Physics – Fluid Dynamics
Scientific paper
Oct 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..797..138l&link_type=abstract
INTERACTING BINARIES: Accretion, Evolution, and Outcomes. AIP Conference Proceedings, Volume 797, pp. 138-143 (2005).
Physics
Fluid Dynamics
1
Accretion Disks, Astrophysical Fluid Dynamics, Neutrinos, Gamma-Ray Sources (Astronomical), Neutron Stars, Accretion And Accretion Disks, Hydrodynamics, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays, Gamma-Ray Sources, Gamma-Ray Bursts, Neutron Stars
Scientific paper
The evolution of accretion disks in the so-called hypercritical regime, where the main source of cooling is neutrino emission, is relevant for the study of gamma ray burst (GRB) central engines. For short bursts, which may arise from compact binary merger remnant disks, no external agent feeds the disk, and when the initial mass supply is exhausted no further energy release is possible. For long bursts, possibly arising from massive rotating core collapse, the infalling envelope may supply the disk with matter and allow the energy release to continue for some time. We give here a general overview of the conditions in such disks, and present detailed calculations of their structure and evolution (for the particular case of disks arising from mergers), taking into account the effects of neutrino opacities.
No associations
LandOfFree
Dynamical evolution of neutrino cooled disks 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 Dynamical evolution of neutrino cooled disks, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamical evolution of neutrino cooled disks will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1618840