Chameleon Fields

Chameleon Fields is a theoretical scalar field model in cosmology that belongs to the class of modified gravity theories and is distinguished by its environment-dependent mass, allowing it to evade local gravitational constraints while driving cosmic acceleration.

192

Publications

14.4K

Citations

334

Authors

222

Institutions

Publications per year

2017–2026

32

Authors

334

  1. PB
    Philippe Brax

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

    20 publications · 1.6K citations

    16

    h-index

  2. AD
    Anne-Christine Davis

    University of Cambridge, United Kingdom

    15 publications · 1.4K citations

    14

    h-index

  3. JK
    Justin Khoury

    University of Pennsylvania, United States

    13 publications · 5.5K citations

    13

    h-index

  4. CB
    Clare Burrage

    University of Nottingham, United Kingdom

    8 publications · 210 citations

    8

    h-index

  5. DJ
    Douglas J. Shaw

    University of Cambridge, United Kingdom

    8 publications · 989 citations

    8

    h-index

1–5 of 334

Venues

  1. 31

    h-index

  2. Journal of Cosmology and Astroparticle Physics

    JCAP · 23 publications · 986 citations

    18

    h-index

  3. Physical Review Letters

    PRL · 17 publications · 3.9K citations

    16

    h-index

  4. Physical review. D/Physical review. D.

    PRD · 14 publications · 522 citations

    13

    h-index

  5. arXiv (Cornell University)

    Repository · 7 publications · 137 citations

    7

    h-index

1–5