Diffuse Neutrino Backgrounds

Diffuse Neutrino Backgrounds is a theoretical astrophysical phenomenon consisting of a pervasive, isotropic flux of neutrinos originating from numerous unresolved cosmic sources across the universe, distinguished from discrete neutrino signals by its lack of directional association with specific astrophysical objects.

147

Publications

8.2K

Citations

3.4K

Authors

423

Institutions

Publications per year

2017–2026

68

Variants

Diffuse Neutrino Background

Authors

3.4K

  1. TM
    T. Montaruli

    University of Wisconsin–Madison, United States

    14 publications · 1.3K citations

    13

    h-index

  2. SY
    S. Yoshida

    University of Maryland, College Park, United States

    12 publications · 1.1K citations

    12

    h-index

  3. MA
    M. Ahlers

    RWTH Aachen University, Germany

    11 publications · 1.2K citations

    11

    h-index

  4. SS
    S. Seunarine

    RWTH Aachen University, Germany

    11 publications · 1.2K citations

    11

    h-index

  5. WR
    W. Rhode

    TU Dortmund University, Germany

    11 publications · 1.1K citations

    11

    h-index

1–5 of 3.4K

Venues

  1. 20

    h-index

  2. Journal of Cosmology and Astroparticle Physics

    JCAP · 26 publications · 1K citations

    20

    h-index

  3. Physical review. D/Physical review. D.

    PRD · 22 publications · 875 citations

    16

    h-index

  4. The Astrophysical Journal

    ApJ · 13 publications · 838 citations

    12

    h-index

  5. Astroparticle Physics

    12 publications · 641 citations

    12

    h-index

1–5