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Perseus – A Huge Reservoir of Dark Matter investigated with MAGIC

Published online by Cambridge University Press:  07 April 2020

Michele Doro Open the ORCID record for Michele Doro [Opens in a new window] ,
Joaquim Palacio ,
Javier Rico  and
Monica Vazquez Acosta
Michele Doro
Affiliation:
Department of Physics and Astronomy, University of Padova, I-35131 Padova, Italy email: [email protected] Istituto Nazionale Fisica Nucleare sez. Padova, I-35131 Padova, Italy
Joaquim Palacio
Affiliation:
Institut de Fìsica dAltes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), E-08193 Bellaterra (Barcelona), Spain
Javier Rico
Affiliation:
Institut de Fìsica dAltes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), E-08193 Bellaterra (Barcelona), Spain
Monica Vazquez Acosta
Affiliation:
Inst. de Astrofìsica de Canarias, E-38200 La Laguna, and Universidad de La Laguna, Dpto. Astrofìsica, E-38206 La Laguna, Tenerife, Spain
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Abstract

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Galaxy clusters are excellent targets for high energy astrophysics with gamma rays. Not only they may host active galaxies, but they are often expected to provide signatures of accelerations of electrons and protons to PeV energies. Furthermore, according to ΛCDM scenario, they should be embedded in an extremely massive dark matter halo, the largest halo expected. In this report, we summarize the recently published MAGIC lower limits on the decaying dark matter lifetime using 202 h of selected high quality data taken on the Perseus galaxy cluster, in a 5-year long campaign.

Keywords

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Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S342: Perseus in Sicily: From Black Hole to Cluster Outskirts , May 2018 , pp. 141 - 144
Copyright
© International Astronomical Union 2020

References

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