Dark matter gamma-ray line searches toward the Galactic Center halo with H.E.S.S. I

Rinchiuso L, Moulin E, Viana A, van Eldik C, Veh J (2017)


Publication Type: Conference contribution

Publication year: 2017

Journal

Publisher: Sissa Medialab Srl

Conference Proceedings Title: Proceedings of Science

Event location: Bexco, Busan, KOR

Abstract

The presence of dark matter is nowadays widely supported by a large body of astronomical and cosmological observations. A large amount of dark matter is expected to be present in the central region of the Milky Way. Very-high-energy (>100 GeV) γ-rays can be produced in the annihilation of dark matter particles. The H.E.S.S. array of Imaging Atmospheric Cherenkov Telescopes is a powerful tools to observe the Galactic Centre trying to detect γ-rays from dark matter annihilation. A new search for a dark matter signal has been carried out on the full H.E.S.S.-I data set of 2004-2014 observations. A 2D-binned likelihood method has been applied to exploit the spectral and spatial properties of signal and background. Updated constraints are derived on the velocity-weighted annihilation cross section for signals from prompt annihilation of dark matter particles into two photons. The larger statistics from the 10-year Galactic Center dataset of H.E.S.S.-I together with the 2D-analysis technique allows to significantly improve the previous limits.

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How to cite

APA:

Rinchiuso, L., Moulin, E., Viana, A., van Eldik, C., & Veh, J. (2017). Dark matter gamma-ray line searches toward the Galactic Center halo with H.E.S.S. I. In Proceedings of Science. Bexco, Busan, KOR: Sissa Medialab Srl.

MLA:

Rinchiuso, Lucia, et al. "Dark matter gamma-ray line searches toward the Galactic Center halo with H.E.S.S. I." Proceedings of the 35th International Cosmic Ray Conference, ICRC 2017, Bexco, Busan, KOR Sissa Medialab Srl, 2017.

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