Scalar Perturbations

Scalar Perturbations is a type of primordial density fluctuation in the early universe that belongs to the class of cosmological perturbations characterized by spatial variations in the energy density and gravitational potential, distinguished from vector and tensor perturbations by its invariance under spatial rotations and its role in seeding large-scale structure formation through gravitational instability.

1.6K

Publications

120.8K

Citations

2K

Authors

824

Institutions

Publications per year

2017–2026

460

Authors

2K

  1. ST
    Shinji Tsujikawa

    Tokyo University of Science, Japan

    23 publications · 2.1K citations

    20

    h-index

  2. RB
    Robert Brandenberger

    McGill University, Canada

    20 publications · 1.7K citations

    17

    h-index

  3. BW
    Bin Wang

    Shanghai Jiao Tong University, China

    16 publications · 842 citations

    15

    h-index

  4. SM
    Shinji Mukohyama

    The University of Tokyo, Japan

    18 publications · 1K citations

    15

    h-index

  5. SM
    S. Matarrese

    University of Padua, Italy

    15 publications · 1.3K citations

    14

    h-index

1–5 of 2K

Venues

  1. 73

    h-index

  2. Journal of Cosmology and Astroparticle Physics

    JCAP · 292 publications · 17.4K citations

    71

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  3. 61

    h-index

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

    PRD · 195 publications · 7.6K citations

    47

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  5. Physics Letters B

    87 publications · 6.1K citations

    39

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1–5