Venue: Physics Building, Max-von-Laue-Str. 1, Seminar Room PHYS 2.116
Time: Monday, October 24, 3:15 pm
Contact: hees@fias.uni-frankfurt.de
I will
outline how we might combine theory, current and upcoming
multi-messenger observations of neutron stars and terrestrial
experiments to unravel the properties of cold dense matter. I will
discuss calculations of the equation of state (EOS), observations of
neutron-star masses and radii, and suggest that taken together they
favor a rapid increase in the pressure of neutron-rich matter in the
vicinity of nuclear saturation density. Time permitting, I will
discuss the thermal and transport properties of cold dense matter and
strategies to constrain them using observations of accreting
neutron stars.