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A next-generation ground-based wide field-of-view gamma-ray observatory in the southern hemisphere

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arxiv 1908.08858 v1 pith:OVYU32RC submitted 2019-08-23 astro-ph.HE astro-ph.IM

classification astro-ph.HEastro-ph.IM
keywords gamma-rayobservatorywillhemispheresouthernfield-of-viewnext-generationrealise
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The very-high-energy gamma-ray sky can be surveyed on a daily basis by particle-detector arrays at high (mountain) elevation. In the northern hemisphere the survey recently conducted by the HAWC gamma-ray observatory significantly enriched our knowledge about TeV gamma-ray sources. In this contribution, we will present an overview on the effort to realise a next-generation gamma-ray survey observatory in the southern hemisphere. We will discuss the unique science case for this observatory and how it will be embedded in the multi-messenger and multi-wavelength census of the non-thermal universe. In addition, we will introduce the newly founded international organisation that aims to realise this facility: The Southern Wide field-of-View Gamma-ray Observatory (SWGO) collaboration.

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    hep-ph 2024-12 conditional novelty 6.0 of 10

    An anomaly-free two-component secluded WIMP model with a dark photon, dark Higgs, and scotogenic Dirac neutrino masses can account for the observed relic density while evading cosmological bounds.

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