Probing the gravitational well: no supernova explosion in spherical symmetry with general relativistic boltzmann neutrino transport - INSPIRE

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Probing the gravitational well: no supernova explosion in spherical symmetry with general relativistic boltzmann neutrino transport

Matthias Liebendoerfer
(
- Basel U. and
- Oak Ridge and
- Tennessee U.
)
,
Anthony Mezzacappa
(
- Oak Ridge
)
,
Friederich-Karl Thielemann
(
- Basel U. and
- Oak Ridge
)
,
O.E. Bronson Messer
(
- Oak Ridge and
- Tennessee U.
)
,
W. Raphael Hix
(
- Oak Ridge and
- Tennessee U.
)

Jun, 2000

5 pages

Published in:

Phys.Rev.D 63 (2001) 103004

e-Print:

astro-ph/0006418 [astro-ph]

DOI:

10.1103/PhysRevD.63.103004

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Abstract: (arXiv)

We report on the vigorous supernova explosion of a 13 solar mass star, obtained in a general relativistic spherically symmetric simulation based on Boltzmann neutrino transport. Contrary to the prevailing opinion, the shock revival is more efficient than in the corresponding Newtonian simulation, producing an explosion energy of 10^{51} erg (1 foe) at 187 ms after bounce.

general relativity
supernova
neutrino: cosmic radiation
transport theory
Boltzmann equation
energy
hydrodynamics
neutrino: luminosity
numerical calculations

References(64)

Figures(0)

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