PIRSA:11060012

Video URL

https://pirsa.org/11060012

Neutron Star Mass and Radius Constraints for the Dense Matter Equation of State

Lattimer, J. (2011). Neutron Star Mass and Radius Constraints for the Dense Matter Equation of State. Perimeter Institute for Theoretical Physics. https://pirsa.org/11060012

Lattimer, James. Neutron Star Mass and Radius Constraints for the Dense Matter Equation of State. Perimeter Institute for Theoretical Physics, Jun. 20, 2011, https://pirsa.org/11060012 

          @misc{ scivideos_PIRSA:11060012,
            doi = {10.48660/11060012},
            url = {https://pirsa.org/11060012},
            author = {Lattimer, James},
            keywords = {Particle Physics},
            language = {en},
            title = {Neutron Star Mass and Radius Constraints for the Dense Matter Equation of State},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2011},
            month = {jun},
            note = {PIRSA:11060012 see, \url{https://scivideos.org/pirsa/11060012}}
          }

James Lattimer Stony Brook University

Talk numberPIRSA:11060012
DOI10.48660/11060012
Source RepositoryPIRSA
Collection
Talk Type Conference
Subject

Abstract

Recent discoveries, including a 2 solar mass pulsar, rapid cooling in the Cas A supernova remnant, and estimates of masses and radii from photospheric radius expansion bursts and thermal emissions from neutron stars, are able to constrain significantly the properties of dense matter. Implications for the pressure-density relation and properties of superfluids in neutron star interiors will be discussed.