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Mori axion 2023 #285

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338 changes: 338 additions & 0 deletions doc/nb/Mori_2023.ipynb

Large diffs are not rendered by default.

72 changes: 72 additions & 0 deletions python/snewpy/models/ccsn.py
Original file line number Diff line number Diff line change
Expand Up @@ -742,6 +742,7 @@ def __new__(cls, filename=None, *, progenitor_mass=None):
# Populate Docstring with abbreviated param values
__new__.__doc__ = __new__.__doc__.format(**_param_abbrv)


class Fornax_2022(_RegistryModel):
"""Model based on 2D simulations of 100 progenitors from Tianshu Wang, David Vartanyan, Adam Burrows, and Matthew S.B. Coleman, MNRAS 517:543, 2022.
Data available at https://www.astro.princeton.edu/~burrows/nu-emissions.2d.large/
Expand Down Expand Up @@ -804,6 +805,77 @@ def __new__(cls, *, progenitor=None, progenitor_mass=None):
# Populate Docstring with abbreviated param values
__new__.__doc__ = __new__.__doc__.format(**_param_abbrv)


class Mori_2023(_RegistryModel):
"""Model based on 2D simulations with axionlike particles, K. Mori, T. Takiwaki, K. Kotake and S. Horiuchi, Phys. Rev. D 108:063027, 2023. All models are based on the non-rotating 20 M_sun solar metallicity progenitor model from S.E. Woolsey and A. Heger, Phys. Rep. 442:269, 2007. Data from private communication.
"""
param = {'axion_mass' : [0, 100, 200]<<u.MeV,
'axion_coupling' : [0, 2, 4, 6, 8, 10, 12, 14, 16, 20]<<(1e-10/u.GeV) }

_param_validator = lambda p: \
(p['axion_mass'] == 0 and p['axion_coupling'] == 0) or \
(p['axion_mass'].to_value('MeV') == 100 and p['axion_coupling'].to_value('1e-10/GeV') in (2,4,10,12,14,16,20)) or \
(p['axion_mass'].to_value('MeV') == 200 and p['axion_coupling'].to_value('1e-10/GeV') in (2,4,6,8,10,20))

_param_abbrv = {
'axion_mass': '[0, 100, 200] MeV',
'axion_coupling' : '[0..20] 1e-10/GeV' }

def __new__(cls, axion_mass, axion_coupling):
"""Model Initialization.

Parameters
----------
axion_mass: int
Axion mass in units of MeV. Valid values are {axion_mass}.
axion_coupling: int
Axion-photon coupling, in units of 1e-10/GeV. Valid values are {axion_coupling}.
"""
# Make sure axion coupling is converted to units 1e-10/GeV:
axion_coupling = np.round(axion_coupling.to('1e-10/GeV'))

# Load from Parameters
cls.check_valid_params(cls, axion_mass=axion_mass, axion_coupling=axion_coupling)

if axion_mass == 0:
filename = 't-prof_std.dat'
else:
filename = f't-prof_{axion_mass.to_value("MeV"):g}_{axion_coupling.to_value("1e-10/GeV"):g}.dat'

# PNS mass table, from Mori+ 2023.
mpns = { (0, 0): 1.78,
(100, 2): 1.77,
(100, 4): 1.76,
(100, 10): 1.77,
(100, 12): 1.77,
(100, 14): 1.77,
(100, 16): 1.77,
(100, 20): 1.74,
(200, 2): 1.77,
(200, 4): 1.76,
(200, 6): 1.75,
(200, 8): 1.74,
(200, 10): 1.73,
(200, 20): 1.62 }

am = int(axion_mass.to_value('MeV'))
ac = int(axion_coupling.to_value('1e-10/GeV'))
pns_mass = mpns[(am,ac)]

# Set the metadata.
metadata = {
'Axion mass': axion_mass,
'Axion coupling': axion_coupling,
'Progenitor mass': 20*u.Msun,
'PNS mass' : pns_mass*u.Msun
}

return loaders.Mori_2023(filename, metadata)

# Populate Docstring with abbreviated param values
__new__.__doc__ = __new__.__doc__.format(**_param_abbrv)


class SNOwGLoBES:
"""A model that does not inherit from SupernovaModel (yet) and imports a group of SNOwGLoBES files."""

Expand Down
56 changes: 56 additions & 0 deletions python/snewpy/models/loaders.py
Original file line number Diff line number Diff line change
Expand Up @@ -749,3 +749,59 @@ def __init__(self, filename, metadata={}):
# Note factor of 0.25 in nu_x and nu_x_bar.
factor = 1. if flavor.is_electron else 0.25
self.luminosity[flavor] = np.sum(dLdE*dE, axis=1) * factor * 1e50 * u.erg/u.s


class Mori_2023(PinchedModel):
def __init__(self, filename, metadata={}):
"""
Parameters
----------
filename : str
Absolute or relative path to file prefix.
"""
# Set up model metadata
self.axion_mass = metadata['Axion mass']
self.axion_coupling = metadata['Axion coupling']
self.progenitor_mass = metadata['Progenitor mass']
self.pns_mass = metadata['PNS mass']

self.metadata = metadata

# Open the requested filename using the model downloader.
datafile = _model_downloader.get_model_data(self.__class__.__name__, filename)

# Read ASCII data.
simtab = Table.read(datafile, format='ascii')

# Remove the first table row, which appears to have zero input.
simtab = simtab[simtab['1:t_sim[s]'] > 0]

# Get grid of model times.
simtab['TIME'] = simtab['2:t_pb[s]'] << u.s
for j, (f, fkey) in enumerate(zip([Flavor.NU_E, Flavor.NU_E_BAR, Flavor.NU_X], 'ebx')):
simtab[f'L_{f.name}'] = simtab[f'{6+j}:Le{fkey}[e/s]'] << u.erg / u.s
# Compute the pinch parameter from E_rms and E_avg
# <E^2> / <E>^2 = (2+a)/(1+a), where
# E_rms^2 = <E^2> - <E>^2.
Eavg = simtab[f'{9+j}:Em{fkey}[MeV]']
Erms = simtab[f'{12+j}:Er{fkey}[MeV]']
E2 = Erms**2 + Eavg**2
x = E2 / Eavg**2
alpha = (2-x) / (x-1)

simtab[f'E_{f.name}'] = Eavg << u.MeV
simtab[f'E2_{f.name}'] = E2 << u.MeV**2
simtab[f'ALPHA_{f.name}'] = alpha

# simtab[f'E_{f.name}'] = simtab[f'{9+j}:Em{fkey}[MeV]'] << u.MeV
# Erms = simtab[f'{12+j}:Er{fkey}[MeV]'] * u.MeV
#
# # Compute the pinch parameter from E_rms and E_avg
# simtab[f'E2_{f.name}'] = Erms**2 + simtab[f'E_{f.name}']**2
# x = simtab[f'E2_{f.name}'] / simtab[f'E_{f.name}']**2
# simtab[f'ALPHA_{f.name}'] = (2-x) / (x-1)

self.filename = os.path.basename(filename)

super().__init__(simtab, metadata)

3 changes: 3 additions & 0 deletions python/snewpy/models/model_files.yml
Original file line number Diff line number Diff line change
Expand Up @@ -50,3 +50,6 @@ models:
Zha_2021:
repository: *snewpy

Mori_2023:
repository: *ccsnmodels

36 changes: 35 additions & 1 deletion python/snewpy/test/test_01_registry.py
Original file line number Diff line number Diff line change
Expand Up @@ -9,7 +9,7 @@
Sukhbold_2015, Bollig_2016, Walk_2018, \
Walk_2019, Fornax_2019, Warren_2020, \
Kuroda_2020, Fornax_2021, Zha_2021, \
Fornax_2022
Fornax_2022, Mori_2023

from astropy import units as u

Expand All @@ -33,6 +33,7 @@ def test_param_combinations(self):
Fornax_2021,
Zha_2021,
Fornax_2022,
Mori_2023,
]

for model in models:
Expand Down Expand Up @@ -394,3 +395,36 @@ def test_Fornax_2022(self):
self.assertEqual(len(f), len(Flavor))
self.assertEqual(f[Flavor.NU_E].unit, 1/(u.erg * u.s))

def test_Mori_2023(self):
"""
Instantiate a set of 'Mori 2023' models
"""
axion_mass_coupling = [ (0,0),
(100,2), (100,4), (100,10), (100,12), (100,14), (100,16), (100,20),
(200,2), (200,4), (200,6), (200,8), (200,10), (200,20)]

pns_mass = [1.78, 1.77, 1.76, 1.77, 1.77, 1.77, 1.77, 1.74, 1.77, 1.76, 1.75, 1.74, 1.73, 1.62] * u.Msun

for ((am, ac), mpns) in zip(axion_mass_coupling, pns_mass):
model = Mori_2023(axion_mass=am*u.MeV, axion_coupling=ac*1e-10/u.GeV)

axion_mass = float(am) * u.MeV
self.assertEqual(model.metadata['Axion mass'], axion_mass)

axion_coupling = float(ac) * 1e-10/u.GeV
axion_coupling = np.round(axion_coupling.to('1e-10/GeV'))
self.assertEqual(model.metadata['Axion coupling'], axion_coupling)

self.assertEqual(model.metadata['Progenitor mass'], 20*u.Msun)
self.assertEqual(model.metadata['PNS mass'], mpns)

# Check that times are in proper units.
t = model.get_time()
self.assertTrue(t.unit, u.s)

# Check that we can compute flux dictionaries.
f = model.get_initial_spectra(0*u.s, 10*u.MeV)
self.assertEqual(type(f), dict)
self.assertEqual(len(f), len(Flavor))
self.assertEqual(f[Flavor.NU_E].unit, 1./(u.erg * u.s))