A Self-Regulated Stochastic Acceleration Model of Pulsar Wind Nebulae

Pulsar wind nebulae (PWNe) are clouds of magnetized relativistic electron/positron plasma supplied from the central pulsar. However, the number of radio-emitting particles inside a PWN is larger than the expectation from the study of pulsar magnetospheres and their origin is still unclear. A stochas...

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Bibliographic Details
Published inProgress of theoretical and experimental physics Vol. 2024; no. 5
Main Authors Tanaka, Shuta J, Ishizaki, Wataru
Format Journal Article
LanguageEnglish
Published Oxford Oxford University Press 01.05.2024
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ISSN2050-3911
2050-3911
DOI10.1093/ptep/ptae069

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