Self-similar Collapse
Self-Similar Collapse is a theoretical model in astrophysics that describes the process of gravitational collapse in which the spatial and temporal evolution of the collapsing system exhibits invariance under scaling transformations, such that the density and velocity profiles maintain a proportional form throughout the collapse.
218
Publications
15.2K
Citations
338
Authors
212
Institutions
Publications per year
2017–2026
21
Parents
218
Self-similar collapse of isothermal spheres and star formation
Frank H. Shu · The Astrophysical Journal · 1977 · 1.7K citations
Natural Sciences, Astronomy, Physics +16
Self-similar gravitational collapse in an expanding universe
J. A. Fillmore, Peter Goldreich · The Astrophysical Journal · 1984 · 552 citations · Full text
Natural Sciences, Astronomy, Physics +14
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212

Tata Institute of Fundamental Research
Mumbai, India
11 h-index
23 publications
1.6K citations

Universidade do Estado do Rio de Janeiro
Rio de Janeiro, Brazil
10 h-index
20 publications
451 citations
University of Chicago
Chicago, United States
9 h-index
11 publications
339 citations

Centre National de la Recherche Scientifique
Paris, France
8 h-index
13 publications
744 citations
University of Southampton
Southampton, United Kingdom
8 h-index
10 publications
225 citations
Tsinghua University
Beijing, China
8 h-index
15 publications
467 citations
Max Planck Institute for Gravitational Physics
Potsdam, Germany
7 h-index
10 publications
252 citations
National Astronomical Observatories
Beijing, China
6 h-index
6 publications
213 citations
1–8 of 212
42 publications · 2.3K citations
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ApJ · 27 publications · 4.3K citations
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PRL · 16 publications · 1.7K citations
16
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19 publications · 1.1K citations
14
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11 publications · 754 citations
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