Constraining neutron star interior properties with transient events from accreting neutron stars and magnetars

APA

Cumming, A. (2013). Constraining neutron star interior properties with transient events from accreting neutron stars and magnetars. Perimeter Institute for Theoretical Physics. https://pirsa.org/13040138

MLA

Cumming, Andrew. Constraining neutron star interior properties with transient events from accreting neutron stars and magnetars. Perimeter Institute for Theoretical Physics, Apr. 25, 2013, https://pirsa.org/13040138

BibTex

          @misc{ scivideos_PIRSA:13040138,
            doi = {10.48660/13040138},
            url = {https://pirsa.org/13040138},
            author = {Cumming, Andrew},
            keywords = {Strong Gravity},
            language = {en},
            title = {Constraining neutron star interior properties with transient events from accreting neutron stars and magnetars},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2013},
            month = {apr},
            note = {PIRSA:13040138 see, \url{https://scivideos.org/pirsa/13040138}}
          }
          

Andrew Cumming McGill University

Source Repository PIRSA
Collection

Abstract

The last few years have seen new opportunities for constraining the physics of neutron star interiors. I will first discuss the current state of neutron star radius measurements and then go on to discuss thermal tomography as a probe of the nuclear, magnetic, and transport properties of neutron star crusts. In each case, I will emphasize the astrophysics that must be understood to make reliable inferences about the properties of dense matter from observations of neutron stars.