Pressure-supported Collapse

Pressure-Supported Collapse is a theoretical astrophysical model in which the gravitational contraction of a gaseous or stellar system proceeds while being temporarily counterbalanced by internal thermal or degeneracy pressure, distinguishing it from pressure-free or dynamically unstable collapse scenarios.

73

Publications

5K

Citations

251

Authors

119

Institutions

Publications per year

2017–2026

14

Authors

251

  1. PS
    Pankaj S. Joshi

    Tata Institute of Fundamental Research, India

    7 publications · 217 citations

    7

    h-index

  2. AS
    A. San Miguel

    Université Claude Bernard Lyon 1, France

    5 publications · 248 citations

    5

    h-index

  3. RG
    Rituparno Goswami

    University of KwaZulu-Natal, South Africa

    3 publications · 68 citations

    3

    h-index

  4. AG
    A. G. Souza Filho

    Universidade Federal do Ceará, Brazil

    3 publications · 155 citations

    3

    h-index

  5. DM
    Denis Machon

    Université Claude Bernard Lyon 1, France

    3 publications · 191 citations

    3

    h-index

1–5 of 251

Venues

  1. Thin-Walled Structures

    4 publications · 214 citations

    4

    h-index

  2. Classical and Quantum Gravity

    4 publications · 125 citations

    4

    h-index

  3. Physical review. D/Physical review. D.

    PRD · 3 publications · 95 citations

    3

    h-index

  4. International Journal of Modern Physics D

    3 publications · 77 citations

    3

    h-index

  5. 3

    h-index

1–5