PIRSA:14020087

Video URL

https://pirsa.org/14020087

The Radius of Neutron Stars and the Dense Matter Equation of State

Rutledge, R. (2014). The Radius of Neutron Stars and the Dense Matter Equation of State. Perimeter Institute for Theoretical Physics. https://pirsa.org/14020087

Rutledge, Robert. The Radius of Neutron Stars and the Dense Matter Equation of State. Perimeter Institute for Theoretical Physics, Feb. 06, 2014, https://pirsa.org/14020087 

          @misc{ scivideos_PIRSA:14020087,
            doi = {10.48660/14020087},
            url = {https://pirsa.org/14020087},
            author = {Rutledge, Robert},
            keywords = {Strong Gravity},
            language = {en},
            title = {The Radius of Neutron Stars and the Dense Matter Equation of State},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2014},
            month = {feb},
            note = {PIRSA:14020087 see, \url{https://scivideos.org/index.php/pirsa/14020087}}
          }

Robert Rutledge McGill University

Talk numberPIRSA:14020087
DOI10.48660/14020087
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

The equation of state of matter at and above nuclear densities remains a major theoretically uncertain prediction of QCD. Observations of the mass-radius relationship of neutron stars constrain, and can directly measure, the dense matter equation of state. I will discuss how measurements of neutron star radii have already constrained the dEOS, and how future work will directly measure the dEOS, providing an important constraint on models of the strong force.