Author: sylvia
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Production of very light elements in kilonovae
We study the production of light elements (Z
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Combining Electromagnetic and Gravitational-Wave Constraints on Neutron-Star Masses and Radii
We perform a joint Bayesian inference of neutron-star mass and radius constraints based on GW170817, observations of quiescent low-mass X-ray binaries (QLMXBs), photospheric radius expansion X-ray bursts (PREs), and X-ray […]
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GW190814 as a massive rapidly-rotating neutron star with exotic degrees of freedom
In the context of the massive secondary object recently observed in the compact-star merger GW190814, we investigate the possibility of producing massive neutron stars from equation of state models that […]
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Constraining hadron-quark phase transition parameters within the quark-mean-field model using multimessenger observations of neutron stars
We extend the quark mean-field (QMF) model for nuclear matter and study the possible presence of quark matter inside the cores of neutron stars. A sharp first-order hadron-quark phase transition […]
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Rank-3 Moment Closures in General Relativistic Neutrino Transport
Many modern simulations of accretion disks use moment-based methods for radiation transport to determine the thermal evolution of the disk and the properties of the ejected matter. The popular M1 […]