학술논문

A Contribution of the HAWC Observatory to the TeV era in the High Energy Gamma-Ray Astrophysics: The case of the TeV-Halos
Document Type
Working Paper
Author
Torres-Escobedo, RamiroZhou, Haode la Fuente, EduardoAbeysekara, A. U.Albert, A.Alfaro, R.Alvarez, C.Álvarez, J. D.Camacho, J. R. AngelesArteaga-Velázquez, J. C.Arunbabu, K. P.Rojas, D. AvilaSolares, H. A. AyalaBabu, R.Baghmanyan, V.Barber, A. S.Gonzalez, J. BecerraBelmont-Moreno, E.BenZvi, S. Y.Berley, D.Brisbois, C.Caballero-Mora, K. S.Capistrán, T.Carramiñana, A.Casanova, S.Chaparro-Amaro, O.Cotti, U.Cotzomi, J.de León, S. Coutiñode León, C.Diaz-Cruz, L.Hernandez, R. DiazDíaz-Vélez, J. C.Dingus, B. L.Durocher, M.DuVernois, M. A.Ellsworth, R. W.Engel, K.Espinoza, C.Fan, K. L.Fang, K.Alonso, M. FernándezFick, B.Fleischhack, H.Flores, J. L.Fraija, N. I.Garcia, D.García-González, J. A.García-Torales, G.Garfias, F.Giacinti, G.Goksu, H.González, M. M.Goodman, J. A.Harding, J. P.Hernandez, S.Herzog, I.Hinton, J.Hona, B.Huang, D.Hueyotl-Zahuantitla, F.Hui, C. M.Humensky, B.Hüntemeyer, P.Iriarte, A.Jardin-Blicq, A.Jhee, H.Joshi, V.Kieda, D.Kunde, G J.Kunwar, S.Lara, A.Lee, J.Lee, W. H.Lennarz, D.Vargas, H. LeónLinnemann, J.Longinotti, A. L.López-Coto, R.Luis-Raya, G.Lundeen, J.Malone, K.Marandon, V.Martinez, O.Martinez-Castellanos, I.Martínez-Huerta, H.Martínez-Castro, J.Matthews, J. A. J.McEnery, J.Miranda-Romagnoli, P.Morales-Soto, J. A.Moreno, E.Mostafá, M.Nayerhoda, A.Nellen, L.Newbold, M.Nisa, M. U.Noriega-Papaqui, R.Olivera-Nieto, L.Omodei, N.Peisker, A.Araujo, Y. PérezPérez-Pérez, E. G.Rho, C. D.Rivière, C.Rosa-Gonzalez, D.Ruiz-Velasco, E.Ryan, J.Salazar, H.Greus, F. SalesaSandoval, A.Schneider, M.Schoorlemmer, H.Serna-Franco, J.Sinnis, G.Smith, A. J.Springer, R. W.Surajbali, P.Taboada, I.Tanner, M.Tollefson, K.Torres, I.Turner, R.Ureña-Mena, F.Villaseñor, L.Wang, X.Watson, I. J.Weisgarber, T.Werner, F.Willox, E.Wood, J.Yodh, G. B.Zepeda, A.
Source
Subject
Astrophysics - High Energy Astrophysical Phenomena
Language
Abstract
We present a short overview of the TeV-Halos objects as a discovery and a relevant contribution of the High Altitude Water \v{C}erenkov (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.
Comment: Work presented in the 21st International Symposium on Very High Energy Cosmic Ray Interactions(ISVHECRI 2022) as part of the Ph. D. Thesis of Ramiro Torres-Escobedo (SJTU, Shanghai, China). Accepted for publication in SciPost Physics Proceedings (ISSN 2666-4003). 11 pages, 3 Figures. Short overview of HAWC and TeV Halos objects until 2022