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What Happens When a Massive Star Fails (Sort of) to Explode?

There are observational and theoretical reasons to suspect that up to 10s of percent of massive stars that undergo core-collapse at the end of their lives fail to explode in a canonical energetic supernova explosion. In this talk I will describe what transpires in such nominally failed supernovae and its importance for understanding the masses and spins of black holes (e.g., detected by LIGO). I will also describe how 'failed' supernovae may manifest themselves observationally in time-domain surveys.

Speaker: Eliot Quataert, UC Berkeley

Thursday, 11/14/19


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Stanford Linear Accelerator (SLAC)

Building 51
3rd Floor Conference room
Menlo Park, CA 94025