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A Contribution of the HAWC Observatory to the TeV era in the High Energy Gamma-Ray Astrophysics: The case of the TeV-Halos

by Eduardo de la Fuente, Ramiro Torres-Escobedo, Hao Zhou

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Submission summary

Authors (as registered SciPost users): Ramiro Torres-Escobedo
Submission information
Preprint Link: scipost_202208_00090v2  (pdf)
Date accepted: 2022-12-01
Date submitted: 2022-11-01 04:45
Submitted by: Torres-Escobedo, Ramiro
Submitted to: SciPost Physics Proceedings
Proceedings issue: 21st International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI2022)
Ontological classification
Academic field: Physics
Specialties:
  • Gravitation, Cosmology and Astroparticle Physics
Approach: Experimental

Abstract

We present a short overview of the TeV-Halos objects as a discovery and a relevant contribution of the High Altitude Water Cerenkov (HAWC) observatory to TeV astrophysics. We discuss history, discovery, knowledge, and the next step through a new and more detailed analysis than the original study in 2017. TeV-Halos will contribute to resolving the problem of the local positron excess observed on the Earth. To clarify the latter, understanding the diffusion process is mandatory.

Published as SciPost Phys. Proc. 13, 029 (2023)

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