A Bayesian model mixing approach to the dense matter equation of state
Author ORCID
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
Creative Commons License
This work is licensed under a Creative Commons Attribution-NonCommercial-No Derivative Works 4.0 International License.
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.