Inspiral Dynamics
Inspiral Dynamics is a theoretical framework within the post-Newtonian approximation that describes the progressive orbital decay and waveform evolution of compact binary systems due to gravitational radiation reaction.
459
Publications
40.3K
Citations
715
Authors
372
Institutions
Publications per year
2017–2026
189
Parents
459
Simple Model of Complete Precessing Black-Hole-Binary Gravitational Waveforms
M. D. Hannam, P. Schmidt, A. Bohé et al. · Physical Review Letters · 2014 · 746 citations · Full text
Natural Sciences, Astronomy, Physics +13
1–5 of 459
715
University of Maryland, College Park, United States
29 publications · 6.9K citations
28
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18
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16
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16
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14
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1–5 of 715
372
California Institute of Technology
Pasadena, United States
45 h-index
122 publications
16.2K citations
Max Planck Institute for Gravitational Physics
Potsdam, Germany
42 h-index
140 publications
18.7K citations

Cornell University
Ithaca, United States
30 h-index
48 publications
6.2K citations
University of Maryland, College Park
College Park, United States
30 h-index
62 publications
10.8K citations

Centre National de la Recherche Scientifique
Paris, France
26 h-index
43 publications
5.3K citations

Institut des Hautes Études Scientifiques
Bures-sur-Yvette, France
24 h-index
34 publications
8.3K citations

Kyoto University
Kyoto, Japan
22 h-index
43 publications
2.9K citations
Max Planck Society
Munich, Germany
20 h-index
25 publications
5.1K citations
1–8 of 372
130 publications · 13.4K citations
64
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PRD · 126 publications · 7.2K citations
46
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35 publications · 7.2K citations
29
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PRL · 26 publications · 3.3K citations
24
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ApJ · 24 publications · 2.2K citations
21
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