Cosmic-ray Reacceleration

Cosmic-Ray Reacceleration is a theoretical framework in astrophysics that describes the process by which previously energetic cosmic rays gain additional kinetic energy through interactions with turbulent interstellar medium or shock waves, distinguishing it from primary acceleration mechanisms by focusing on the subsequent energization of pre-existing cosmic-ray populations.

148

Publications

12.7K

Citations

324

Authors

211

Institutions

Publications per year

2017–2026

22

Authors

324

  1. EG
    E. G. Berezhko

    Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy, Russia

    7 publications · 528 citations

    7

    h-index

  2. AR
    A. R. Bell

    University of Oxford, United Kingdom

    5 publications · 543 citations

    5

    h-index

  3. KM
    Kohta Murase

    Pennsylvania State University, United States

    4 publications · 261 citations

    4

    h-index

  4. HJ
    H. J. Völk

    Max Planck Institute for Nuclear Physics, Germany

    4 publications · 275 citations

    4

    h-index

  5. VN
    V. N. Zirakashvili

    Institute of Terrestrial Magnetism Ionosphere and Radio Wave Propagation, Russia

    4 publications · 160 citations

    4

    h-index

1–5 of 324

Venues

  1. The Astrophysical Journal

    ApJ · 23 publications · 3K citations

    20

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    13 publications · 1.7K citations

    13

    h-index

  3. Advances in Space Research

    10 publications · 243 citations

    10

    h-index

  4. Astronomy and Astrophysics

    7 publications · 553 citations

    7

    h-index

  5. Nature

    7 publications · 894 citations

    7

    h-index

1–5