Two-Dimensional Simulation of Core-Collapse Supernovae: Role of Anisotropic Neutrino Radiation on Explosion Dynamics

Details Two-Dimensional Simulation of Core-Collapse Supernovae: Role of Anisotropic Neutrino Radiation on Explosion Dynamics Two-Dimensional Simulation of Core-Collapse Supernovae: Role of Anisotropic Neutrino Radiation on Explosion Dynamics

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..847..430m&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: International Symposium on Origin of Matter and Evolution of Galaxies 2005: New Hori

Astronomy and Astrophysics

Astrophysics

Supernovae, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

We perform two-dimensional numerical simulations of core-collapse supernovae. Starting from a rotating progenitor, we obtain a deformed neutrino sphere in a oblate shape in which the ratio of the polar axis to the equatorial one is ~ 5%. This implies anisotropy of ~ 5% in the emerging neutrino flux. Combined with our previous results, this anisotropy in neutrino radiation is sufficient to increase the explosion energy compared with that of spherical models, and can lead to a successful explosion.

Affiliated with

Also associated with

No associations

Rating

Two-Dimensional Simulation of Core-Collapse Supernovae: Role of Anisotropic Neutrino Radiation on Explosion Dynamics does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Two-Dimensional Simulation of Core-Collapse Supernovae: Role of Anisotropic Neutrino Radiation on Explosion Dynamics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Two-Dimensional Simulation of Core-Collapse Supernovae: Role of Anisotropic Neutrino Radiation on Explosion Dynamics will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1136919