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arXiv · 2405.03817

Search for joint multimessenger signals from potential galactic cosmic-ray accelerators with HAWC and IceCube

R. Alfaro·C. Alvarez·J. C. Arteaga-Velázquez·D. Avila Rojas·H. A. Ayala Solares·R. Babu·E. Belmont-Moreno·K. S. Caballero-Mora·T. Capistrán·A. Carramiñana·S. Casanova·U. Cotti·J. Cotzomi·S. Coutiño de León·E. De la Fuente·D. Depaoli·N. Di Lalla·R. Diaz Hernandez·J. C. Díaz-Vélez·K. Engel·T. Ergin·K. L. Fan·K. Fang·N. Fraija·S. Fraija·J. A. García-González·F. Garfias·M. M. González·J. A. Goodman·S. Groetsch·J. P. Harding·S. Hernández-Cadena·I. Herzog·D. Huang·F. Hueyotl-Zahuantitla·P. Hüntemeyer·A. Iriarte·S. Kaufmann·J. Lee·H. León Vargas·A. L. Longinotti·G. Luis-Raya·K. Malone·J. Martínez-Castro·J. A. Matthews·P. Miranda-Romagnoli·J. A. Montes·E. Moreno·M. Mostafá·L. Nellen·N. Omodei·M. Osorio·Y. Pérez Araujo·E. G. Pérez-Pérez·C. D. Rho·D. Rosa-González·H. Salazar·D. Salazar-Gallegos·A. Sandoval·M. Schneider·J. Serna-Franco·A. J. Smith·Y. Son·O. Tibolla·K. Tollefson·I. Torres·R. Torres-Escobedo·R. Turner·F. Ureña-Mena·X. Wang·I. J. Watson·K. Whitaker·E. Willox·H. Wu·S. Yun-Cárcamo·H. Zhou·C. de León·R. Abbasi·M. Ackermann·J. Adams·S. K. Agarwalla·J. A. Aguilar·M. Ahlers·J. M. Alameddine·N. M. Amin·K. Andeen·C. Argüelles·Y. Ashida·S. Athanasiadou·L. Ausborm·S. N. Axani·X. Bai·A. Balagopal V.·M. Baricevic·S. W. Barwick·S. Bash·V. Basu·R. Bay·J. J. Beatty·J. Becker Tjus
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Abstract

The origin of high-energy galactic cosmic rays is yet to be understood, but some galactic cosmic-ray accelerators can accelerate cosmic rays up to PeV energies. The high-energy cosmic rays are expected to interact with the surrounding material or radiation, resulting in the production of gamma-rays and neutrinos. To optimize for the detection of such associated production of gamma-rays and neutrinos for a given source morphology and spectrum, a multimessenger analysis that combines gamma-rays and neutrinos is required. In this study, we use the Multi-Mission Maximum Likelihood framework with IceCube Maximum Likelihood Analysis software and HAWC Accelerated Likelihood to search for a correlation between 22 known gamma-ray sources from the third HAWC gamma-ray catalog and 14 yr of IceCube track-like data. No significant neutrino emission from the direction of the HAWC sources was found. We report the best-fit gamma-ray model and 90% CL neutrino flux limit from the 22 sources. From the neutrino flux limit, we conclude that, for five of the sources, the gamma-ray emission observed by HAWC cannot be produced purely from hadronic interactions. We report the limit for the fraction of gamma-rays produced by hadronic interactions for these five sources.

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R. Alfaro, C. Alvarez, J. C. Arteaga-Velázquez, D. Avila Rojas, H. A. Ayala Solares, R. Babu, E. Belmont-Moreno, K. S. Caballero-Mora, T. Capistrán, A. Carramiñana, S. Casanova, U. Cotti, J. Cotzomi, S. Coutiño de León, E. De la Fuente, D. Depaoli, N. Di Lalla, R. Diaz Hernandez, J. C. Díaz-Vélez, K. Engel, T. Ergin, K. L. Fan, K. Fang, N. Fraija, S. Fraija, J. A. García-González, F. Garfias, M. M. González, J. A. Goodman, S. Groetsch, J. P. Harding, S. Hernández-Cadena, I. Herzog, D. Huang, F. Hueyotl-Zahuantitla, P. Hüntemeyer, A. Iriarte, S. Kaufmann, J. Lee, H. León Vargas, A. L. Longinotti, G. Luis-Raya, K. Malone, J. Martínez-Castro, J. A. Matthews, P. Miranda-Romagnoli, J. A. Montes, E. Moreno, M. Mostafá, L. Nellen, N. Omodei, M. Osorio, Y. Pérez Araujo, E. G. Pérez-Pérez, C. D. Rho, D. Rosa-González, H. Salazar, D. Salazar-Gallegos, A. Sandoval, M. Schneider, J. Serna-Franco, A. J. Smith, Y. Son, O. Tibolla, K. Tollefson, I. Torres, R. Torres-Escobedo, R. Turner, F. Ureña-Mena, X. Wang, I. J. Watson, K. Whitaker, E. Willox, H. Wu, S. Yun-Cárcamo, H. Zhou, C. de León, R. Abbasi, M. Ackermann, J. Adams, S. K. Agarwalla, J. A. Aguilar, M. Ahlers, J. M. Alameddine, N. M. Amin, K. Andeen, C. Argüelles, Y. Ashida, S. Athanasiadou, L. Ausborm, S. N. Axani, X. Bai, A. Balagopal V., M. Baricevic, S. W. Barwick, S. Bash, V. Basu, R. Bay, J. J. Beatty, J. Becker Tjus. 2024-05-06. Search for joint multimessenger signals from potential galactic cosmic-ray accelerators with HAWC and IceCube. https://doi.org/10.3847/1538-4357%2Fad812f

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