Dark Energy Models

Dark Energy Models is a theoretical framework within cosmological gravity that postulates specific dynamical or modified-gravity mechanisms to explain the observed accelerated expansion of the universe, distinguishing it from alternative cosmological models by attributing this acceleration to an exotic form of energy with negative pressure.

4.4K

Publications

326.1K

Citations

7.3K

Authors

1.5K

Institutions

Publications per year

2017–2026

1.3K

Authors

7.3K

  1. SD
    Sergei D. Odintsov

    Institució Catalana de Recerca i Estudis Avançats, Spain

    63 publications · 18.3K citations

    43

    h-index

  2. XZ
    Xin Zhang

    Northeastern University, China

    57 publications · 4.8K citations

    39

    h-index

  3. SN
    Shin’ichi Nojiri

    Institució Catalana de Recerca i Estudis Avançats, Spain

    52 publications · 17.4K citations

    38

    h-index

  4. SP
    Supriya Pan

    Presidency University, India

    40 publications · 2.6K citations

    34

    h-index

  5. EN
    Emmanuel N. Saridakis

    National Observatory of Athens, Greece

    40 publications · 3.7K citations

    31

    h-index

1–5 of 7.3K

Venues

  1. 121

    h-index

  2. Journal of Cosmology and Astroparticle Physics

    JCAP · 538 publications · 35.4K citations

    93

    h-index

  3. Physics Letters B

    283 publications · 36.1K citations

    91

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    251 publications · 20.5K citations

    70

    h-index

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

    PRD · 326 publications · 18.2K citations

    68

    h-index

1–5