/*******************************************************************************
* 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_GRAVITY_PROPERTIES
#define SWIFT_GRAVITY_PROPERTIES
/* Config parameters. */
#include
#if defined(HAVE_HDF5)
#include
#endif
/* Forward declarations */
struct cosmology;
struct phys_const;
struct swift_params;
/**
* @brief Contains all the constants and parameters of the self-gravity scheme
*/
struct gravity_props {
/* -------------- Softening for the regular particles ---------------- */
/*! Co-moving softening length for high-res. DM particles at the current
* redshift. */
float epsilon_DM_cur;
/*! Co-moving softening length for high-res. baryon particles at the current
* redshift. */
float epsilon_baryon_cur;
/* -------------- Softening for the background DM -------------------- */
/*! Conversion factor from cbrt of particle mass to softening assuming
* a constant fraction of the mean inter-particle separation at that mass. */
float epsilon_background_fac;
/* -------------- Softening for the neutrino DM ---------------------- */
/*! Co-moving softening length for neutrino DM particles at the current
* redshift. */
float epsilon_nu_cur;
/* -------------- Properties of the FFM gravity ---------------------- */
/*! What MAC are we currently using? */
int use_advanced_MAC;
/*! Are we using the adaptive opening angle? (as read from param file) */
int use_adaptive_tolerance;
/*! Are we using the Gadget adaptive opening angle? (as read from param file)
*/
int use_gadget_tolerance;
/*! Accuracy parameter of the advanced MAC */
float adaptive_tolerance;
/*! Tree opening angle (Multipole acceptance criterion) */
double theta_crit;
/*! Are we allowing tree gravity below softening? */
int use_tree_below_softening;
/*! Are we applying long-range truncation to the forces in the MAC? */
int consider_truncation_in_MAC;
/* ------------- Properties of the softened gravity ------------------ */
/*! Co-moving softening length for for high-res. DM particles */
float epsilon_DM_comoving;
/*! Maximal softening length in physical coordinates for the high-res.
* DM particles */
float epsilon_DM_max_physical;
/*! Co-moving softening length for for high-res. baryon particles */
float epsilon_baryon_comoving;
/*! Maximal softening length in physical coordinates for the high-res.
* baryon particles */
float epsilon_baryon_max_physical;
/*! Co-moving softening length for for neutrino DM particles */
float epsilon_nu_comoving;
/*! Maximal softening length in physical coordinates for the neutrino
* DM particles */
float epsilon_nu_max_physical;
/*! Fraction of the mean inter particle separation corresponding to the
* co-moving softening length of the low-res. particles (DM + baryons) */
float mean_inter_particle_fraction_high_res;
/*! Maximal comoving softening in the case of adaptive softening for gas */
float max_adaptive_softening;
/*! Minimal comoving softening in the case of adaptive softening for gas */
float min_adaptive_softening;
/* ------------- Properties of the time integration ----------------- */
/*! Frequency of tree-rebuild in units of #gpart updates. */
float rebuild_frequency;
/*! Fraction of active #gpart needed to trigger a tree-rebuild */
float rebuild_active_fraction;
/*! Time integration dimensionless multiplier */
float eta;
/* ------------- Properties of the mesh-based gravity ---------------- */
/*! Periodic long-range mesh side-length */
int mesh_size;
/*! Whether mesh is distributed between MPI ranks when we use MPI */
int distributed_mesh;
/*! Whether or not to use local patches rather than
* direct atomic writes to the mesh when running without MPI */
int mesh_uses_local_patches;
/*! Mesh smoothing scale in units of top-level cell size */
float a_smooth;
/*! Distance below which the truncated mesh force is Newtonian in units of
* a_smooth */
float r_cut_min_ratio;
/*! Distance above which the truncated mesh force is negligible in units of
* a_smooth */
float r_cut_max_ratio;
/*! Long-range gravity mesh scale. */
float r_s;
/*! Inverse of the long-range gravity mesh scale. */
float r_s_inv;
/* ------------- Physical constants ---------------------------------- */
/*! Gravitational constant (in internal units, copied from the physical
* constants) */
float G_Newton;
};
void gravity_props_print(const struct gravity_props *p);
void gravity_props_init(struct gravity_props *p, struct swift_params *params,
const struct phys_const *phys_const,
const struct cosmology *cosmo, const int with_cosmology,
const int with_external_potential,
const int has_baryons, const int has_DM,
const int has_neutrinos, const int is_zoom_simulation,
const int periodic, const double dim[3],
const int cdim[3]);
void gravity_props_update(struct gravity_props *p,
const struct cosmology *cosmo);
void gravity_props_update_MAC_choice(struct gravity_props *p);
#if defined(HAVE_HDF5)
void gravity_props_print_snapshot(hid_t h_grpsph,
const struct gravity_props *p);
#endif
/* Dump/restore. */
void gravity_props_struct_dump(const struct gravity_props *p, FILE *stream);
void gravity_props_struct_restore(struct gravity_props *p, FILE *stream);
#endif /* SWIFT_GRAVITY_PROPERTIES */