Stellar Collapse and Explosion: Relativistic AMR Simulations

Details Stellar Collapse and Explosion: Relativistic AMR Simulations Stellar Collapse and Explosion: Relativistic AMR Simulations

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aps..dppcz2003m&link_type=abstract

American Physical Society, 47th Annual DPP Meeting, October 24-28, 2005, abstract #CZ2.003

Physics

Scientific paper

Numerical simulations of the collapse of massive rotating stars, accretion disk formation and relativistic jet propagation relevant for explosions producing supernovae, gamma-ray bursts (GRBs) and their afterglows will be presented. Outflows driven from the accretion disk formed after core collapse may be responsible for accretion-powered supernova, independent of any GRB-producing jet which may also be produced. The simulations are performed with RAM, a newly written relativistic hydrodynamics code with adaptive mesh refinement (AMR). The importance of AMR for resolving thin structures in relativistic flow is emphasized. RAM will be described and test calculations presented.

Affiliated with

Also associated with

No associations

Rating

Stellar Collapse and Explosion: Relativistic AMR Simulations 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 Stellar Collapse and Explosion: Relativistic AMR Simulations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar Collapse and Explosion: Relativistic AMR Simulations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1620114