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. https://pirsa.org/13040138
MLA
Cumming, Andrew. Constraining neutron star interior properties with transient events from accreting neutron stars and magnetars. Perimeter Institute, Apr. 25, 2013, https://pirsa.org/13040138
BibTex
@misc{ pirsa_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}, year = {2013}, month = {apr}, note = {PIRSA:13040138 see, \url{https://pirsa.org}} }
McGill University
Collection
Talk Type
Subject
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.