Neutrino Nucleus Reactions and Supernova
Neutrino Nucleus Reactions and Supernova
Neutrino Nucleus Reactions and Supernova
You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
Revival of stalled shock by ν-heatingWhole collapse energy is carried out byneutrinosνAfter bounce~100msec10^53erg (seen by Kamiok<strong>and</strong>e)Rho~1e11g/cm^3T~3MeV Many Alpha existsOnly 1~2% of the neutrino energy isdeposited to the hot matter behind theshock front is enough for supernovaνexplosionννRCNP Workshop, Feb.24, 2005νν10 100 1000kmν-sphereν-heating