activity
20172022
most citedGW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations

556 citations · 1.3k across the 11 of their papers we have counts for

collaborators

38 papers

gr-qc202210 cited

Kilohertz Gravitational Waves From Binary Neutron Star Mergers: Numerical-relativity Informed Postmerger Model

Matteo Breschi, Sebastiano Bernuzzi, Kabir Chakravarti +3

We present , an analytical model of gravitational-waves from neutron star merger remnants informed using 618 numerical relativity (NR) simulations. is de…

astro-ph.HE2021

Signatures of deconfined quark phases in binary neutron star mergers

Aviral Prakash, David Radice, Domenico Logoteta +6

(abridged) We investigate the quark deconfinement phase transition in the context of binary neutron star (BNS) mergers. We employ a new finite-temperature composition-dependent equ…

astro-ph.HE2021

Dynamical ejecta synchrotron emission as possible contributor to the changing behaviour of GRB170817A

Vsevolod Nedora, David Radice, Sebastiano Bernuzzi +5

Over the past three years, the fading non-thermal emission from the GW170817 remained generally consistent with the afterglow powered by synchrotron radiation produced by the inter…

astro-ph.HE2021

Calibration of the Advanced Spectral Leakage scheme for neutron star merger simulations, and extension to smoothed-particle hydrodynamics

Davide Gizzi, Christoffer Lundman, Evan O'Connor +2

We calibrate a neutrino transport approximation, called Advanced Spectral Leakage (ASL), with the purpose of modeling neutrino-driven winds in neutron star mergers. Based on a numb…

astro-ph.HE2021

AT2017gfo: Bayesian inference and model selection of multi-component kilonovae and constraints on the neutron star equation of state

Matteo Breschi, Albino Perego, Sebastiano Bernuzzi +4

The joint detection of the gravitational wave GW170817, of the short -ray burst GRB170817A and of the kilonova AT2017gfo, generated by the the binary neutron star merger observe…

nucl-th202054 cited

Microscopic equation of state of hot nuclear matter for numerical relativity simulations

Domenico Logoteta, Albino Perego, Ignazio Bombaci

A precise understanding of the equation of state (EOS) of dense and hot matter is key to modeling relativistic astrophysical environments, including core-collapse supernovae (CCSNe…