Particle Physics and Cosmology with H.E.S.S.

Abstract : Gamma-ray astronomy is a powerful mean of studying particle physics and cosmology independently of particle colliders and more conventional observatories. In a 50 GeV-50 TeV range, observations of Galactic and extragalactic high-energy sources allow to efficiently search for new particles such as dark matter particles and axions; they probe the UV to infrared backgrounds of the universe whose energy density is linked to star formation and evolution of structures; and they permit to test Lorentz invariance up to the Planck scale. This report focues on some recent results in these matters obtained with the H.E.S.S. array of Cherenkov telescopes.
Type de document :
Communication dans un congrès
10th Cosmic Ray International Seminar, Jul 2016, Ischia, Italy. Nucl.Part.Phys.Proc., 291-293, pp.25-29, 2017, 〈10.1016/j.nuclphysbps.2017.06.006〉
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https://hal.archives-ouvertes.fr/hal-01669633
Contributeur : Inspire Hep <>
Soumis le : mercredi 20 décembre 2017 - 23:48:01
Dernière modification le : jeudi 15 mars 2018 - 15:05:20

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Pierre Brun. Particle Physics and Cosmology with H.E.S.S.. 10th Cosmic Ray International Seminar, Jul 2016, Ischia, Italy. Nucl.Part.Phys.Proc., 291-293, pp.25-29, 2017, 〈10.1016/j.nuclphysbps.2017.06.006〉. 〈hal-01669633〉

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