Nonlinear Structure Formation

Nonlinear Structure Formation is a theoretical framework in cosmology that describes the gravitational evolution of matter density fluctuations in the late universe, distinguishing itself from linear perturbation theory by accounting for the complex, scale-dependent clustering of dark matter and baryons under strong gravitational interactions.

331

Publications

28.4K

Citations

695

Authors

362

Institutions

Publications per year

2017–2026

56

Authors

695

  1. BL
    Baojiu Li

    Durham University, United Kingdom

    9 publications · 835 citations

    9

    h-index

  2. SF
    S. F. Shandarin

    University of Kansas, United States

    8 publications · 1.3K citations

    8

    h-index

  3. PC
    Peter Coles

    Queen Mary University of London, United Kingdom

    6 publications · 280 citations

    6

    h-index

  4. PB
    Philippe Brax

    Commissariat à l'Énergie Atomique et aux Énergies Alternatives, France

    6 publications · 581 citations

    6

    h-index

  5. AL
    Adrian L. Melott

    University of Kansas, United States

    6 publications · 348 citations

    6

    h-index

1–5 of 695

Venues

  1. 35

    h-index

  2. The Astrophysical Journal

    ApJ · 50 publications · 9.9K citations

    33

    h-index

  3. Journal of Cosmology and Astroparticle Physics

    JCAP · 32 publications · 2.1K citations

    25

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    24 publications · 1.4K citations

    21

    h-index

  5. Physical review. D/Physical review. D.

    PRD · 29 publications · 1.1K citations

    20

    h-index

1–5