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A measurement of the all-particle energy spectrum of cosmic rays from 1013 to 1015eV using HAWC

Authors
Alfaro, R.Alvarez, C.Arteaga-Velázquez, J.C.Rojas, D. AvilaSolares, H.A. AyalaBelmont-Moreno, E.Bernal, A.Caballero-Mora, K.S.Capistrán, T.Carramiñana, A.Casanova, S.Cotzomi, J.de León, S. CoutiñoDe la Fuente, E.Depaoli, D.Desiati, P.Di Lalla, N.Hernandez, R. DiazDuVernois, M.A.Díaz-Vélez, J.C.Engel, K.Ergin, T.Fan, K.L.Fraija, N.García-González, J.A.Muñoz, A. GonzalezGonzález, M.M.Goodman, J.A.Harding, J.P.Hernández-Cadena, S.Herzog, I.Huang, D.Hueyotl-Zahuantitla, F.Hüntemeyer, P.Iriarte, A.Lara, A.Lee, W.H.Vargas, H. LeónLonginotti, A.L.Luis-Raya, G.Malone, K.Martinez, O.Martínez-Castro, J.Martínez-Huerta, H.Matthews, J.A.Miranda-Romagnoli, P.Morales-Soto, J.A.Moreno, E.Mostafá, M.Najafi, M.Nellen, L.Noriega-Papaqui, R.Omodei, N.Araujo, Y. PérezPérez-Pérez, E.G.Rho, C.D.Rosa-González, D.Salazar, H.Sandoval, A.Schneider, M.Serna-Franco, J.Smith, A.J.Son, Y.Springer, R.W.Tollefson, K.Torres, I.Torres-Escobedo, R.Turner, R.Ureña-Mena, F.Varela, E.Villaseñor, L.Wang, X.Watson, I.J.Wu, H.Yu, S.Zhou, H.de León, C.
Issue Date
May-2025
Publisher
Elsevier B.V.
Keywords
Cosmic-ray energy spectrum; Extensive air showers; Ground-based cosmic-ray detectors; HAWC; High-energy cosmic rays; Water Cherenkov detectors
Citation
Astroparticle Physics, v.167
Indexed
SCIE
SCOPUS
Journal Title
Astroparticle Physics
Volume
167
URI
https://scholarx.skku.edu/handle/2021.sw.skku/119943
DOI
10.1016/j.astropartphys.2024.103077
ISSN
0927-6505
1873-2852
Abstract
We report the total energy spectrum of cosmic rays in the energy interval from 10TeV to 1PeV, which lies in the energy region where both direct and indirect cosmic ray experiments overlap. The all-particle spectrum was obtained from an unfolding analysis of 5.3 years of data collected with the High Altitude Water Cherenkov (HAWC) observatory for zenith angles smaller than or equal to 35°. The study was carried out in the framework of the QGSJET-II-04 hadronic interaction model. The measured spectrum confirms the presence of a knee-like feature at tens of TeV. In our analysis, the position of this softening is found at 40.2±1.0(stat.)−6.4+6.2(sys.)TeV. The measured spectral indices before and after the break are γ1=−2.53±0.01(stat.)−0.05+0.04(sys.) and γ2=−2.71±0.01(stat.)−0.04+0.03(sys.), respectively. © 2024 Elsevier B.V.
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