Possible Interpretations of the Joint Observations of UHECR Arrival Directions Using Data Recorded at the Telescope Array and the Pierre Auger Observatory
M. Kuznetsov, Adila Abdul Halim,Pedro Abreu, M. Aglietta, I. Allekotte,Kévin Almeida Cheminant,Alejandro Almela, Roberto Aloisio, J. Álvarez-Muñiz,Juan Ammerman Yebra,Gioacchino Alex Anastasi, Luis A. Anchordoqui,Belén Andrada, S. Andringa, C. Aramo,Paulo Ricardo Araújo Ferreira, Enrico Arnone,Juan Carlos Arteaga Velázquez, H. Asorey, P. Assis, G. Ávila,Emanuele Avocone,Alina Mihaela Badescu,Alena Bakalová,Alexandru Bălăceanu,Felicia Barbato,Adriel Bartz Mocellin,Jose A. Bellido, C. Bérat, M. Bertaina,Gopal Bhatta,Marta Bianciotto, Peter L. Biermann,Virginia Binet,Kathrin Bismark,Teresa Bister,Jonathan Biteau, Jiří Blažek, C. Bleve, J. Blümer, M. Bohã̌cov́a,Denise Boncioli, C. Bonifazi,Luan Bonneau Arbeletche,Nataliia Borodai,Jeffrey Brack,P. Gabriel Brichetto Orchera,Florian Lukas Briechle, A. Bueno, S. Buitink,Mario Buscemi,Max Büsken,Anthony Bwembya, K. S. Caballero‐Mora,S. Cabana-Freire,Lorenzo Caccianiga,Ioana Caracas, R. Caruso, A. Castellina,Fernando Catalani, G. Cataldi,Lorenzo Cazon,Marcos Cerda,A. Cermenati, Jose Chinellato, J. Chudoba, Ladislav Chytka, R. W. Clay,Agustín Cobos Cerutti,Roberta Colalillo, Alan Coleman,Maria Rita Coluccia, R. Conceição,Antonio Condorelli, G. Consolati, Matteo Conte,Fabio Convenga,Diego Correia dos Santos,Pedro J. Costa, C. E. Covault, M. Cristinziani,Carlo Salvattore Cruz Sanchez, S. Dasso, K. Daumiller, B. R. Dawson, Rogério M. de Almeida,Joaquin de Jesus, Sijbrand J. de Jong,João de Mello Neto, I. De Mitri,Jaime de Oliveira, D. Franco, F. de Palma, Vítor de Souza,Emanuele De Vito, A. Del Popolo, Olivier Deligny,N. Denner,Luca Deval,Armando di Matteo,Madalina Dobre, C. Dobrigkeit, Juan Carlos D’Olivo,Luis Miguel Domingues Mendes,Joao dos Anjos,Rita Cassia dos Anjos, Jan Ebr, Fiona H. Ellwanger, Mohamed Emam, R. Engel, Italo Epicoco, Martin Erdmann, A. Etchegoyen, Carmelo Evoli, H. Falcke, John Farmer, Glennys R. Farrar, A. C. Fauth, N. Fazzini,Fridtjof Feldbusch, Francesco Fenu, Alexandra Fernandes, B. 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openalex（2023）
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摘要
Various hints for anisotropies in the distribution of arrival directions of ultra-high-energy cosmic rays (UHECRs) have been reported.Still, our poor knowledge about intergalactic and Galactic magnetic fields and about the UHECR mass composition makes it non-trivial to interpret such results in terms of possible models of UHECR sources.In this work, we apply the same analyses that have been performed on the Pierre Auger Observatory and the Telescope Array UHECR data to a variety of Monte Carlo simulations generated according to many different combinations of hypotheses about the sources, composition and magnetic deflections of UHECRs.We find that only some of these models can yield results similar to those obtained with the real data.
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