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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Published in | Progress of theoretical and experimental physics Vol. 2024; no. 5 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
Oxford
Oxford University Press
01.05.2024
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Subjects | |
Online Access | Get full text |
ISSN | 2050-3911 2050-3911 |
DOI | 10.1093/ptep/ptae069 |
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