Long-term evolution of (short) Gamma-Ray Burst central engines

Details Long-term evolution of (short) Gamma-Ray Burst central engines Long-term evolution of (short) Gamma-Ray Burst central engines

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..20..132l&link_type=abstract

Compact Binaries in the Galaxy and Beyond, Proceedings of the conference held 17-22 November, 2003 in La Paz, Baja California Su

Mathematics

Logic

Accretion, Accretion Disks, Gamma Rays: Bursts, Hydrodynamics, Stars: Neutron

Scientific paper

Cosmological gamma ray bursts (GRBs) possibly originate from accretion disks around stellar mass black holes. These could be formed after the merger of a double neutron star or black hole-neutron star binary. The dynamical evolution of the disk is important if one wishes to relate characteristic timescales with the observed duration and variability. We show here the results of such a set of calculations, relevant for short GRBs.

Affiliated with

Also associated with

No associations

Rating

Long-term evolution of (short) Gamma-Ray Burst central engines 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 Long-term evolution of (short) Gamma-Ray Burst central engines, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Long-term evolution of (short) Gamma-Ray Burst central engines will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-771861