Cmb Bispectrum

The CMB Bispectrum is the three-point correlation function of temperature anisotropies in the cosmic microwave background, serving as a statistical measure of non-Gaussianity that distinguishes primordial density fluctuations from those generated by linear evolution in the early universe.

1.1K

Publications

71.7K

Citations

3.5K

Authors

736

Institutions

Publications per year

2017–2026

255

Variants

Cosmic Microwave Background Bispectrum

Authors

3.5K

  1. ML
    M. Liguori

    University of Padua, Italy

    29 publications · 2.6K citations

    24

    h-index

  2. SM
    S. Matarrese

    University of Padua, Italy

    27 publications · 3.5K citations

    24

    h-index

  3. KM
    K. M. Górski

    University of Warsaw, Poland

    26 publications · 5.2K citations

    22

    h-index

  4. FR
    F. R. Bouchet

    Institut d'Astrophysique de Paris, France

    26 publications · 3.6K citations

    21

    h-index

  5. BD
    B. D. Wandelt

    Institut d'Astrophysique de Paris, France

    24 publications · 2.8K citations

    20

    h-index

1–5 of 3.5K

Venues

  1. The Astrophysical Journal

    ApJ · 138 publications · 13.3K citations

    61

    h-index

  2. 56

    h-index

  3. Journal of Cosmology and Astroparticle Physics

    JCAP · 177 publications · 8.9K citations

    55

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    171 publications · 7.9K citations

    51

    h-index

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

    PRD · 65 publications · 3.1K citations

    29

    h-index

1–5