activity
20152020
most citedTwo coexisting families of compact stars: observational implications for millisecond pulsars

18 citations · 18 across the 1 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2020

Accretion-induced prompt black hole formation in asymmetric neutron star mergers, dynamical ejecta and kilonova signals

Sebastiano Bernuzzi, Matteo Breschi, Boris Daszuta +9

We present new numerical relativity results of neutron star mergers with chirp mass and mass ratios and using finite-temperature equations of state…

nucl-th2019

Benchmark calculations of pure neutron matter with realistic nucleon-nucleon interactions

M. Piarulli, I. Bombaci, D. Logoteta +2

We report benchmark calculations of the energy per particle of pure neutron matter as a function of the baryon density using three independent many-body methods: Brueckner-Bethe-Go…

nucl-th2019

Impact of chiral hyperonic three-body forces on neutron stars

Domenico Logoteta, Isaac Vidana, Ignazio Bombaci

We study the effect of the nucleon-nucleon-lambda (NN) three-body force on neutron stars. In particular, we consider the NN force recently derived by the Jülich--Bonn--Munich…

astro-ph.HE201718 cited

Two coexisting families of compact stars: observational implications for millisecond pulsars

Sudip Bhattacharyya, Ignazio Bombaci, Domenico Logoteta +1

It is usually thought that a single equation of state (EoS) model "correctly" represents cores of all compact stars. Here we emphasize that two families of compact stars, viz., neu…

nucl-th2015

Comparative study of three-nucleon force models in nuclear matter

Domenico Logoteta, Isaac Vidaña, Ignazio Bombaci +1

We calculate the energy per particle of symmetric nuclear matter and pure neutron matter using the microscopic many-body Brueckner-Hartree-Fock (BHF) approach and employing the Arg…