Cosmic-ray Escape

Cosmic-Ray Escape is a theoretical construct in astrophysics that denotes the process by which high-energy particles accelerated by supernova remnant shocks propagate beyond the confines of their host remnants into the interstellar medium, distinguished from other cosmic-ray transport phenomena by its specific association with the termination of diffusive shock acceleration and the onset of galactic cosmic-ray diffusion.

127

Publications

7.2K

Citations

370

Authors

197

Institutions

Publications per year

2017–2026

25

Authors

370

  1. YO
    Yutaka Ohira

    Aoyama Gakuin University, Japan

    6 publications · 520 citations

    6

    h-index

  2. KI
    Kunihito Ioka

    Kyoto University, Japan

    4 publications · 378 citations

    4

    h-index

  3. KM
    Kohta Murase

    Pennsylvania State University, United States

    4 publications · 540 citations

    4

    h-index

  4. AM
    A. M. Bykov

    Ioffe Institute, Russia

    4 publications · 341 citations

    4

    h-index

  5. AM
    Alexandre Marcowith

    Centre National de la Recherche Scientifique, France

    4 publications · 129 citations

    4

    h-index

1–5 of 370

Venues

  1. The Astrophysical Journal

    ApJ · 38 publications · 2.1K citations

    25

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    23 publications · 1.9K citations

    19

    h-index

  3. Astronomy and Astrophysics

    14 publications · 751 citations

    13

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 3 publications · 90 citations

    3

    h-index

  5. The Astrophysical Journal Letters

    3 publications · 196 citations

    3

    h-index

1–5