Source code for tardis.energy_input.gamma_ray_estimators

import numpy as np
from numba import njit

from tardis.energy_input.util import (
    ELECTRON_MASS_ENERGY_KEV,
    H_CGS_KEV,
    angle_aberration_gamma,
    doppler_factor_3d,
)
from tardis.opacities.opacities import (
    SIGMA_T,
    compton_opacity_calculation,
    kappa_calculation,
    photoabsorption_opacity_calculation,
)
from tardis.transport.montecarlo import njit_dict_no_parallel


[docs] def compton_emissivity_estimator(packet, distance): """Compton scattering emissivity estimator for integral calculations Parameters ---------- packet : GXPacket Packet that needs its emissivity calculated distance : float64 Distance packet has travelled Returns ------- float64, int Unnormalized emissivity estimator, line index """ cmf_direction = angle_aberration_gamma( packet.get_direction_vector(), packet.location_r ) cmf_angle = np.dot(cmf_direction, [1, 0, 0]) frequency_factor = ( 1 + H_CGS_KEV * packet.nu_cmf / ELECTRON_MASS_ENERGY_KEV + (1.0 - cmf_angle) ) line_index = GET_NEAREST_LINE_REDWARD_FUNCTION( packet.nu_cmf / frequency_factor ) partial_cross_section = ( 3.0 / 16.0 / np.pi * SIGMA_T / frequency_factor / frequency_factor * (frequency_factor + (1.0 / frequency_factor) + cmf_angle**2.0 - 1.0) ) doppler_factor = doppler_factor_3d( packet.get_direction_vector(), packet.location_r ) emissivity = ( packet.energy_rf * partial_cross_section * distance * doppler_factor**2.0 / frequency_factor ) return emissivity, line_index
[docs] def pair_creation_estimator(packet, pair_creation_opacity, distance): """Calculates the emissivity for pair creation gamma-rays Parameters ---------- packet : GXPacket Packet that needs its emissivity calculated pair_creation_opacity : float64 Opacity of the pair creation process distance : float64 Distance packet has travelled Returns ------- float64 Emissivity estimator """ normalized_energy = ( 2 * ELECTRON_MASS_ENERGY_KEV / (H_CGS_KEV * packet.nu_cmf) ) emissivity = ( pair_creation_opacity * normalized_energy * packet.energy_rf * distance ) return emissivity
[docs] @njit(**njit_dict_no_parallel) def get_average_compton_fraction(energy): def f(x, mu): return 1.0 / (1.0 + x * (1.0 - mu)) def cross_section(x, mu): return ( (3.0 * SIGMA_T) / (16.0 * np.pi) * f(x, mu) ** 2.0 * (f(x, mu) + 1.0 / f(x, mu) - (1.0 - mu**2)) ) x = kappa_calculation(energy) mus = np.linspace(-1, 1, 100) dmu = mus[1] - mus[0] sum = 0 norm = 0 for mu in mus: sum += cross_section(x, mu) * f(x, mu) * dmu norm += cross_section(x, mu) * dmu integral = 1.0 - sum / norm return 1 - integral
[docs] @njit(**njit_dict_no_parallel) def deposition_estimator_kasen(energy, ejecta_density, iron_group_fraction): return get_average_compton_fraction(energy) * compton_opacity_calculation( energy, ejecta_density ) + photoabsorption_opacity_calculation( energy, ejecta_density, iron_group_fraction )