Author: sylvia

• research-publ

  Constraints on the neutron star’s maximum densities from postmerger gravitational-waves with third-generation observations

  Using data from 289 numerical relativity simulations of merging binary neutron stars, we identify, for the first time, a robust quasi-universal relation connecting the postmerger peak gravitational-wave frequency and the […]

• research-publ

  Machine Learning for Conservative-to-Primitive in Relativistic Hydrodynamics

  The numerical solution of relativistic hydrodynamics equations in conservative form requires root-finding algorithms that invert the conservative-to-primitive variables map. These algorithms employ the equation of state of the fluid and […]

• research-publ

  High-Order Multipole and Binary Love Number Universal Relations

  Using a data set of approximately 2 million phenomenological equations of state consistent with observational constraints, we construct new equation-of-state-insensitive universal relations that exist between the multipolar tidal deformability parameters […]

• research-publ

  Long-term GRHMD simulation of magnetic field in isolated neutron stars

  Strong magnetic fields play an important role in powering the emission of neutron stars. Nevertheless a full understanding of the interior configuration of the field remains elusive. In this work, […]

• research-publ

  Large and massive neutron stars: implications for the sound speed in dense QCD

  The NASA telescope NICER has recently measured x-ray emissions from the heaviest of the precisely known two-solar mass neutron stars, PSR J0740+6620. Analysis of the data [Miller et al., Astrophys. […]