Understanding Core-Collapse Supernovae

Details Understanding Core-Collapse Supernovae Understanding Core-Collapse Supernovae

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010nupha.834..602h&link_type=abstract

Nuclear Physics A, Volume 834, Issue 1-4, p. 602-607c.

Physics

Nuclear Physics

Scientific paper

Our understanding of core-collapse supernovae continues to improve as better microphysics is included in increasingly realistic neutrino-radiationhydrodynamic simulations. Recent multi-dimensional models with spectral neutrino transport, which slowly develop successful explosions for a range of progenitors between 12 and 25 solar mass, have motivated changes in our understanding of the neutrino reheating mechanism. In a similar fashion, improvements in nuclear physics, most notably explorations of weak interactions on nuclei and the nuclear equation of state, continue to refine our understanding of how supernovae explode. Recent progresses on both the macroscopic and microscopic effects that affect core-collapse supernovae are discussed.

Affiliated with

Also associated with

No associations

Rating

Understanding Core-Collapse Supernovae 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 Understanding Core-Collapse Supernovae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Understanding Core-Collapse Supernovae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1224406