arXiv Analytics

Sign in

arXiv:1006.1705 [astro-ph.HE]AbstractReferencesReviewsResources

Probing Explosion Geometry of Core-collapse Supernovae with Light Curves of the Shock Breakout

Akihiro Suzuki, Toshikazu Shigeyama

Published 2010-06-09Version 1

We investigate effects of aspherical energy deposition in core-collapse supernovae on the light curve of the supernova shock breakout. We performed two-dimensional hydrodynamical calculations of an aspherical supernova explosion to obtain the time when a shock wave generated in the stellar interior reaches the stellar surface in each radial direction. Using results of the calculations, light curves during the shock breakout are derived in an approximate way. We show that the light curve during the shock breakout can be a strong indicator of aspherical properties of core-collapse supernovae.

Related articles: Most relevant | Search more
arXiv:1112.6328 [astro-ph.HE] (Published 2011-12-29)
Strange matter in core-collapse supernovae
arXiv:2112.03613 [astro-ph.HE] (Published 2021-12-07, updated 2022-02-22)
Shock Revival in Core-collapse Supernovae Assisted by Heavy Axion-like Particles
arXiv:2201.01397 [astro-ph.HE] (Published 2022-01-05)
Inferring Astrophysical Parameters of Core-Collapse Supernovae from their Gravitational-Wave Emission