Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/220457
Title: Constraints on axion-like particles with the Perseus Galaxy Cluster with MAGIC
Author: Abe, H.
Abe, S.
Abhir, J.
Acciari, V.A.
Agudo, I.
Aniello, T.
Ansoldi, S.
Antonelli, L.A.
Arbet Engels, A.
Arcaro, C.
Artero, M.
Kushida, J.
Láinez Lezáun, M.
Lamastra, A.
Leone, F.
Lindfors, E.
Linhoff, L.
Lombardi, S.
Longo, F.
López-Coto, R.
López-Moya, M.
Asano, K.
López-Oramas, A.
Loporchio, S.
Lorini, A.
Machado de Oliveira Fraga, B.
Majumdar, P.
Makariev, M.
Maneva, G.
Mang, N.
Manganaro, M.
Mangano, S.
Baack, D.
Mannheim, K.
Mariotti, M.
Martínez, M.
Martínez-Chicharro, M.
Mas-Aguilar, A.
Mazin, D.
Menchiari, S.
Mender, S.
Miceli, D.
Miener, T.
Babić, A.
Miranda, J.M.
Mirzoyan, R.
Molero González, M.
Molina, Edgar
Mondal, H.A.
Moralejo, A.
Morcuende, D.
Nakamori, T.
Nanci, C.
Nava, L.
Baquero, A.
Neustroev, V.
Nickel, L.
Nievas Rosillo, M.
Nigro, C.
Nikolić, L.
Nilsson, K.
Nishijima, K.
Njoh Ekoume, T.
Noda, K.
Nozaki, S.
Barres de Almeida, U.
Ohtani, Y.
Okumura, A.
Otero-Santos, J.
Paiano, S.
Palatiello, M.
Paneque, D.
Paoletti, R.
Paredes i Poy, Josep Maria
Pavlović, D.
Persic, M.
Barrio, J.A.
Pihet, M.
Pirola, G.
Podobnik, F.
Prada Moroni, P.G.
Prandini, E.
Principe, G.
Priyadarshi, C.
Rhode, W.
Ribó Gomis, Marc
Rico, J.
Batković, I.
Righi, C.
Sahakyan, N.
Saito, T.
Satalecka, K.
Saturni, F.G.
Schleicher, B.
Schmidt, K.
Schmuckermaier, F.
Schubert, J.L.
Schweizer, T.
Baxter, J.
Sciaccaluga, A.
Sitarek, J.
Sliusar, V.
Sobczynska, D.
Spolon, A.
Stamerra, A.
Strišković, J.
Strom, D.
Strzys, M.
Suda, Y.
Becerra González, J.
Suutarinen, S.
Tajima, H.
Takahashi, M.
Takeishi, R.
Tavecchio, F.
Temnikov, P.
Terauchi, K.
Terzić, T.
Teshima, M.
Tosti, L.
Bednarek, W.
Truzzi, S.
Tutone, A.
Ubach, S.
van Scherpenberg, J.
Vazquez Acosta, M.
Ventura, S.
Verguilov, V.
Viale, I.
Vigorito, C.F.
Vitale, V.
Bernardini, E.
Vovk, I.
Walter, R.
Will, M.
Yamamoto, T.
Bernete, J.
Berti, A.
Besenrieder, J.
Bigongiari, C.
Biland, A.
Blanch, O.
Bonnoli, G.
Bošnjak, Ž.
Burelli, I.
Busetto, G.
Campoy-Ordaz, A.
Carosi, A.
Carosi, R.
Carretero-Castrillo, Mar
Castro-Tirado, A.J.
Ceribella, G.
Chai, Y.
Cifuentes, A.
Cikota, S.
Colombo, Elisabetta
Contreras, J.L.
Cortina, J.
Covino, S.
D'Amico, G.
D'Elia, V.
Da Vela, P.
Dazzi, F.
De Angelis, A.
De Lotto, B.
Del Popolo, A.
Delgado, J.
Delgado Mendez, C.
Depaoli, D.
Di Pierro, F.
Di Venere, L.
Dominis Prester, D.
Donini, A.
Dorner, D.
Doro, M.
Elsaesser, D.
Emery, G.
Escudero, J.
Fariña, L.
Fattorini, A.
Foffano, L.
Font, L.
Fukami, S.
Fukazawa, Yugo
García López, R.J.
Garczarczyk, M.
Gasparyan, S.
Gaug, M.
Giesbrecht Paiva, J.G.
Giglietto, N.
Giordano, F.
Gliwny, P.
Godinović, N.
Grau, R.
Green, D.
Green, J.G.
Hadasch, D.
Hahn, A.
Hassan, T.
Heckmann, L.
Herrera, J.
Hrupec, D.
Hütten, M.
Imazawa, R.
Inada, T.
Iotov, R.
Ishio, K.
Jiménez Martínez, I.
Jormanainen, J.
Kerszberg, D.
Kluge, G.W.
Kobayashi, Y.
Kouch, P.M.
Kubo, H.
Keywords: Raigs gamma
Telescopis
Cúmuls de galàxies
Gamma rays
Telescopes
Clusters of galaxies
Issue Date: 1-May-2024
Publisher: Elsevier B.V.
Abstract: Axion-like particles (ALPs) are pseudo-Nambu-Goldstone bosons that emerge in various theories beyond the standard model. These particles can interact with high-energy photons in external magnetic fields, influencing the observed gamma-ray spectrum. This study analyzes 41.3 h of observational data from the Perseus Galaxy Cluster collected with the MAGIC telescopes. We focused on the spectra the radio galaxy in the center of the cluster: NGC 1275. By modeling the magnetic field surrounding this target, we searched for spectral indications of ALP presence. Despite finding no statistical evidence of ALP signatures, we were able to exclude ALP models in the sub-micro electronvolt range. Our analysis improved upon previous work by calculating the full likelihood and statistical coverage for all considered models across the parameter space. Consequently, we achieved the most stringent limits to date for ALP masses around 50 neV, with cross sections down to gaγ = 3 × 10-12 GeV-1.
Note: Reproducció del document publicat a: https://doi.org/10.1016/j.dark.2024.101425
It is part of: Physics of the Dark Universe, 2024, vol. 44
URI: https://hdl.handle.net/2445/220457
Related resource: https://doi.org/10.1016/j.dark.2024.101425
ISSN: 2212-6864
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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