activity
20182025
most citedNumerical relativity simulations of prompt collapse mergers: threshold mass and phenomenological constraints on neutron star properties after GW170817

63 citations · 230 across the 8 of their papers we have counts for

collaborators

9 papers

cond-mat.soft2025

Memories of amplitude and direction coexist and compete in non-Brownian suspensions

Surendra Padamata, Nathan C. Keim

Steadily shearing a non-Brownian suspension forms a memory of direction, while shearing back and forth forms a memory of amplitude. Each memory is evident in the systems response t…

astro-ph.HE2023★ 3 cited

Numerical Relativity Estimates of the Remnant Recoil Velocity in Binary Neutron Star Mergers

Sumeet Kulkarni, Surendra Padamata, Anuradha Gupta +2

We present, for the first time, recoil velocity estimates for binary neutron star mergers using data from numerical relativity simulations. We find that binary neutron star merger…

astro-ph.HE2022★ 12 cited

Detectability of Sub-Solar Mass Neutron Stars Through a Template Bank Search

Ananya Bandopadhyay, Brendan Reed, Surendra Padamata +6

We study the detectability of gravitational-wave signals from sub-solar mass binary neutron star systems by the current generation of ground-based gravitational-wave detectors. We…

gr-qc2022★ 57 cited

Second release of the CoRe database of binary neutron star merger waveforms

Alejandra Gonzalez, Francesco Zappa, Matteo Breschi +15

We present the second data release of gravitational waveforms from binary neutron star merger simulations performed by the Computational Relativity (CoRe) collaboration. The curren…

astro-ph.HE2022★ 2 cited

Recoil Velocity of Binary Neutron Star Merger Remnants

Sumeet Kulkarni, Surendra Padamata, Anuradha Gupta

The LIGO-Virgo gravitational wave detectors have confidently observed 4 events involving neutron stars: two binary neutron star (BNS) mergers (GW170817 and GW190425), and two neutr…

astro-ph.HE2022★ 40 cited

Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects

A. Camilletti, L. Chiesa, G. Ricigliano +7

GW190425 was the second gravitational wave (GW) signal compatible with a binary neutron star (BNS) merger detected by the Advanced LIGO and Advanced Virgo detectors. Since no elect…

astro-ph.HE2021★ 53 cited

Probing the incompressibility of nuclear matter at ultra-high density through the prompt collapse of asymmetric neutron star binaries

A. Perego, D. Logoteta, D. Radice +5

Using 250 neutron star merger simulations with microphysics, we explore for the first time the role of nuclear incompressibility in the prompt collapse threshold for binaries with…

astro-ph.HE2021★ 63 cited

Numerical relativity simulations of prompt collapse mergers: threshold mass and phenomenological constraints on neutron star properties after GW170817

Rahul Kashyap, Abhishek Das, David Radice +10

We determine the threshold mass for prompt (no bounce) black hole formation in equal-mass neutron star (NS) mergers using a new set of 227 numerical relativity simulations. We cons…

gr-qc2018

CoRe database of binary neutron star merger waveforms and its application in waveform development

Tim Dietrich, David Radice, Sebastiano Bernuzzi +7

We present the Computational Relativity CoRe collaboration's public database of gravitational waveforms from binary neutron star mergers. The database currently contains 367 wavefo…