The Effects of Rotation on Spherical Accretion Shock Instability

Details The Effects of Rotation on Spherical Accretion Shock Instability The Effects of Rotation on Spherical Accretion Shock Instability

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...206.4508u&link_type=abstract

American Astronomical Society Meeting 206, #45.08; Bulletin of the American Astronomical Society, Vol. 37, p.500

Computer Science

Numerical Analysis

Scientific paper

We examine the effects of rotation on the stability of the stalled accretion shock in core-collapse supernovae. Like in Blondin & Mezzacappa (2005), we find that for non-spherical perturbations lower modes are unstable, in particular l=1 is unstable and always dominant. However, the rotation tends to inhibit the growth of such modes, and for high enough rotation even suppress it. We perform our numerical analysis with two different numerical codes: ZEUS-MP and VH-1, and obtain essentially identical results.

Affiliated with

Also associated with

No associations

Rating

The Effects of Rotation on Spherical Accretion Shock Instability 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 The Effects of Rotation on Spherical Accretion Shock Instability, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Effects of Rotation on Spherical Accretion Shock Instability will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1687365