/*******************************************************************************
 * This file is part of SWIFT.
 * Copyright (c) 2018 Folkert Nobels (nobels@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 <http://www.gnu.org/licenses/>.
 *
 *******************************************************************************/
#ifndef SWIFT_NONE_STAR_FORMATION_H
#define SWIFT_NONE_STAR_FORMATION_H

/* Local includes */
#include "cooling_properties.h"
#include "cosmology.h"
#include "entropy_floor.h"
#include "error.h"
#include "hydro_properties.h"
#include "parser.h"
#include "part.h"
#include "physical_constants.h"
#include "units.h"

/* Starformation struct */
struct star_formation {};

/* Does the star formation model move the hydro particles?
   This will update the c->hydro.dx_max_part and
   c->hydro.dx_max_sort after forming a star. */
#define star_formation_need_update_dx_max 0

/**
 * @brief Calculate if the gas has the potential of becoming
 * a star.
 *
 * No star formation should occur, so return 0.
 *
 * @param starform the star formation law properties to use.
 * @param p the gas particles.
 * @param xp the additional properties of the gas particles.
 * @param phys_const the physical constants in internal units.
 * @param cosmo the cosmological parameters and properties.
 * @param hydro_props The properties of the hydro scheme.
 * @param us The internal system of units.
 * @param cooling The cooling data struct.
 *
 */
INLINE static int star_formation_is_star_forming(
    const struct part* p, const struct xpart* xp,
    const struct star_formation* starform, const struct phys_const* phys_const,
    const struct cosmology* cosmo, const struct hydro_props* hydro_props,
    const struct unit_system* us, const struct cooling_function_data* cooling,
    const struct entropy_floor_properties* entropy_floor) {

  return 0;
}

/**
 * @brief Compute the star-formation rate of a given particle and store
 * it into the #xpart.
 *
 * Nothing to do here.
 *
 * @param p #part.
 * @param xp the #xpart.
 * @param starform the star formation law properties to use
 * @param phys_const the physical constants in internal units.
 * @param hydro_props The properties of the hydro scheme.
 * @param cosmo the cosmological parameters and properties.
 * @param dt_star The time-step of this particle.
 */
INLINE static void star_formation_compute_SFR(
    const struct part* p, struct xpart* xp,
    const struct star_formation* starform, const struct phys_const* phys_const,
    const struct hydro_props* hydro_props, const struct cosmology* cosmo,
    const double dt_star) {}

/**
 * @brief Decides whether a particle should be converted into a
 * star or not.
 *
 * No SF should occur, so return 0.
 *
 * @param p The #part.
 * @param xp The #xpart.
 * @param starform The properties of the star formation model.
 * @param e The #engine (for random numbers).
 * @param dt_star The time-step of this particle
 * @return 1 if a conversion should be done, 0 otherwise.
 */
INLINE static int star_formation_should_convert_to_star(
    const struct part* p, const struct xpart* xp,
    const struct star_formation* starform, const struct engine* e,
    const double dt_star) {

  return 0;
}

/**
 * @brief Returns the number of new star particles to create per SF event.
 *
 * @param p The #part.
 * @param xp The #xpart.
 * @param starform The properties of the star formation model.
 *
 * @return The number of extra star particles to generate per gas particles.
 *        (return 0 if the gas particle itself is to be converted)
 */
INLINE static int star_formation_number_spart_to_spawn(
    const struct part* p, const struct xpart* xp,
    const struct star_formation* starform) {
  return 0;
}

/**
 * @brief Returns the number of particles to convert per SF event.
 *
 * @param p The #part.
 * @param xp The #xpart.
 * @param starform The properties of the star formation model.
 *
 * @return The number of particles to generate per gas particles.
 *        (This has to be 0 or 1)
 */
INLINE static int star_formation_number_spart_to_convert(
    const struct part* p, const struct xpart* xp,
    const struct star_formation* starform) {
  return 0;
}

/**
 * @brief Update the SF properties of a particle that is not star forming.
 *
 * Nothing to do here.
 *
 * @param p The #part.
 * @param xp The #xpart.
 * @param e The #engine.
 * @param starform The properties of the star formation model.
 * @param with_cosmology Are we running with cosmology switched on?
 */
INLINE static void star_formation_update_part_not_SFR(
    struct part* p, struct xpart* xp, const struct engine* e,
    const struct star_formation* starform, const int with_cosmology) {}

/**
 * @brief Copies the properties of the gas particle over to the
 * star particle.
 *
 * Nothing to do here.
 *
 * @param e The #engine
 * @param p the gas particles.
 * @param xp the additional properties of the gas particles.
 * @param sp the new created star particle with its properties.
 * @param starform the star formation law properties to use.
 * @param phys_const the physical constants in internal units.
 * @param cosmo the cosmological parameters and properties.
 * @param with_cosmology if we run with cosmology.
 * @param convert_part Did we convert a part (or spawned one)?
 */
INLINE static void star_formation_copy_properties(
    const struct part* p, const struct xpart* xp, struct spart* sp,
    const struct engine* e, const struct star_formation* starform,
    const struct cosmology* cosmo, const int with_cosmology,
    const struct phys_const* phys_const, const struct hydro_props* hydro_props,
    const struct unit_system* us, const struct cooling_function_data* cooling,
    const int convert_part) {}

/**
 * @brief initialization of the star formation law
 *
 * @param parameter_file The parsed parameter file
 * @param phys_const Physical constants in internal units
 * @param us The current internal system of units
 * @param hydro_props The propertis of the hydro model.
 * @param cosmo The current cosmological model.
 * @param entropy_floor The properties of the entropy floor used in this
 * simulation.
 * @param starform the star formation law properties to initialize
 */
INLINE static void starformation_init_backend(
    struct swift_params* parameter_file, const struct phys_const* phys_const,
    const struct unit_system* us, const struct hydro_props* hydro_props,
    const struct cosmology* cosmo,
    const struct entropy_floor_properties* entropy_floor,
    const struct star_formation* starform) {}

/**
 * @brief Prints the used parameters of the star formation law
 *
 * @param starform the star formation law properties.
 */
INLINE static void starformation_print_backend(
    const struct star_formation* starform) {

  message("Star formation law is 'No Star Formation'");
}

/**
 * @brief Return the star formation rate of a particle.
 *
 * No star formation in this model --> we return 0
 *
 * @param p The particle.
 * @param xp The extended data of the particle.
 */
INLINE static float star_formation_get_SFR(const struct part* p,
                                           const struct xpart* xp) {
  return 0.f;
}

/**
 * @brief Finishes the density calculation.
 *
 * Nothing to do here.
 *
 * @param p The particle to act upon
 * @param xp The extra particle to act upon
 * @param cd The global star_formation information.
 * @param cosmo The current cosmological model.
 */
__attribute__((always_inline)) INLINE static void star_formation_end_density(
    struct part* p, struct xpart* xp, const struct star_formation* cd,
    const struct cosmology* cosmo) {}

/**
 * @brief Sets all particle fields to sensible values when the #part has 0 ngbs.
 *
 * Nothing to do here.
 *
 * @param p The particle to act upon
 * @param xp The extended particle data to act upon
 * @param cd #star_formation containing star_formation informations.
 * @param cosmo The current cosmological model.
 */
__attribute__((always_inline)) INLINE static void
star_formation_part_has_no_neighbours(struct part* p, struct xpart* xp,
                                      const struct star_formation* cd,
                                      const struct cosmology* cosmo) {}

/**
 * @brief Sets the star_formation properties of the (x-)particles to a valid
 * state to start the density loop.
 *
 * Nothing to do here.
 *
 * @param data The global star_formation information used for this run.
 * @param p Pointer to the particle data.
 */
__attribute__((always_inline)) INLINE static void star_formation_init_part(
    struct part* p, const struct star_formation* data) {}

/**
 * @brief Sets the star_formation properties of the (x-)particles to a valid
 * start state at the beginning of the simulation after the ICs have been read.
 *
 * Nothing to do here.
 *
 * @param phys_const The physical constant in internal units.
 * @param us The unit system.
 * @param cosmo The current cosmological model.
 * @param data The global star_formation information used for this run.
 * @param p Pointer to the particle data.
 * @param xp Pointer to the extended particle data.
 */
__attribute__((always_inline)) INLINE static void
star_formation_first_init_part(const struct phys_const* phys_const,
                               const struct unit_system* us,
                               const struct cosmology* cosmo,
                               const struct star_formation* data,
                               const struct part* p, struct xpart* xp) {}

/**
 * @brief Split the star formation content of a particle into n pieces
 *
 * @param p The #part.
 * @param xp The #xpart.
 * @param n The number of pieces to split into.
 */
__attribute__((always_inline)) INLINE static void star_formation_split_part(
    struct part* p, struct xpart* xp, const double n) {}

/**
 * @brief Deal with the case where no spart are available for star formation.
 *
 * @param e The #engine.
 * @param p The #part.
 * @param xp The #xpart.
 */
__attribute__((always_inline)) INLINE static void
star_formation_no_spart_available(const struct engine* e, const struct part* p,
                                  const struct xpart* xp) {
  /* Nothing to do, we just skip it and deal with it next step */
}

/**
 * @brief Compute some information for the star formation model based
 * on all the particles that were read in.
 *
 * This is called once on start-up of the code.
 *
 * Nothing to do here.
 *
 * @param star_form The #star_formation structure.
 * @param e The #engine.
 */
__attribute__((always_inline)) INLINE static void
star_formation_first_init_stats(struct star_formation* star_form,
                                const struct engine* e) {}

#endif /* SWIFT_NONE_STAR_FORMATION_H */