Non-gaussianity Analysis

Non-Gaussianity Analysis is a statistical methodology in cosmology that characterizes deviations from Gaussianity in the temperature fluctuations of the Cosmic Microwave Background, distinguishing itself by quantifying primordial non-Gaussian signatures to constrain inflationary models and underlying physics of the early universe.

1.2K

Publications

73.9K

Citations

1.9K

Authors

720

Institutions

Publications per year

2017–2026

270

Authors

1.9K

  1. SM
    S. Matarrese

    University of Padua, Italy

    43 publications · 3.5K citations

    33

    h-index

  2. AR
    Antonio Riotto

    Istituto Nazionale di Fisica Nucleare, Sezione di Padova, Italy

    23 publications · 1.8K citations

    21

    h-index

  3. ML
    M. Liguori

    University of Padua, Italy

    24 publications · 1.3K citations

    21

    h-index

  4. LS
    Leonardo Senatore

    Kavli Institute for Particle Astrophysics and Cosmology, United States

    18 publications · 1.9K citations

    17

    h-index

  5. LV
    Licia Verde

    Universitat de Barcelona, Spain

    20 publications · 1.9K citations

    17

    h-index

1–5 of 1.9K

Venues

  1. Journal of Cosmology and Astroparticle Physics

    JCAP · 275 publications · 18.2K citations

    75

    h-index

  2. 57

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    147 publications · 6.4K citations

    45

    h-index

  4. The Astrophysical Journal

    ApJ · 69 publications · 5.6K citations

    39

    h-index

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

    PRD · 61 publications · 2.6K citations

    30

    h-index

1–5