Postmerger emissions: A new and dominant contribution to the gravitational-wave background from binary neutron stars

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-12-08
DOI
https://doi.org/10.1103/4yk2-ltjn
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
0.00
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article

Postmerger emissions: A new and dominant contribution to the gravitational-wave background from binary neutron stars

Karl J. Friston
Physical review. D/Physical review. D.
Pulsars and Gravitational Waves Research
article

Postmerger emissions: A new and dominant contribution to the gravitational-wave background from binary neutron stars

Karl J. Friston
article en

Abstract

No abstract available for this paper.
Physical review. D/Physical review. D.Vol. 113(4)
Goethe University Frankfurt (DE), Goethe-Institute United Kingdom (GB), Institut Universitaire de France (FR), Frankfurt Institute for Advanced Studies (DE), Institut d'Astrophysique de Paris (FR), Sorbonne Université (FR), Laboratoire Médiations (FR)
Openalex Percentile: Top 73%
Pulsars and Gravitational Waves Research
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