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arxiv: 2203.06508 · v2 · pith:JO5LQRY2new · submitted 2022-03-12 · ✦ hep-ph · astro-ph.CO· hep-ex

Snowmass2021 Cosmic Frontier White Paper: Ultraheavy particle dark matter

classification ✦ hep-ph astro-ph.COhep-ex
keywords darkmatterultraheavyspacecosmiccurrentdetectorsdirect
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We outline the unique opportunities and challenges in the search for "ultraheavy" dark matter candidates with masses between roughly $10~{\rm TeV}$ and the Planck scale $m_{\rm pl} \approx 10^{16}~{\rm TeV}$. This mass range presents a wide and relatively unexplored dark matter parameter space, with a rich space of possible models and cosmic histories. We emphasize that both current detectors and new, targeted search techniques, via both direct and indirect detection, are poised to contribute to searches for ultraheavy particle dark matter in the coming decade. We highlight the need for new developments in this space, including new analyses of current and imminent direct and indirect experiments targeting ultraheavy dark matter and development of new, ultra-sensitive detector technologies like next-generation liquid noble detectors, neutrino experiments, and specialized quantum sensing techniques.

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Cited by 1 Pith paper

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  1. Too Heavy to Hide: Gamma-Ray Constraints on Annihilating Dark Matter beyond Unitarity

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    Gamma-ray upper limits from five high-energy observatories constrain the annihilation cross sections of composite dark matter in the mass range 10^5--10^12 GeV.