Test of the superdiffusion model in the interstellar medium around the Geminga pulsar
Author:
Funder
National Key Program for Research and Development
National Natural Science Foundation of China
Publisher
American Physical Society (APS)
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.103.063035/fulltext
Reference38 articles.
1. Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth
2. Evidences of low-diffusion bubbles around Galactic pulsars
3. Halo fraction in TeV-bright pulsar wind nebulae
4. The Evolution and Structure of Pulsar Wind Nebulae
5. Possible origin of the slow-diffusion region around Geminga
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1. Interpretation of Fluxes of Cosmic-Ray Nuclei and Electrons within a Nonclassical Diffusion Model;Bulletin of the Russian Academy of Sciences: Physics;2023-07
2. Gamma-ray pulsar halos in the Galaxy;Frontiers in Astronomy and Space Sciences;2022-10-03
3. Geminga contribution to the cosmic-ray positron excess according to the gamma-ray observations;Communications in Theoretical Physics;2022-09-26
4. Evidence of TeV halos around millisecond pulsars;Physical Review D;2022-05-16
5. Interpretation of the puzzling gamma-ray spectrum of the Geminga halo;Physical Review D;2022-05-06
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