Cuspy Halo Models

Cuspy Halo Models is a theoretical astrophysical framework characterized by a predicted density profile of dark matter halos that increases sharply toward the galactic center, thereby producing a "cusp" in contrast to observed rotation curves that suggest a more uniform central density.

153

Publications

13.3K

Citations

367

Authors

254

Institutions

Publications per year

2017–2026

31

Authors

367

  1. SM
    Stacy McGaugh

    Case Western Reserve University, United States

    5 publications · 1.2K citations

    5

    h-index

  2. AV
    Andrea V. Macciò

    Max Planck Institute for Astronomy, Germany

    5 publications · 462 citations

    5

    h-index

  3. CB
    Chris B. Brook

    Universidad Autónoma de Madrid, Spain

    5 publications · 523 citations

    5

    h-index

  4. WJ
    W. J. G. de Blok

    University of Cape Town, South Africa

    4 publications · 1.1K citations

    4

    h-index

  5. TQ
    Thomas Quinn

    University of Washington, United States

    4 publications · 429 citations

    4

    h-index

1–5 of 367

Venues

  1. Monthly Notices of the Royal Astronomical Society

    54 publications · 5.5K citations

    36

    h-index

  2. The Astrophysical Journal

    ApJ · 30 publications · 3.4K citations

    23

    h-index

  3. Journal of Cosmology and Astroparticle Physics

    JCAP · 9 publications · 414 citations

    9

    h-index

  4. 8

    h-index

  5. Astronomy and Astrophysics

    6 publications · 259 citations

    6

    h-index

1–5