Dark matter line searches with the Cherenkov Telescope Array

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dc.contributor.authorAbe, S.
dc.contributor.authorAbhir, J.
dc.contributor.authorAbhishek, A.
dc.contributor.authorAcero, F.
dc.contributor.authorAcharyya, A.
dc.contributor.authorAdam, R.
dc.contributor.authorAguasca-Cabot, A.
dc.contributor.authorAgudo, I.
dc.contributor.authorAguirre-Santaella, A.
dc.contributor.authorAlfaro, J.
dc.contributor.authorAlfaro, R.
dc.contributor.authorAlvarez-Crespo, N.
dc.contributor.authorAlves Batista, R.
dc.contributor.authorAmans, J. -P.
dc.contributor.authorAmato, E.
dc.contributor.authorAmbrosi, G.
dc.contributor.authorAngel, L.
dc.contributor.authorAramo, C.
dc.contributor.authorArcaro, C.
dc.contributor.authorArnesen, T. T. H.
dc.contributor.authorArrabito, L.
dc.contributor.authorAsano, K.
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dc.contributor.authorBackes, M.
dc.contributor.authorBaktash, A.
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dc.contributor.authorBalbo, M.
dc.contributor.authorBaquero Larriva, A.
dc.contributor.authorMartins, V. Barbosa
dc.contributor.authorBarres de Almeida, U.
dc.contributor.authorBarrio, J. A.
dc.contributor.authorBatkovic, I.
dc.contributor.authorBatzofin, R.
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dc.contributor.authorBenbow, W.
dc.contributor.authorBerge, D.
dc.contributor.authorBernardini, E.
dc.contributor.authorBernete, J.
dc.contributor.authorBernloehr, K.
dc.contributor.authorBerti, A.
dc.contributor.authorBertucci, B.
dc.contributor.authorBhattacharjee, P.
dc.contributor.authorBhattacharyya, S.
dc.contributor.authorBigongiari, C.
dc.contributor.authorBiland, A.
dc.contributor.authorBissaldi, E.
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dc.contributor.authorBocchino, F.
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dc.contributor.authorBosnjak, Z.
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dc.contributor.authorBringmann, T.
dc.contributor.authorBronzini, E.
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dc.contributor.authorBulgarelli, A.
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dc.contributor.authorBurmistrov, L.
dc.contributor.authorBurton, M.
dc.contributor.authorBuscemi, M.
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dc.contributor.authorCailleux, J.
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dc.contributor.authorCapasso, G.
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dc.contributor.authorCapuzzo-Dolcetta, R.
dc.contributor.authorCaraveo, P.
dc.contributor.authorCaroff, S.
dc.contributor.authorCarosi, A.
dc.contributor.authorCarosi, R.
dc.contributor.authorCarquin, E.
dc.contributor.authorCarrasco, M. -S.
dc.contributor.authorCassol, F.
dc.contributor.authorCastaldini, L.
dc.contributor.authorCastrejon, N.
dc.contributor.authorCastro-Tirado, A. J.
dc.contributor.authorCerasole, D.
dc.contributor.authorCerruti, M.
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dc.contributor.authorChaty, S.
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dc.contributor.authorDai, S.
dc.contributor.authorDalchenko, M.
dc.contributor.authorDazzi, F.
dc.contributor.authorDe Angelis, A.
dc.contributor.authorde Lavergne, M. de Bony
dc.contributor.authorDe Caprio, V.
dc.contributor.authorde Gouveia Dal Pino, E. M.
dc.contributor.authorDe Lotto, B.
dc.contributor.authorDe Lucia, M.
dc.contributor.authorde Menezes, R.
dc.contributor.authorde Naurois, M.
dc.contributor.authorde Souza, V.
dc.contributor.authordel Peral, L.
dc.contributor.authordel Valle, M. V.
dc.contributor.authorDelgado Giler, A. G.
dc.contributor.authorDelgado Mengual, J.
dc.contributor.authorDelgado, C.
dc.contributor.authorDell'aiera, M.
dc.contributor.authordella Volpe, D.
dc.contributor.authorDepaoli, D.
dc.contributor.authorDi Girolamo, T.
dc.contributor.authorDi Piano, A.
dc.contributor.authorDi Pierro, F.
dc.contributor.authorDi Tria, R.
dc.contributor.authorDi Venere, L.
dc.contributor.authorDiaz, C.
dc.contributor.authorDiebold, S.
dc.contributor.authorDinesh, A.
dc.contributor.authorDjuvsland, J.
dc.contributor.authorDominik, R. M.
dc.contributor.authorPrester, D. Dominis
dc.contributor.authorDonini, A.
dc.contributor.authorDorner, D.
dc.contributor.authorDoerner, J.
dc.contributor.authorDoro, M.
dc.contributor.authorDournaux, J. -L.
dc.contributor.authorDuangchan, C.
dc.contributor.authorDubos, C.
dc.contributor.authorDucci, L.
dc.contributor.authorDwarkadas, V. V.
dc.contributor.authorEbr, J.
dc.contributor.authorEckner, C.
dc.contributor.authorEgberts, K.
dc.contributor.authorEinecke, S.
dc.contributor.authorElsaesser, D.
dc.contributor.authorEmery, G.
dc.contributor.authorErrando, M.
dc.contributor.authorEscanuela, C.
dc.contributor.authorEscarate, P.
dc.contributor.authorGodoy, M. Escobar
dc.contributor.authorEscudero, J.
dc.contributor.authorEsposito, P.
dc.contributor.authorEttori, S.
dc.contributor.authorFalceta-Goncalves, D.
dc.contributor.authorFedorova, E.
dc.contributor.authorFegan, S.
dc.contributor.authorFeng, Q.
dc.contributor.authorFerrand, G.
dc.contributor.authorFerrarotto, F.
dc.contributor.authorFiandrini, E.
dc.contributor.authorFiasson, A.
dc.contributor.authorFilipovic, M.
dc.contributor.authorFioretti, V.
dc.contributor.authorFiori, M.
dc.contributor.authorFoffano, L.
dc.contributor.authorFont Guiteras, L.
dc.contributor.authorFontaine, G.
dc.contributor.authorFroese, S.
dc.contributor.authorFukazawa, Y.
dc.contributor.authorFukui, Y.
dc.contributor.authorFurniss, A.
dc.contributor.authorGalanti, G.
dc.contributor.authorGalaz, G.
dc.contributor.authorGalelli, C.
dc.contributor.authorGallozzi, S.
dc.contributor.authorGammaldi, V.
dc.contributor.authorGarczarczyk, M.
dc.contributor.authorGasbarra, C.
dc.contributor.authorGasparrini, D.
dc.contributor.authorGhalumyan, A.
dc.contributor.authorGianotti, F.
dc.contributor.authorGiarrusso, M.
dc.contributor.authorGiesbrecht Formiga Paiva, J. G.
dc.contributor.authorGiglietto, N.
dc.contributor.authorGiordano, F.
dc.contributor.authorGiuffrida, R.
dc.contributor.authorGlicenstein, J. -F.
dc.contributor.authorGlombitza, J.
dc.contributor.authorGoldoni, P.
dc.contributor.authorGonzalez, J. M.
dc.contributor.authorGonzalez, M. M.
dc.contributor.authorGoulart Coelho, J.
dc.contributor.authorGradetzke, T.
dc.contributor.authorGranot, J.
dc.contributor.authorGrasso, D.
dc.contributor.authorGrau, R.
dc.contributor.authorGreaux, L.
dc.contributor.authorGreen, D.
dc.contributor.authorGreen, J. G.
dc.contributor.authorGrolleron, G.
dc.contributor.authorGuedes, L. M. V.
dc.contributor.authorGueta, O.
dc.contributor.authorHackfeld, J.
dc.contributor.authorHadasch, D.
dc.contributor.authorHamal, P.
dc.contributor.authorHanlon, W.
dc.contributor.authorHara, S.
dc.contributor.authorHarvey, V. M.
dc.contributor.authorHassan, T.
dc.contributor.authorHayashi, K.
dc.contributor.authorHess, B.
dc.contributor.authorHeckmann, L.
dc.contributor.authorHeller, M.
dc.contributor.authorHernandez Cadena, S.
dc.contributor.authorHervet, O.
dc.contributor.authorHinton, J.
dc.contributor.authorHiroshima, N.
dc.contributor.authorHnatyk, B.
dc.contributor.authorHnatyk, R.
dc.contributor.authorHofmann, W.
dc.contributor.authorHolder, J.
dc.contributor.authorHoran, D.
dc.contributor.authorHorvath, P.
dc.contributor.authorHovatta, T.
dc.contributor.authorHrabovsky, M.
dc.contributor.authorHrupec, D.
dc.contributor.authorIarlori, M.
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dc.contributor.authorInoue, S.
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dc.contributor.authorJankowsky, F.
dc.contributor.authorJean, P.
dc.contributor.authorJimenez Quiles, J.
dc.contributor.authorJin, W.
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dc.contributor.authorKagaya, M.
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dc.contributor.authorYoshida, T.
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dc.date.accessioned2025-01-20T16:05:28Z
dc.date.available2025-01-20T16:05:28Z
dc.date.issued2024
dc.description.abstractMonochromatic gamma-ray signals constitute a potential smoking gun signature for annihilating or decaying dark matter particles that could relatively easily be distinguished from astrophysical or instrumental backgrounds. We provide an updated assessment of the sensitivity of the Cherenkov Telescope Array (CTA) to such signals, based on observations of the Galactic centre region as well as of selected dwarf spheroidal galaxies. We find that current limits and detection prospects for dark matter masses above 300 GeV will be significantly improved, by up to an order of magnitude in the multi-TeV range. This demonstrates that CTA will set a new standard for gamma-ray astronomy also in this respect, as the world's largest and most sensitive high-energy gamma-ray observatory, in particular due to its exquisite energy resolution at TeV energies and the adopted observational strategy focussing on regions with large dark matter densities. Throughout our analysis, we use up-to-date instrument response functions, and we thoroughly model the effect of instrumental systematic uncertainties in our statistical treatment. We further present results for other potential signatures with sharp spectral features, e.g. box-shaped spectra, that would likewise very clearly point to a particle dark matter origin.
dc.fuente.origenWOS
dc.identifier.doi10.1088/1475-7516/2024/07/047
dc.identifier.issn1475-7516
dc.identifier.urihttps://doi.org/10.1088/1475-7516/2024/07/047
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/89898
dc.identifier.wosidWOS:001287348500001
dc.issue.numero7
dc.language.isoen
dc.revistaJournal of cosmology and astroparticle physics
dc.rightsacceso restringido
dc.subjectdark matter experiments
dc.subjectdark matter theory
dc.subjectgamma ray experiments
dc.titleDark matter line searches with the Cherenkov Telescope Array
dc.typeartículo
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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