Primary Anisotropies

Primary Anisotropies is a type of cosmic microwave background temperature fluctuation that originates from acoustic and gravitational effects in the primordial plasma prior to photon decoupling, distinguishing it from secondary anisotropies that arise from later interactions during the photon propagation to the observer.

624

Publications

52.8K

Citations

9.6K

Authors

982

Institutions

Publications per year

2017–2026

96

Variants

Primordial Anisotropies

Authors

9.6K

  1. AC
    A. Challinor

    University of Cambridge, United Kingdom

    12 publications · 9.8K citations

    12

    h-index

  2. NA
    N. Aghanim

    Centre National de la Recherche Scientifique, France

    10 publications · 9.2K citations

    10

    h-index

  3. AL
    A. Lasenby

    University of Cambridge, United Kingdom

    10 publications · 7.4K citations

    10

    h-index

  4. PA
    P. A. R. Ade

    Cardiff University, United Kingdom

    10 publications · 2.9K citations

    10

    h-index

  5. SM
    S. Matarrese

    University of Padua, Italy

    9 publications · 7.8K citations

    9

    h-index

1–5 of 9.6K

Venues

  1. The Astrophysical Journal

    ApJ · 89 publications · 7.7K citations

    44

    h-index

  2. Journal of Cosmology and Astroparticle Physics

    JCAP · 31 publications · 1.6K citations

    26

    h-index

  3. 24

    h-index

  4. Journal of Geophysical Research Atmospheres

    JGR · 26 publications · 2K citations

    19

    h-index

  5. Monthly Notices of the Royal Astronomical Society

    23 publications · 1.1K citations

    19

    h-index

1–5