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

Authors

338

  1. CG
    Carsten Gundlach

    University of Southampton, United Kingdom

    13 publications · 526 citations

    12

    h-index

  2. MW
    Matthew W. Choptuik

    University of British Columbia, Canada

    8 publications · 506 citations

    8

    h-index

  3. EH
    Eric Hirschmann

    Brigham Young University, United States

    6 publications · 339 citations

    6

    h-index

  4. TH
    Tomohiro Harada

    Rikkyo University, Japan

    6 publications · 231 citations

    6

    h-index

  5. YL
    Yuqing Lou

    Shanghai Chest Hospital, China

    6 publications · 135 citations

    6

    h-index

1–5 of 338

Venues

  1. 26

    h-index

  2. The Astrophysical Journal

    ApJ · 27 publications · 4.3K citations

    22

    h-index

  3. Physical Review Letters

    PRL · 16 publications · 1.7K citations

    16

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    19 publications · 1.1K citations

    14

    h-index

  5. Classical and Quantum Gravity

    11 publications · 754 citations

    11

    h-index

1–5