General-relativistic hydrodynamics simulation of a neutron star–sub-solar-mass black hole merger-Reference-Cited by-同舟云学术

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General-relativistic hydrodynamics simulation of a neutron star–sub-solar-mass black hole merger

Published:2023-09-13 Issue:6 Volume:108 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Markin Ivan^ORCID,Neuweiler Anna^ORCID,Abac Adrian^ORCID,Chaurasia Swami Vivekanandji,Ujevic Maximiliano^ORCID,Bulla Mattia^ORCID,Dietrich Tim^ORCID

Funder

Deutsche Forschungsgemeinschaft

Vetenskapsrådet

Daimler und Benz Stiftung

Leibniz-Rechenzentrum

High Performance Computing (HPC) Center Stuttgart

North German Supercomputing Alliance

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.108.064025/fulltext

Reference95 articles.

1. Observation of Gravitational Waves from a Binary Black Hole Merger

2. GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

3. Multi-messenger Observations of a Binary Neutron Star Merger

4. Observation of Gravitational Waves from Two Neutron Star–Black Hole Coalescences

5. Advanced LIGO

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1. Using equation of state constraints to classify low-mass compact binary mergers;Physical Review D;2024-09-09

2. Can we identify primordial black holes? Tidal tests for subsolar-mass gravitational-wave observations;Physical Review D;2024-06-27

3. Prospects of detection of subsolar mass primordial black hole and white dwarf binary mergers;Physical Review D;2024-05-10

4. M1 neutrino transport within the numerical-relativistic code BAM with application to low mass binary neutron star mergers;Physical Review D;2024-02-05

5. New and robust gravitational-waveform model for high-mass-ratio binary neutron star systems with dynamical tidal effects;Physical Review D;2024-01-31

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