Abstract
Standing accretion shock instability (SASI) is one of the candidates to solve the mystery of why we cannot reproduce the explosion with the present core-collapse supernova models. We have studied this phenomenon with including neutrino heating and realistic EOS and found that SASI may enhance neutrino heating. Although g-mode of proto-neutron star may enhance the SASI growth, the simulations just including the pressure perturbation as a mimic of g-mode induced sound wave reveal no significant effect on the shock dynamics. Moreover, we discuss the required conditions toward the possible laboratory experiment of SASI.
Original language | English |
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Article number | 042018 |
Journal | Journal of Physics: Conference Series |
Volume | 112 |
Issue number | Part 4 |
DOIs | |
Publication status | Published - 2008 Jun 12 |
Event | 5th International Conference on Inertial Fusion Sciences and Applications, IFSA 2007 - Kobe, Japan Duration: 2007 Sep 9 → 2007 Sep 14 |
ASJC Scopus subject areas
- Physics and Astronomy(all)