Please use this identifier to cite or link to this item: https://hdl.handle.net/1959.11/63222
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dc.contributor.authorEbadi, Rezaen
dc.contributor.authorMathur, Anubhaven
dc.contributor.authorTanin, Erwin Hen
dc.contributor.authorTailby, Nicholas Den
dc.contributor.authorMarshall, Mason Cen
dc.contributor.authorRavi, Aakashen
dc.contributor.authorTrubko, Raisaen
dc.contributor.authorFu, Roger Ren
dc.contributor.authorPhillips, David Fen
dc.contributor.authorRajendran, Surjeeten
dc.contributor.authorWalsworth, Ronald Len
dc.date.accessioned2024-10-01T00:36:45Z-
dc.date.available2024-10-01T00:36:45Z-
dc.date.issued2021-07-30-
dc.identifier.citationPhysical Review D, 104(1), p. 1-10en
dc.identifier.issn2470-0029en
dc.identifier.issn2470-0010en
dc.identifier.urihttps://hdl.handle.net/1959.11/63222-
dc.description.abstract<p>Self-interactions within the dark sector could clump dark matter into heavy composite states with low number density, leading to a highly suppressed event rate in existing direct detection experiments. However, the large interaction cross section between such ultraheavy dark matter (UHDM) and standard model matter results in a distinctive and compelling signature; long, straight damage tracks as they pass through and scatter with matter. In this work, we propose using geologically old quartz samples as largeexposure detectors for UHDM. We describe a high-resolution readout method based on electron microscopy, characterize the most favorable geological samples for this approach, and study its reach in a simple model of the dark sector. The advantage of this search strategy is twofold; the age of geological quartz compensates for the low number density of ultraheavy composite dark matter, and the distinct geometry of the damage track serves as a high-fidelity background rejection tool.</p>en
dc.languageenen
dc.publisherAmerican Physical Societyen
dc.relation.ispartofPhysical Review Den
dc.rightsAttribution 4.0 International*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.titleUltraheavy dark matter search with electron microscopy of geological quartzen
dc.typeJournal Articleen
dc.identifier.doi10.1103/physrevd.104.015041en
local.contributor.firstnameRezaen
local.contributor.firstnameAnubhaven
local.contributor.firstnameErwin Hen
local.contributor.firstnameNicholas Den
local.contributor.firstnameMason Cen
local.contributor.firstnameAakashen
local.contributor.firstnameRaisaen
local.contributor.firstnameRoger Ren
local.contributor.firstnameDavid Fen
local.contributor.firstnameSurjeeten
local.contributor.firstnameRonald Len
local.profile.schoolSchool of Environmental & Rural Scienceen
local.profile.emailntailby@une.edu.auen
local.output.categoryC1en
local.record.placeauen
local.record.institutionUniversity of New Englanden
local.publisher.placeUnited States of Americaen
local.identifier.runningnumber015041en
local.format.startpage1en
local.format.endpage10en
local.peerreviewedYesen
local.identifier.volume104en
local.identifier.issue1en
local.access.fulltextYesen
local.contributor.lastnameEbadien
local.contributor.lastnameMathuren
local.contributor.lastnameTaninen
local.contributor.lastnameTailbyen
local.contributor.lastnameMarshallen
local.contributor.lastnameRavien
local.contributor.lastnameTrubkoen
local.contributor.lastnameFuen
local.contributor.lastnamePhillipsen
local.contributor.lastnameRajendranen
local.contributor.lastnameWalsworthen
dc.identifier.staffune-id:ntailbyen
local.profile.orcid0000-0002-2305-3338en
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local.identifier.unepublicationidune:1959.11/63222en
dc.identifier.academiclevelAcademicen
dc.identifier.academiclevelAcademicen
dc.identifier.academiclevelAcademicen
dc.identifier.academiclevelAcademicen
dc.identifier.academiclevelAcademicen
dc.identifier.academiclevelAcademicen
dc.identifier.academiclevelAcademicen
dc.identifier.academiclevelAcademicen
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local.title.maintitleUltraheavy dark matter search with electron microscopy of geological quartzen
local.relation.fundingsourcenoteThis work was supported by the DOE QuANTISED program under Award No. DE-SC0019396; the Army Research Laboratory MAQP program under Contract No. W911NF-19-2-0181; and the University of Maryland Quantum Technology Center. S. R. is supported by the NSF under Grant No. PHY-1818899, the Superconducting Quantum Materials and Systems Center (SQMS) Quantum Center and DOE support for MAGIS.en
local.output.categorydescriptionC1 Refereed Article in a Scholarly Journalen
local.search.authorEbadi, Rezaen
local.search.authorMathur, Anubhaven
local.search.authorTanin, Erwin Hen
local.search.authorTailby, Nicholas Den
local.search.authorMarshall, Mason Cen
local.search.authorRavi, Aakashen
local.search.authorTrubko, Raisaen
local.search.authorFu, Roger Ren
local.search.authorPhillips, David Fen
local.search.authorRajendran, Surjeeten
local.search.authorWalsworth, Ronald Len
local.open.fileurlhttps://rune.une.edu.au/web/retrieve/b2330285-555a-43b4-bbba-dbd9fe82e147en
local.uneassociationNoen
local.atsiresearchNoen
local.sensitive.culturalNoen
local.year.published2021en
local.fileurl.openhttps://rune.une.edu.au/web/retrieve/b2330285-555a-43b4-bbba-dbd9fe82e147en
local.fileurl.openpublishedhttps://rune.une.edu.au/web/retrieve/b2330285-555a-43b4-bbba-dbd9fe82e147en
local.subject.for2020370505 Mineralogy and crystallographyen
local.subject.for2020370507 Planetary geologyen
local.subject.for2020510106 High energy astrophysics and galactic cosmic raysen
local.codeupdate.date2024-11-01T17:08:47.412en
local.codeupdate.epersonntailby@une.edu.auen
local.codeupdate.finalisedtrueen
local.original.for20203705 Geologyen
local.profile.affiliationtypeExternal Affiliationen
local.profile.affiliationtypeExternal Affiliationen
local.profile.affiliationtypeExternal Affiliationen
local.profile.affiliationtypeExternal Affiliationen
local.profile.affiliationtypeExternal Affiliationen
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local.profile.affiliationtypeExternal Affiliationen
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local.date.moved2024-10-01en
Appears in Collections:Journal Article
School of Environmental and Rural Science
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