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LIGO Seminar

Tuesday, February 26, 2019
1:00pm to 2:00pm
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West Bridge 351 (LIGO Science Conference Room)
Core-collapse Supernova Physics in the Multimessenger Era
Sarah Gossan, LIGO, Department of Physics, Caltech,
  • Public Event

Eighty-five years following the historic proposal that core-collapse supernovae (CCSNe) accompanied the transition of evolved massive stars to neutron stars, the mechanism through which these transients explode remain uncertain. Numerical simulations, arguably a fourth messenger of sorts, employ approximations to improve viability of broad parameter space studies for CCSNe. We discuss the impact of failure to accurately capture proto-neutron star hydrodynamics in the context of explodability of progenitor stars. Furthermore, we discuss the prospects for detection of GWs from CCSNe with the third-generation of ground-based GW detectors, and consider the limitations to inferring CCSN science through GW observations moving forward.

For more information, please contact Sydney Meshkov by phone at 626-395-2129 or by email at [email protected].

Event Series
LIGO Seminar Series