Orateur
Lami Suleiman
(Deutsches Elektronen Synchrotron)
Description
Observations of neutron stars can expand our understanding of strong interaction and help us explore the properties of dense matter in thermodynamic conditions unreachable in laboratories on Earth. In this overview, we discuss the field of extremely dense matter and particularly how gravitational waves combined with other astrophysical detections can constrain the equation of state of dense and neutron-rich matter. We expand on the techniques used to do so, the caveats and various approximations they rely on, and finally comment on the prospects for dense matter exploration with future detections.
Auteur
Lami Suleiman
(Deutsches Elektronen Synchrotron)
