/*******************************************************************************
 * This file is part of SWIFT.
 * Copyright (c) 2020 Mladen Ivkovic (mladen.ivkovic@hotmail.com)
 *
 * 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_RT_IACT_DEBUG_H
#define SWIFT_RT_IACT_DEBUG_H

#include "rt_debugging.h"
#include "rt_gradients.h"

/**
 * @file src/rt/debug/rt_iact.h
 * @brief Main header file for the debug radiative transfer scheme particle
 * interactions.
 */

/**
 * @brief Preparation step for injection to gather necessary data.
 * This function gets called during the feedback force loop.
 *
 * @param r2 Comoving square distance between the two particles.
 * @param dx Comoving vector separating both particles (si - pj).
 * @param hi Comoving smoothing-length of particle i.
 * @param hj Comoving smoothing-length of particle j.
 * @param si First (star) particle.
 * @param pj Second (gas) particle (not updated).
 * @param cosmo The cosmological model.
 * @param rt_props Properties of the RT scheme.
 */

__attribute__((always_inline)) INLINE static void
runner_iact_nonsym_rt_injection_prep(const float r2, const float dx[3],
                                     const float hi, const float hj,
                                     struct spart *si, const struct part *pj,
                                     const struct cosmology *cosmo,
                                     const struct rt_props *rt_props) {

  si->rt_data.debug_iact_hydro_inject_prep += 1;
}

/**
 * @brief Injection step interaction between star and hydro 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 si Star particle.
 * @param pj Hydro particle.
 * @param a Current scale factor.
 * @param H Current Hubble parameter.
 * @param rt_props Properties of the RT scheme.
 */
__attribute__((always_inline)) INLINE static void runner_iact_rt_inject(
    const float r2, float dx[3], const float hi, const float hj,
    struct spart *restrict si, struct part *restrict pj, const float a,
    const float H, const struct rt_props *rt_props) {

  /* If the star doesn't have any neighbours, we
   * have nothing to do here. */
  if (si->density.wcount == 0.f) return;

  /* Do some checks and increase neighbour counts
   * before other potential early exits */
  if (si->rt_data.debug_iact_hydro_inject_prep == 0)
    error(
        "Injecting energy from star that wasn't called during injection prep");

  if (!si->rt_data.debug_emission_rate_set)
    error("Injecting energy from star without setting emission rate");

  si->rt_data.debug_iact_hydro_inject += 1;
  si->rt_data.debug_radiation_emitted_tot += 1ULL;

  pj->rt_data.debug_iact_stars_inject += 1;
  pj->rt_data.debug_radiation_absorbed_tot += 1ULL;
}

/**
 * @brief Flux calculation between particle i and particle j
 *
 * This method calls runner_iact_rt_fluxes_common with mode 1.
 *
 * @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.
 * @param mode 0 if non-symmetric interaction, 1 if symmetric
 */
__attribute__((always_inline)) INLINE static void runner_iact_rt_flux_common(
    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, int mode) {

  const char *func_name = (mode == 1) ? "sym flux iact" : "nonsym flux iact";
  rt_debug_sequence_check(pi, 3, func_name);
  pi->rt_data.debug_calls_iact_transport_interaction += 1;

  if (mode == 1) {
    rt_debug_sequence_check(pj, 3, func_name);
    pj->rt_data.debug_calls_iact_transport_interaction += 1;
  }
}

/**
 * @brief Flux calculation between particle i and particle j
 *
 * This method calls runner_iact_rt_fluxes_common with mode 1.
 *
 * @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_rt_transport(
    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) {

  runner_iact_rt_flux_common(r2, dx, hi, hj, pi, pj, a, H, 1);
}

/**
 * @brief Flux calculation between particle i and particle j: non-symmetric
 * version
 *
 * This method calls runner_iact_rt_fluxes_common with mode 0.
 *
 * @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_rt_transport(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) {

  runner_iact_rt_flux_common(r2, dx, hi, hj, pi, pj, a, H, 0);
}

/**
 * @brief Calculate the gradient interaction between particle i and particle j
 *
 * This method wraps around rt_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 a Current scale factor.
 * @param H Current Hubble parameter.
 */
__attribute__((always_inline)) INLINE static void runner_iact_rt_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) {

  rt_gradients_collect(r2, dx, hi, hj, pi, pj);
}

/**
 * @brief Calculate the gradient interaction between particle i and particle j:
 * non-symmetric version
 *
 * This method wraps around rt_gradients_nonsym_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 a Current scale factor.
 * @param H Current Hubble parameter.
 */
__attribute__((always_inline)) INLINE static void
runner_iact_nonsym_rt_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) {

  rt_gradients_nonsym_collect(r2, dx, hi, hj, pi, pj);
}

#endif /* SWIFT_RT_IACT_DEBUG_H */