Flavor-dependent neutrino angular distribution in core-collapse supernovae

Tamborra, I., et al. (2017)

For selected snapshots in time, we provide the radius- and angle-dependent properties of neutrinos emitted from 11.2, 15 and 25 solar mass progenitors (LS220 equation of state). Instructions on how to read the data files presented below are provided here. All data are provided in a coordinate frame that moves with the matter fluid. We also provide an animation of the electron neutrino lepton number variation with radius for the 15 solar mass progenitor. For support or further information, please contact Irene Tamborra (tamborra@nbi.ku.dk).

Animation of the electron neutrino lepton number variation as a function of the radius for an 1D simulation of a 15 solar-mass progenitor (t = 280 ms)

The electron lepton number is always positive. In particular, the dip in the forward direction never turns negative, so there is no crossing between the electron neutrino and antineutrino angular distributions. The animation is available here.

Neutrino angular distributions for 1D simulations of 11.2, 15, and 25 solar-mass progenitors

More information about the progenitors as well as the explosion simulations is available via the following link upon request: Neutrinos from the Formation, Cooling, and Black Hole Collapse of Neutron stars (2014).

1) Neutrino angular distribution for an 1D simulation of an 11.2 solar-mass progenitor

The full energy- and angle-dependent neutrino intensities are available from the PhD thesis by L. Hüdepohl (TU Munich, 2014) and via the following link upon request: Neutrino intensity for a set of progenitors (2012)

a) Radial properties

t = 61 ms

• Radial neutrino properties (61 ms)
• Matter density profile (61 ms)
• Velocity profile (61 ms)
• Central values of the energy bins (61 ms)
• Boundary values of the energy bins (61 ms)
• Radial grid (61 ms)
• Electron abundance (61 ms)

t = 256 ms

• Radial neutrino properties (256 ms)
• Matter density profile (256 ms)
• Velocity profile (256 ms)
• Central values of the energy bins (256 ms)
• Boundary values of the energy bins (256 ms)
• Radial grid (256 ms)
• Electron abundance (256 ms)

t = 550 ms

• Radial neutrino properties (550 ms)
• Matter density profile (550 ms)
• Velocity profile (550 ms)
• Central values of the energy bins (550 ms)
• Boundary values of the energy bins (550 ms)
• Radial grid (550 ms)
• Electron abundance (550 ms)

b) Angular emission properties

t = 61 ms

• Angle- and radius-dependent neutrino properties (61 ms, electron neutrino)
• Angle- and radius-dependent neutrino properties (61 ms, electron antineutrino)
• Angle- and radius-dependent neutrino properties (61 ms, mu,tau neutrino)

t = 256 ms

• Angle- and radius-dependent neutrino properties (256 ms, electron neutrino)
• Angle- and radius-dependent neutrino properties (256 ms, electron antineutrino)
• Angle- and radius-dependent neutrino properties (256 ms, mu,tau neutrino)

t = 550 ms

• Angle- and radius-dependent neutrino properties (550 ms, electron neutrino)
• Angle- and radius-dependent neutrino properties (550 ms, electron antineutrino)
• Angle- and radius-dependent neutrino properties (550 ms, mu,tau neutrino)

2) Neutrino angular distribution for an 1D simulation of a 15 solar-mass progenitor

The full energy- and angle-dependent neutrino intensities are available from the PhD thesis by L. Hüdepohl (TU Munich, 2014) and via the following link upon request: Neutrino intensity for a 15 solar-mass star core collapse (2012)

a) Radial properties

t = 150 ms

• Radial neutrino properties (150 ms)
• Matter density profile (150 ms)
• Velocity profile (150 ms)
• Central values of the energy bins (150 ms)
• Boundary values of the energy bins (150 ms)
• Radial grid (150 ms)
• Electron abundance (150 ms)

t = 280 ms

• Radial neutrino properties (280 ms)
• Matter density profile (280 ms)
• Velocity profile (280 ms)
• Central values of the energy bins (280 ms)
• Boundary values of the energy bins (280 ms)
• Radial grid (280 ms)
• Electron abundance (280 ms)

t = 500 ms

• Radial neutrino properties (500 ms)
• Matter density profile (500 ms)
• Velocity profile (500 ms)
• Central values of the energy bins (500 ms)
• Boundary values of the energy bins (500 ms)
• Radial grid (500 ms)
• Electron abundance (500 ms)

b) Angular emission properties

t = 150 ms

• Angle- and radius-dependent neutrino properties (150 ms, electron neutrino)
• Angle- and radius-dependent neutrino properties (150 ms, electron antineutrino)
• Angle- and radius-dependent neutrino properties (150 ms, mu,tau neutrino)

t = 280 ms

• Angle- and radius-dependent neutrino properties (280 ms, electron neutrino)
• Angle- and radius-dependent neutrino properties (280 ms, electron antineutrino)
• Angle- and radius-dependent neutrino properties (280 ms, mu,tau neutrino)

t = 500 ms

• Angle- and radius-dependent neutrino properties (500 ms, electron neutrino)
• Angle- and radius-dependent neutrino properties (500 ms, electron antineutrino)
• Angle- and radius-dependent neutrino properties (500 ms, mu,tau neutrino)

3) Neutrino angular distribution for an 1D simulation of a 25 solar-mass progenitor

The full energy- and angle-dependent neutrino intensities are available from the PhD thesis by L. Hüdepohl (TU Munich, 2014) and via the following link upon request: Neutrino intensity for a set of progenitors (2012)

a) Radial properties

t = 63 ms

• Radial neutrino properties (63 ms)
• Matter density profile (63 ms)
• Velocity profile (63 ms)
• Central values of the energy bins (63 ms)
• Boundary values of the energy bins (63 ms)
• Radial grid (63 ms)
• Electron abundance (63 ms)

t = 252 ms

• Radial neutrino properties (252 ms)
• Matter density profile (252 ms)
• Velocity profile (252 ms)
• Central values of the energy bins (252 ms)
• Boundary values of the energy bins (252 ms)
• Radial grid (252 ms)
• Electron abundance (252 ms)

t = 352 ms

• Radial neutrino properties (352 ms)
• Matter density profile (352 ms)
• Velocity profile (352 ms)
• Central values of the energy bins (352 ms)
• Boundary values of the energy bins (352 ms)
• Radial grid (352 ms)
• Electron abundance (352 ms)

b) Angular emission properties

t = 63 ms

• Angle- and radius-dependent neutrino properties (63 ms, electron neutrino)
• Angle- and radius-dependent neutrino properties (63 ms, electron antineutrino)
• Angle- and radius-dependent neutrino properties (63 ms, mu,tau neutrino)

t = 252 ms

• Angle- and radius-dependent neutrino properties (252 ms, electron neutrino)
• Angle- and radius-dependent neutrino properties (252 ms, electron antineutrino)
• Angle- and radius-dependent neutrino properties (252 ms, mu,tau neutrino)

t = 352 ms

• Angle- and radius-dependent neutrino properties (352 ms, electron neutrino)
• Angle- and radius-dependent neutrino properties (352 ms, electron antineutrino)
• Angle- and radius-dependent neutrino properties (352 ms, mu,tau neutrino)