Probing Explosion Geometry of Core-collapse Supernovae with Light Curves of the Shock Breakout
Akihiro Suzuki, Toshikazu Shigeyama

TL;DR
This paper explores how aspherical energy deposition in core-collapse supernovae affects the shock breakout light curves, proposing that these light curves can reveal explosion geometry details.
Contribution
It introduces a two-dimensional hydrodynamical model to simulate aspherical supernova explosions and derives light curves to link shock breakout features with explosion asymmetry.
Findings
Shock breakout light curves vary with explosion geometry
Aspherical energy deposition influences shock propagation timing
Light curves can serve as indicators of supernova asymmetry
Abstract
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.
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