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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 |
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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) |
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Academic field: | Physics |
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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)