Probing the mass composition of TeV cosmic rays with HAWC

In this contribution, we have investigated the energy spectra of the elemental mass groups of cosmic rays for the Light (H+He), medium (C+O) and heavy (Ne-Fe) components using the High Altitude Water Cherenkov Gamma-Ray observatory (HAWC). The study was carried out in the energy interval from $10$ TeV to $1$ PeV using almost $5$ years of data on hadronic air showers. The energy spectra were unfolded using the bidimensional distribution of the lateral shower age versus the reconstructed primary energy. We have employed the QGSJET-II-04 high-energy hadronic interaction model for the current analysis. The results show the presence of fine structure in the spectra of the light, medium and heavy mass groups of cosmic rays.

Authors

Publication Details

Published
2025-09-23
DOI
https://doi.org/10.22323/1.501.0178
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
0.00

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Probing the mass composition of TeV cosmic rays with HAWC

Miguel Araya, E. Belmont‐Moreno, S. Coutinõ de León, J. A. Morales-Soto et al.
Astrophysics and Cosmic Phenomena
article

Probing the mass composition of TeV cosmic rays with HAWC

Miguel Araya, E. Belmont‐Moreno, S. Coutinõ de León, J. A. Morales-Soto, Enrique Varela, P. Desiati, D. Salazar-Gallegos, T. Capistrán, Y. Pérez Araujo, Keith Leavitt, R. Torres-Escobedo, P. Miranda-Romagnoli, E. De la Fuente, I. Herzog, M. Roth, J. C. Díaz–Vélez, K. Malone, L. Nellen, José Erandi Serna-Franco, J. A. Goodman, S. Casanova, O. Tibolla, J. Martínez-Castro, Y. Son, G. Luis-Raya, A. Sandoval, N. Fraija, E. G. Pérez‐Pérez, G. Schwefer, Rhiannon M. Turner, N. Di Lalla, H. Salazar, D. Kieda, C. Espinoza, K. S. Caballero‐Mora, R. W. Springer, Chang Dong Rho, A. Iriarte, F. Garfias, D. Rosa‐González, P. Bangale, A. L. Longinotti, M. A. DuVernois, A. Carramiñana, T. Ergin, B.L. Dingus, E. Ponce, J. P. Harding, Sergio Hernández Cadena, J. Gyeong, A.J. Smith, M. Mostafá, J. A. García-González, J. Matthews, M. M. González, K. Engel, Kwok Lung Fan, Davide Depaoli, H. A. Ayala Solares, S. Yun-Cárcamo, P. E. Mirón-Enriquez, S. Fraija, Lingling Wang, L. Villaseñor, M. Najafi, M. Schneider, A. Gonzalez Muñoz, D. Avila Rojas, I. J. Watson, M. U. Nisa, F. Carreón, S. Kaufmann, H. León Vargas, H. Martínez-Huerta, K. Tollefson, I. Torres, R. Alfaro, J. C. Arteaga‐Velázquez, S. Yu, H. Wu, C. Alvarez, Q. Remy, N. Omodei, H. Zhou, R. Babu, D. Huang, Z. M. Wang, S. Groetsch, O. Martinez, Ana de Andrés, Juan Carlos Arteaga Velázquez, J. A. Rodríguez Montes, Nandita Ghosh, A. Bernal, J.T. Linnemann, P. Hüntemeyer, R. Díaz Hernández, E. Anita-Rangel
article en

Abstract

In this contribution, we have investigated the energy spectra of the elemental mass groups of cosmic rays for the Light (H+He), medium (C+O) and heavy (Ne-Fe) components using the High Altitude Water Cherenkov Gamma-Ray observatory (HAWC). The study was carried out in the energy interval from $10$ TeV to $1$ PeV using almost $5$ years of data on hadronic air showers. The energy spectra were unfolded using the bidimensional distribution of the lateral shower age versus the reconstructed primary energy. We have employed the QGSJET-II-04 high-energy hadronic interaction model for the current analysis. The results show the presence of fine structure in the spectra of the light, medium and heavy mass groups of cosmic rays.

National Science Foundation, U.S. Department of Energy, National Aeronautics and Space Administration, European Commission, National Research Foundation, Consejo Nacional de Ciencia y Tecnología, National Research Foundation of Korea, Benemérita Universidad Autónoma de Puebla, Office of National Higher Education Science Research and Innovation Policy Council, Goddard Space Flight Center, Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México, Coordinación de la Investigación Científica, Institute for Cosmic Ray Research, University of Tokyo, Laboratory Directed Research and Development, Los Alamos National Laboratory
Openalex Percentile: Top 89%
Astrophysics and Cosmic Phenomena
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.