1.2k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Russian Academy of SciencesRU133 papers
- Lomonosov Moscow State UniversityRU72 papers
- National Research Tomsk State UniversityRU34 papers
- Institute of Solar-Terrestrial PhysicsRU32 papers
- Universitat de ValènciaES27 papers
- Troitsk Institute for Innovation and Fusion ResearchRU23 papers
- Universidade de São PauloBR21 papers
- Chinese Academy of SciencesCN20 papers
- Instituto de Física CorpuscularES19 papers
- Institute for High Energy PhysicsES18 papers
- National Astronomical ObservatoriesCN18 papers
- Kurchatov InstituteRU17 papers
4 papers · 2 filters
Non-linear diffusion of cosmic rays escaping from supernova remnants: Cold partially neutral atomic and molecular phases
L. Brahimi, A. Marcowith, V. S. Ptuskin
We aim to elucidate cosmic ray (CR) propagation in the weakly ionized environments of supernova remnants (SNRs) basing our analysis on the cosmic ray cloud (CRC) model developed by…
Generation of strong magnetic fields in old neutron stars accounting for continuous chiral magnetic effect
Maxim Dvornikov, V. B. Semikoz, D. D. Sokoloff
We suggest a new mean field dynamo model in anomalous MagnetoHydroDynamics (AMHD) accounting for the mean spin (polarization) of the magnetized chiral (ultrarelativistic) plasma of…
Permanent mean spin source of the chiral magnetic effect in neutron stars
Maxim Dvornikov, Victor B. Semikoz
We suggest the generalization of the Anomalous Magneto-Hydro-Dynamics (AMHD) in the chiral plasma of a neutron star (NS) accounting for the mean spin in the ultrarelativistic degen…
Non-linear diffusion of cosmic rays escaping from supernova remnants - II. Hot ionized media
L. Nava, S. Recchia, S. Gabici +3
We study the problem of the escape and transport of Cosmic-Rays (CR) from a source embedded in a fully ionised, hot phase of the interstellar medium (HIM). In particular, we model…