Long time supernova neutrino simulations

Long time neutrino simulation data up to 20 seconds with no neutrino oscillation

File names are formatted as below:

model.A.bary.B.BB_grav.C.CC.dat

A is a model number and B.BB is a baryonic mass and C.CC is a gravitational mass.

Neutron star masses are measured at 20 seconds.

Readme.txt
    explanation of each file

model1.bary.1.27_grav.1.36.dat

    includes neutrino fluxes and luminosities from z9.6 in the Nakazato format (see below and http://asphwww.ph.noda.tus.ac.jp/snn/guide.pdf).

    See
        https://academic.oup.com/ptep/article/2021/2/023E01/6045986
    for more details on the z9.6 supernova explosion.

model2.bary.1.41_grav.1.31.dat

    includes neutrino spectra from a supernova which leave a neutron star of 1.41 Msun in baryonic mass and 1.31 in gravitational mass.

model3.bary.1.22_grav.1.29.dat

    includes neutrino spectra from a supernova which leave a neutron star of 1.22 Msun in baryonic mass and 1.29 in gravititonal mass.

sn_spectra.py
    a python script which interprets the nakazato format.
    If you run the script from command line, the script outputs fluxes and luminosities and average energies for each flavor.

Nakazato format

    The Nakazato format contains time evolutions of neutrino spectra and is a suitable format for estimation of supernova neutrino signals on earth.

"T0
  E0  E1    dN_nue(T0)/dE1  dN_anue(T0)/dE1  dN_nux(T0)/dE1  dL_nue(T0)/dE1  dL_anue(T0)/dE1  dL_nux(T0)/dE1 
  E1  E2    dN_nue(T0)/dE2  dN_anue(T0)/dE1  dN_nux(T0)/dE2  dL_nue(T0)/dE2  dL_anue(T0)/dE2  dL_nux(T0)/dE2 
  .
  .
  .
  E19 E20   dN_nue(T0)/dE20 dN_anue(T0)/dE20 dN_nux(T0)/dE20 dL_nue(T0)/dE20 dL_anue(T0)/dE20 dL_nux(T0)/dE20

  T1
  E0  E1    dN_nue(T0)/dE1  dN_anue(T1)/dE1  dN_nux(T1)/dE1  dL_nue(T1)/dE1  dL_anue(T1)/dE1  dL_nux(T1)/dE1
  .
  .
  .
",where Tn [s] is a time measured from the bounce and Ek [MeV] is a neutrino energy.