Albert A, Alves S, André M, Ardid M, Ardid S, Aubert JJ, Aublin J, Baret B, Basa S, Becherini Y, Belhorma B, Benfenati F, Bertin V, Biagi S, Boumaaza J, Bouta M, Bouwhuis MC, Brânzaş H, Bruijn R, Brunner J, Busto J, Caiffi B, Calvo D, Campion S, Capone A, Carenini F, Carr J, Carretero V, Cartraud T, Celli S, Cerisy L, Chabab M, Cherkaoui El Moursli R, Chiarusi T, Circella M, Coelho JA, Coleiro A, Coniglione R, Coyle P, Creusot A, Díaz AF, De Martino B, Distefano C, Di Palma I, Donzaud C, Dornic D, Drouhin D, Eberl T, Eddymaoui A, Van Eeden T, Van Eijk D, El Hedri S, Khayati NE, Enzenhöfer A, Fermani P, Ferrara G, Filippini F, Fusco L, Gagliardini S, García-Méndez J, Gatius Oliver C, Gay P, Geißelbrecht N, Glotin H, Gozzini R, Gracia Ruiz R, Graf K, Guidi C, Haegel L, Hallmann S, Van Haren H, Heijboer AJ, Hello Y, Hennig L, Hernández-Rey JJ, Hößl J, Huang F, Illuminati G, Jisse-Jung B, De Jong M, De Jong P, Kadler M, Kalekin O, Katz U, Kouchner A, Kreykenbohm I, Kulikovskiy V, Lahmann R, Lamoureux M, Lazo A, Lefèvre D, Leonora E, Levi G, Le Stum S, Loucatos S, Manczak J, Marcelin M, Margiotta A, Marinelli A, Martínez-Mora JA, Migliozzi P, Moussa A, Muller R, Navas S, Nezri E, Ó Fearraigh B, Oukacha E, Păun AM, Păvălaş GE, Peña-Martínez S, Perrin-Terrin M, Piattelli P, Poirè C, Popa V, Pradier T, Randazzo N, Real D, Riccobene G, Romanov A, Sánchez Losa A, Saina A, Greus FS, Samtleben DF, Sanguineti M, Sapienza P, Schüssler F, Seneca J, Spurio M, Stolarczyk T, Taiuti M, Tayalati Y, Vallage B, Vannoye G, Van Elewyck V, Viola S, Vivolo D, Wilms J, Zavatarelli S, Zegarelli A, Zornoza JD, Zúñiga J, De La Torre Luque P, Gaggero D, Grasso D, Pagliaroli G, Vecchiotti V, Villante FL (2026)
Publication Type: Journal article
Publication year: 2026
Book Volume: 53
Article Number: 100565
DOI: 10.1016/j.jheap.2026.100565
The diffuse emission of γ -rays and neutrinos, produced by interactions of cosmic rays with interstellar matter in the Milky Way, provides valuable insights into cosmic ray propagation and Galactic processes. Emission models incorporating different assumptions about cosmic ray diffusion, source distribution, and target gas density are tested using data from neutrino telescopes. In this study, the final all-flavor neutrino dataset, collected over 15 years (2007-2022) by the ANTARES neutrino telescope, is analyzed. A maximum likelihood ratio method built to handle templates of Galactic emission models is employed to evaluate the compatibility of these models with the observed spatial and energy distributions of neutrino events. The results do not yield stringent constraints on the tested models and upper limits on the diffuse neutrino flux are derived, which are compatible with the results obtained by other experiments.
APA:
Albert, A., Alves, S., André, M., Ardid, M., Ardid, S., Aubert, J.J.,... Villante, F.L. (2026). Search for diffuse galactic neutrinos with the full ANTARES telescope dataset. Journal of High Energy Astrophysics, 53. https://doi.org/10.1016/j.jheap.2026.100565
MLA:
Albert, A., et al. "Search for diffuse galactic neutrinos with the full ANTARES telescope dataset." Journal of High Energy Astrophysics 53 (2026).
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