Collapse With Rotation
Collapse with Rotation is a theoretical model in astrophysics that describes the asymmetric implosion of a massive stellar core under self-gravity while conserving angular momentum, leading to the formation of a compact object with rotational dynamics and associated phenomena such as accretion disks and jet formation.
142
Publications
11.2K
Citations
313
Authors
170
Institutions
Publications per year
2017–2026
19
Parents
142
On Continued Gravitational Contraction
J. Robert Oppenheimer, Hartland S. Snyder · Physical Review · 1939 · 2K citations · Full text
Natural Sciences, Astronomy, Physics +17
The collapse of the cores of slowly rotating isothermal clouds
S. Terebey, Frank H. Shu, P. Cassen · The Astrophysical Journal · 1984 · 642 citations
Natural Sciences, Astronomy, Physics +16
Inner-horizon instability and mass inflation in black holes
Eric Poisson, W. Israel · Physical Review Letters · 1989 · 325 citations
Natural Sciences, Astronomy, Physics +15
1–5 of 142
313
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170
The University of Tokyo
Tokyo, Japan
11 h-index
17 publications
1.1K citations

Kyoto University
Kyoto, Japan
11 h-index
19 publications
888 citations
University of Illinois Urbana-Champaign
Urbana, United States
8 h-index
17 publications
1.4K citations
California Institute of Technology
Pasadena, United States
7 h-index
19 publications
2.3K citations

Ames Research Center
Mountain View, United States
6 h-index
9 publications
1.2K citations
Los Alamos National Laboratory
Los Alamos, United States
6 h-index
7 publications
786 citations
Tokyo University of the Arts
Tokyo, Japan
5 h-index
6 publications
541 citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
5 h-index
5 publications
240 citations
1–8 of 170
ApJ · 57 publications · 4K citations
33
h-index
12 publications · 696 citations
12
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PRL · 7 publications · 820 citations
7
h-index
6 publications · 626 citations
6
h-index
6 publications · 229 citations
6
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