import abc
import numpy as np
import numexpr as ne
from tardis import constants as const
from tardis.montecarlo.montecarlo_numba.packet_collections import (
PacketCollection,
)
from astropy import units as u
[docs]class BasePacketSource(abc.ABC):
"""
Abstract base packet source
Parameters
----------
base_seed : int
Base Seed for random number generator
legacy_secondary_seed : int
Secondary seed for global numpy rng (Deprecated: Legacy reasons only)
"""
# MAX_SEED_VAL must be multiple orders of magnitude larger than no_of_packets;
# otherwise, each packet would not have its own seed. Here, we set the max
# seed val to the maximum allowed by numpy.
MAX_SEED_VAL = 2**32 - 1
def __init__(
self, base_seed=None, legacy_mode_enabled=False, legacy_second_seed=None
):
self.base_seed = base_seed
self.legacy_mode_enabled = legacy_mode_enabled
if self.legacy_mode_enabled and legacy_second_seed is not None:
np.random.seed(legacy_second_seed)
else:
np.random.seed(self.base_seed)
def _reseed(self, seed):
self.rng = np.random.default_rng(seed=seed)
[docs] @abc.abstractmethod
def create_packet_radii(self, no_of_packets, *args, **kwargs):
pass
[docs] @abc.abstractmethod
def create_packet_nus(self, no_of_packets, *args, **kwargs):
pass
[docs] @abc.abstractmethod
def create_packet_mus(self, no_of_packets, *args, **kwargs):
pass
[docs] @abc.abstractmethod
def create_packet_energies(self, no_of_packets, *args, **kwargs):
pass
[docs] def create_packets(self, no_of_packets, seed_offset=0, *args, **kwargs):
"""Generate packet properties as arrays
Parameters
----------
no_of_packets : int
Number of packets
Returns
-------
array
Packet radii
array
Packet frequencies
array
Packet directions
array
Packet energies
"""
# the iteration (passed as seed_offset) is added each time to preserve randomness
# across different simulations with the same temperature,
# for example. We seed the random module instead of the numpy module
# because we call random.sample, which references a different internal
# state than in the numpy.random module.
self._reseed(self.base_seed + seed_offset)
packet_seeds = self.rng.choice(
self.MAX_SEED_VAL, no_of_packets, replace=True
)
radii = self.create_packet_radii(no_of_packets, *args, **kwargs).value
nus = self.create_packet_nus(no_of_packets, *args, **kwargs).value
mus = self.create_packet_mus(no_of_packets, *args, **kwargs)
energies = self.create_packet_energies(
no_of_packets, *args, **kwargs
).value
# Check if all arrays have the same length
assert (
len(radii) == len(nus) == len(mus) == len(energies) == no_of_packets
)
radiation_field_luminosity = self.calculate_radfield_luminosity().value
return PacketCollection(
radii,
nus,
mus,
energies,
packet_seeds,
radiation_field_luminosity,
)
[docs] def calculate_radfield_luminosity(self):
"""
Calculate inner luminosity.
Parameters
----------
model : model.SimulationState
Returns
-------
astropy.units.Quantity
"""
return (
4
* np.pi
* const.sigma_sb
* self.radius**2
* self.temperature**4
).to("erg/s")
[docs]class BlackBodySimpleSource(BasePacketSource):
"""
Simple packet source that generates Blackbody packets for the Montecarlo
part.
Parameters
----------
radius : astropy.units.Quantity
Initial packet radius
temperature : astropy.units.Quantity
Absolute Temperature.
base_seed : int
Base Seed for random number generator
legacy_secondary_seed : int
Secondary seed for global numpy rng (Deprecated: Legacy reasons only)
"""
[docs] @classmethod
def from_simulation_state(cls, simulation_state, *args, **kwargs):
return cls(
simulation_state.r_inner[0],
simulation_state.t_inner,
*args,
**kwargs,
)
def __init__(self, radius=None, temperature=None, **kwargs):
self.radius = radius
self.temperature = temperature
super().__init__(**kwargs)
[docs] def create_packets(self, no_of_packets, *args, **kwargs):
if self.radius is None or self.temperature is None:
raise ValueError("Black body Radius or Temperature isn't set")
return super().create_packets(no_of_packets, *args, **kwargs)
[docs] def create_packet_radii(self, no_of_packets):
"""
Create packet radii
Parameters
----------
no_of_packets : int
number of packets to be created
Returns
-------
Radii for packets
numpy.ndarray
"""
return np.ones(no_of_packets) * self.radius.cgs
[docs] def create_packet_nus(self, no_of_packets, l_samples=1000):
"""
Create packet :math:`\\nu` distributed using the algorithm described in
Bjorkman & Wood 2001 (page 4) which references
Carter & Cashwell 1975:
First, generate a uniform random number, :math:`\\xi_0 \\in [0, 1]` and
determine the minimum value of
:math:`l, l_{\\rm min}`, that satisfies the condition
.. math::
\\sum_{i=1}^{l} i^{-4} \\ge {{\\pi^4}\\over{90}} m_0 \\;.
Next obtain four additional uniform random numbers (in the range 0
to 1) :math:`\\xi_1, \\xi_2, \\xi_3, {\\rm and } \\xi_4`.
Finally, the packet frequency is given by
.. math::
x = -\\ln{(\\xi_1\\xi_2\\xi_3\\xi_4)}/l_{\\rm min}\\;.
where :math:`x=h\\nu/kT`
Parameters
----------
no_of_packets : int
l_samples : int
number of l_samples needed in the algorithm
Returns
-------
array of frequencies
numpy.ndarray
"""
l_array = np.cumsum(np.arange(1, l_samples, dtype=np.float64) ** -4)
l_coef = np.pi**4 / 90.0
# For testing purposes
if self.legacy_mode_enabled:
xis = np.random.random((5, no_of_packets))
else:
xis = self.rng.random((5, no_of_packets))
l = l_array.searchsorted(xis[0] * l_coef) + 1.0
xis_prod = np.prod(xis[1:], 0)
x = ne.evaluate("-log(xis_prod)/l")
return (x * (const.k_B * self.temperature) / const.h).cgs
[docs] def create_packet_mus(self, no_of_packets):
"""
Create zero-limb-darkening packet :math:`\mu` distributed
according to :math:`\\mu=\\sqrt{z}, z \isin [0, 1]`
Parameters
----------
no_of_packets : int
number of packets to be created
Returns
-------
Directions for packets
numpy.ndarray
"""
# For testing purposes
if self.legacy_mode_enabled:
return np.sqrt(np.random.random(no_of_packets))
else:
return np.sqrt(self.rng.random(no_of_packets))
[docs] def create_packet_energies(self, no_of_packets):
"""
Uniformly distribute energy in arbitrary units where the ensemble of
packets has energy of 1.
Parameters
----------
no_of_packets : int
number of packets
Returns
-------
energies for packets
numpy.ndarray
"""
return np.ones(no_of_packets) / no_of_packets * u.erg
[docs] def set_temperature_from_luminosity(self, luminosity: u.Quantity):
"""
Set blackbody packet source temperature from luminosity
Parameters
----------
luminosity : u.Quantity
"""
self.temperature = (
(luminosity / (4 * np.pi * self.radius**2 * const.sigma_sb))
** 0.25
).to("K")
[docs]class BlackBodySimpleSourceRelativistic(BlackBodySimpleSource):
"""
Simple packet source that generates Blackbody packets for the Montecarlo
part.
Parameters
----------
time_explosion : astropy.units.Quantity
Time elapsed since explosion
radius : astropy.units.Quantity
Initial packet radius
temperature : astropy.units.Quantity
Absolute Temperature.
base_seed : int
Base Seed for random number generator
legacy_secondary_seed : int
Secondary seed for global numpy rng (Deprecated: Legacy reasons only)
"""
[docs] @classmethod
def from_simulation_state(cls, simulation_state, *args, **kwargs):
return cls(
simulation_state.time_explosion,
simulation_state.r_inner[0],
simulation_state.t_inner,
*args,
**kwargs,
)
def __init__(self, time_explosion=None, **kwargs):
self.time_explosion = time_explosion
super().__init__(**kwargs)
[docs] def create_packets(self, no_of_packets):
"""Generate relativistic black-body packet properties as arrays
Parameters
----------
no_of_packets : int
Number of packets
Returns
-------
array
Packet radii
array
Packet frequencies
array
Packet directions
array
Packet energies
"""
if self.radius is None or self.time_explosion is None:
raise ValueError("Black body Radius or Time of Explosion isn't set")
self.beta = (self.radius / self.time_explosion) / const.c
return super().create_packets(no_of_packets)
[docs] def create_packet_mus(self, no_of_packets):
"""
Create zero-limb-darkening packet :math:`\mu^\prime` distributed
according to :math:`\\mu^\\prime=2 \\frac{\\mu^\\prime + \\beta}{2 \\beta + 1}`.
The complicated distribution is due to the fact that the inner boundary
on which the packets are initialized is not comoving with the material.
Parameters
----------
no_of_packets : int
number of packets to be created
Returns
-------
Directions for packets
numpy.ndarray
"""
z = self.rng.random(no_of_packets)
beta = self.beta
return -beta + np.sqrt(beta**2 + 2 * beta * z + z)
[docs] def create_packet_energies(self, no_of_packets):
"""
Uniformly distribute energy in arbitrary units where the ensemble of
packets has energy of 1 multiplied by relativistic correction factors.
Parameters
----------
no_of_packets : int
number of packets
Returns
-------
energies for packets
numpy.ndarray
"""
beta = self.beta
gamma = 1.0 / np.sqrt(1 - beta**2)
static_inner_boundary2cmf_factor = (2 * beta + 1) / (1 - beta**2)
energies = np.ones(no_of_packets) / no_of_packets
# In principle, the factor gamma should be applied to the time of
# simulation to account for time dilation between the lab and comoving
# frame. However, all relevant quantities (luminosities, estimators, ...)
# are calculated as ratios of packet energies and the time of simulation.
# Thus, we can absorb the factor gamma in the packet energies, which is
# more convenient.
return energies * static_inner_boundary2cmf_factor / gamma * u.erg