A Bayesian model mixing approach to the dense matter equation of state

Presenter Information

Alexandra Semposki

Author ORCID

0000-0003-2354-1523

Abstract

I use the novel statistical technique, Bayesian model mixing, to combine theoretical models of neutron star equations of state and compare the resulting predictions to known gravitational wave and pulsar observations.

Status

Graduate

Department

Physics & Astronomy

College

College of Arts and Sciences

Campus

Athens

Faculty Mentor

Daniel R Phillips

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A Bayesian model mixing approach to the dense matter equation of state

I use the novel statistical technique, Bayesian model mixing, to combine theoretical models of neutron star equations of state and compare the resulting predictions to known gravitational wave and pulsar observations.