Equation of state effects on core-collapse supernovae

ORAL

Abstract

Using the recently developed SROEOS code we construct many hot dense equations of state (EOSs) of nuclear matter. We use the newly computed EOSs to investigate how different aspects of nuclear matter affect the dynamics and observables of the core-collapse of a massive star and the properties of the resulting proto-neutron star.

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Authors

  • Andre da Silva Schneider

    • California Institute of Technology

  • Christian Ott

    • None

  • Luke Roberts

    • Michigan State University