3 papers
astro-ph.HE2019
Crust Cooling Models are Insensitive to the Crust-Core Transition Pressure for Realistic Equations of State
Sudhanva Lalit, Zach Meisel, Edward F. Brown
Neutron stars cooling after sustained accretion outbursts provide unique information about the neutron star crust and underlying dense matter. Comparisons between astronomical obse…
astro-ph.HE2019
Treating quarks within neutron stars
Sophia Han, M. A. A. Mamun, S. Lalit +2
Neutron star interiors provide the opportunity to probe properties of cold dense matter in the QCD phase diagram. Utilizing models of dense matter in accord with nuclear systematic…
astro-ph.HE2018
Dense matter equation of state for neutron star mergers
S. Lalit, M. A. A. Mamun, C. Constantinou +1
In simulations of binary neutron star mergers, the dense matter equation of state (EOS) is required over wide ranges of density and temperature as well as under conditions in which…