Compact Object Merger Simulations
Compact Object Merger Simulations is a computational framework that models the dynamical interactions and gravitational wave emissions of coalescing compact astrophysical bodies, such as neutron stars and black holes, through high-resolution numerical relativity and hydrodynamics to predict observable signatures and post-merger remnants.
119
Publications
12.9K
Citations
1.3K
Authors
356
Institutions
Publications per year
2017–2026
65
Parents
119
DOUBLE COMPACT OBJECTS. III. GRAVITATIONAL-WAVE DETECTION RATES
The Astrophysical Journal · 2015 · 432 citations · Full text
Natural Sciences, Astronomy, Physics +15
Formation and Evolution of Compact-object Binaries in AGN Disks
The Astrophysical Journal · 2020 · 372 citations · Full text
Natural Sciences, Astronomy, Physics +12
1–5 of 119
1.3K
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University of Maryland, College Park, United States
5 publications · 482 citations
5
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1–5 of 1.3K
356
Max Planck Institute for Gravitational Physics
Potsdam, Germany
16 h-index
134 publications
15.1K citations

University of Birmingham
Birmingham, United Kingdom
11 h-index
40 publications
4.3K citations
Max Planck Institute for Astrophysics
Garching, Germany
11 h-index
23 publications
1.3K citations
Osservatorio Astronomico di Padova
Padua, Italy
8 h-index
18 publications
2.3K citations
California Institute of Technology
Pasadena, United States
8 h-index
103 publications
10.4K citations
Cardiff University
Cardiff, United Kingdom
7 h-index
31 publications
4K citations
University of California, Berkeley
Berkeley, United States
7 h-index
17 publications
4.8K citations
GSI Helmholtz Centre for Heavy Ion Research
Darmstadt, Germany
6 h-index
8 publications
2K citations
1–8 of 356
29 publications · 3.9K citations
26
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ApJ · 25 publications · 4.1K citations
22
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PRD · 17 publications · 1.1K citations
16
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6 publications · 448 citations
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5 publications · 632 citations
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