The Physics of Pulsar Halos: Research Progress and Prospect
arXiv:2207.04011 · doi:10.1142/S0217751X22300113
Abstract
Diffusive TeV gamma-ray emissions have been recently discovered extending beyond the pulsar wind nebulae of a few middle-aged pulsars, implying that energetic electron/positron pairs are escaping from the pulsar wind nebulae and radiating in the ambient interstellar medium. It has been suggested that these extended emissions constitute a distinct class of nonthermal sources, termed "pulsar halos". In this article, I will review the research progress on pulsar halos and discuss our current understanding on their physics, including the multiwavelength observations, different theoretical models, as well as implications for the origin of cosmic-ray positron excess and Galactic diffuse gamma-ray emission.
26 pages, 5 figures, 2 tables; invited review for International Journal of Modern Physics A
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Cited by in corpus (18)
- HAWC Detection of a TeV Halo Candidate Surrounding a Radio-quiet pulsar
- Pulsars Do Not Produce Sharp Features in the Cosmic-Ray Electron and Positron Spectra
- Ultra-High-Energy Gamma-Ray Astronomy
- Geminga's pulsar halo: an X-ray view
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- Effect of magnetic field correlation length on the gamma-ray pulsar halo morphology under anisotropic diffusion
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- Discrete treatment of inverse Compton scattering: implications on parameter estimation in gamma-ray astronomy
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