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Searching for Heavy Dark Matter near the Planck Mass with XENON1T
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).ORCID iD: 0000-0001-9984-4411
Stockholm University, Faculty of Science, Department of Physics.ORCID iD: 0000-0002-4664-5504
Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC). Stockholm University, Faculty of Science, Department of Physics.
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Number of Authors: 1632023 (English)In: Physical Review Letters, ISSN 0031-9007, E-ISSN 1079-7114, Vol. 130, no 26, article id 261002Article in journal (Refereed) Published
Abstract [en]

Multiple viable theoretical models predict heavy dark matter particles with a mass close to the Planck mass, a range relatively unexplored by current experimental measurements. We use 219.4 days of data collected with the XENON1T experiment to conduct a blind search for signals from multiply interacting massive particles (MIMPs). Their unique track signature allows a targeted analysis with only 0.05 expected background events from muons. Following unblinding, we observe no signal candidate events. This Letter places strong constraints on spin-independent interactions of dark matter particles with a mass between 1 x 1012 and 2 x 1017 GeV/c2. In addition, we present the first exclusion limits on spin-dependent MIMP-neutron and MIMP-proton cross sections for dark matter particles with masses close to the Planck scale.

Place, publisher, year, edition, pages
2023. Vol. 130, no 26, article id 261002
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Subatomic Physics
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URN: urn:nbn:se:su:diva-223218DOI: 10.1103/PhysRevLett.130.261002ISI: 001058033400011PubMedID: 37450817Scopus ID: 2-s2.0-85164537137OAI: oai:DiVA.org:su-223218DiVA, id: diva2:1816226
Available from: 2023-12-01 Created: 2023-12-01 Last updated: 2023-12-07Bibliographically approved

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Conrad, JanRosso, Andrea GalloJoy, AshleyMahlstedt, JörnTan, Pueh-Leng

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