Semantic Scholar Open Access 2022 7 sitasi

The Physics of Pulsar Halos: Research Progress and Prospect

Ruo-Yu Liu

Abstrak

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.

Topik & Kata Kunci

Penulis (1)

R

Ruo-Yu Liu

Format Sitasi

Liu, R. (2022). The Physics of Pulsar Halos: Research Progress and Prospect. https://doi.org/10.1142/S0217751X22300113

Akses Cepat

Lihat di Sumber doi.org/10.1142/S0217751X22300113
Informasi Jurnal
Tahun Terbit
2022
Bahasa
en
Total Sitasi
Sumber Database
Semantic Scholar
DOI
10.1142/S0217751X22300113
Akses
Open Access ✓