Clusters of galaxies are the largest known gravitationally bound structures in the Universe, with masses around 1015 M⊙, most of it in the form of dark matter. The ground-based Imaging Atmospheric Cherenkov Telescope MAGIC made a deep survey of the Perseus cluster of galaxies using almost 400 h of data recorded between 2009 and 2017. This is the deepest observational campaign so far on a cluster of galaxies in the very high energy range. We search for gamma-ray signals from dark matter particles in the mass range between 200 GeV and 200 TeV decaying into standard model pairs. We apply an analysis optimized for the spectral and morphological features expected from dark matter decays and find no evidence of decaying dark matter. From this, we conclude that dark matter particles have a decay lifetime longer than ∼1026 s in all considered channels. Our results improve previous lower limits found by MAGIC and represent the strongest limits on decaying dark matter particles from ground-based gamma-ray instruments.

Acciari, V.A., Ansoldi, S., Antonelli, L.A., Arbet Engels, A., Arcaro, C., Baack, D., et al. (2018). Constraining dark matter lifetime with a deep gamma-ray survey of the Perseus galaxy cluster with MAGIC. PHYSICS OF THE DARK UNIVERSE, 22, 38-47 [10.1016/j.dark.2018.08.002].

Constraining dark matter lifetime with a deep gamma-ray survey of the Perseus galaxy cluster with MAGIC

Bonnoli, G.;Da Vela, P.;Martínez, M.;LO NIGRO, CRISTIANA;Ninci, D.;Paoletti, R.;Rugliancich, A.;
2018-01-01

Abstract

Clusters of galaxies are the largest known gravitationally bound structures in the Universe, with masses around 1015 M⊙, most of it in the form of dark matter. The ground-based Imaging Atmospheric Cherenkov Telescope MAGIC made a deep survey of the Perseus cluster of galaxies using almost 400 h of data recorded between 2009 and 2017. This is the deepest observational campaign so far on a cluster of galaxies in the very high energy range. We search for gamma-ray signals from dark matter particles in the mass range between 200 GeV and 200 TeV decaying into standard model pairs. We apply an analysis optimized for the spectral and morphological features expected from dark matter decays and find no evidence of decaying dark matter. From this, we conclude that dark matter particles have a decay lifetime longer than ∼1026 s in all considered channels. Our results improve previous lower limits found by MAGIC and represent the strongest limits on decaying dark matter particles from ground-based gamma-ray instruments.
2018
Acciari, V.A., Ansoldi, S., Antonelli, L.A., Arbet Engels, A., Arcaro, C., Baack, D., et al. (2018). Constraining dark matter lifetime with a deep gamma-ray survey of the Perseus galaxy cluster with MAGIC. PHYSICS OF THE DARK UNIVERSE, 22, 38-47 [10.1016/j.dark.2018.08.002].
File in questo prodotto:
File Dimensione Formato  
1-s2.0-S2212686418300621-main.pdf

non disponibili

Descrizione: Articolo su rivista
Tipologia: PDF editoriale
Licenza: NON PUBBLICO - Accesso privato/ristretto
Dimensione 1.1 MB
Formato Adobe PDF
1.1 MB Adobe PDF   Visualizza/Apri   Richiedi una copia

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11365/1064628