Compact Binary Inspirals
Compact Binary Inspirals is a dynamical astrophysical process in which two compact objects, such as neutron stars or black holes, gradually spiral toward each other due to the emission of gravitational radiation, ultimately leading to merger within the framework of post-Newtonian gravity.
225
Publications
28.3K
Citations
2.4K
Authors
371
Institutions
Publications per year
2017–2026
83
Parents
225
Tests of General Relativity with GW150914
B. P. Abbott, R. Abbott, T. D. Abbott et al. · Physical Review Letters · 2016 · 1.8K citations · Full text
Natural Sciences, Astronomy, Physics +15
Properties of the Binary Neutron Star Merger GW170817
B. P. Abbott, R. Abbott, T. D. Abbott et al. · Physical Review X · 2019 · 1.3K citations · Full text
Natural Sciences, Astronomy, Physics +13
1–5 of 225
2.4K
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University of Maryland, College Park, United States
13 publications · 3.5K citations
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11
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371
Max Planck Institute for Gravitational Physics
Potsdam, Germany
27 h-index
425 publications
339.7K citations

Centre National de la Recherche Scientifique
Paris, France
26 h-index
196 publications
153.6K citations
California Institute of Technology
Pasadena, United States
25 h-index
495 publications
305.7K citations
University of Maryland, College Park
College Park, United States
22 h-index
56 publications
25.3K citations
Northwestern University
Evanston, United States
20 h-index
86 publications
41.2K citations
Institut d'Astrophysique de Paris
Paris, France
18 h-index
30 publications
5.7K citations
Carleton College
Northfield, United States
18 h-index
31 publications
14.5K citations

University of Birmingham
Birmingham, United Kingdom
15 h-index
99 publications
78K citations
1–8 of 371
45 publications · 5.7K citations
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PRD · 40 publications · 3.2K citations
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34 publications · 1.9K citations
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17 publications · 5.4K citations
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ApJ · 18 publications · 3.5K citations
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