Mirages and Large TeV Halo-Pulsar Offsets from Cosmic Ray Propagation

Fuente: arXiv
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Auteurs principaux: Bao, Yiwei, Giacinti, Gwenael, Liu, Ruo-Yu, Zhang, Hai-Ming, Chen, Yang
Format: Preprint
Publié: 2024
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author Bao, Yiwei
Giacinti, Gwenael
Liu, Ruo-Yu
Zhang, Hai-Ming
Chen, Yang
author_facet Bao, Yiwei
Giacinti, Gwenael
Liu, Ruo-Yu
Zhang, Hai-Ming
Chen, Yang
contents The study of extended $γ$-ray sources usually assumes symmetric diffusion of cosmic rays. However, recent observations of multiple sources near single pulsars and significant offsets between TeV halo centroids and their parent pulsars suggest that this assumption is overly simplistic. In this Letter, we demonstrate that asymmetric propagation of cosmic rays near their accelerators may create multiple TeV sources instead of a single symmetric source. This mechanism also explains the large offsets between TeV halo centroids and their pulsars. We demonstrate that several perplexing detected sources can be naturally explained without invoking additional invisible accelerators.
format Preprint
id arxiv_https___arxiv_org_abs_2407_02478
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Mirages and Large TeV Halo-Pulsar Offsets from Cosmic Ray Propagation
Bao, Yiwei
Giacinti, Gwenael
Liu, Ruo-Yu
Zhang, Hai-Ming
Chen, Yang
High Energy Astrophysical Phenomena
The study of extended $γ$-ray sources usually assumes symmetric diffusion of cosmic rays. However, recent observations of multiple sources near single pulsars and significant offsets between TeV halo centroids and their parent pulsars suggest that this assumption is overly simplistic. In this Letter, we demonstrate that asymmetric propagation of cosmic rays near their accelerators may create multiple TeV sources instead of a single symmetric source. This mechanism also explains the large offsets between TeV halo centroids and their pulsars. We demonstrate that several perplexing detected sources can be naturally explained without invoking additional invisible accelerators.
title Mirages and Large TeV Halo-Pulsar Offsets from Cosmic Ray Propagation
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2407.02478