; /* Use the force Luke ! */ pi->a_hydro[0] -= mj * acc * dx[0]; pi->a_hydro[1] -= mj * acc * dx[1]; pi->a_hydro[2] -= mj * acc * dx[2]; /* Get the time derivative for h. */ pi->force.h_dt -= mj * dvdr * r_inv / rhoj * wi_dr; /* Update the signal velocity. */ pi->force.v_sig = fmaxf(pi->force.v_sig, v_sig); /* Change in entropy */ pi->entropy_dt += mj * visc_term * r_inv * dvdr; } #endif /* SWIFT_PRESSURE_ENTROPY_HYDRO_IACT_H */