Cmb Trispectrum

The CMB trispectrum is a statistical measure in cosmology that quantifies the four-point correlation function of temperature anisotropies in the cosmic microwave background, extending the power spectrum and bispectrum to capture non-Gaussian features arising from primordial fluctuations or late-time physics.

519

Publications

30.7K

Citations

2.2K

Authors

538

Institutions

Publications per year

2017–2026

126

Variants

Cosmic Microwave Background Trispectrum

Authors

2.2K

  1. ML
    M. Liguori

    University of Padua, Italy

    18 publications · 1.6K citations

    17

    h-index

  2. EH
    E. Hivon

    California Institute of Technology, United States

    18 publications · 2.3K citations

    16

    h-index

  3. FR
    F. R. Bouchet

    Institut d'Astrophysique de Paris, France

    18 publications · 2K citations

    15

    h-index

  4. MS
    Maresuke Shiraishi

    The University of Tokyo, Japan

    15 publications · 628 citations

    15

    h-index

  5. JE
    J. E. Ruhl

    Case Western Reserve University, United States

    17 publications · 2.1K citations

    14

    h-index

1–5 of 2.2K

Venues

  1. 37

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    62 publications · 3.2K citations

    32

    h-index

  3. Journal of Cosmology and Astroparticle Physics

    JCAP · 74 publications · 3.1K citations

    32

    h-index

  4. The Astrophysical Journal

    ApJ · 37 publications · 3K citations

    24

    h-index

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

    PRD · 29 publications · 1.2K citations

    20

    h-index

1–5