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dc.contributor.advisorWebb, Robert
dc.creatorMannino, Rachel Louise
dc.date.accessioned2018-02-05T16:48:26Z
dc.date.available2018-02-05T16:48:26Z
dc.date.created2017-08
dc.date.issued2017-05-18
dc.date.submittedAugust 2017
dc.identifier.urihttps://hdl.handle.net/1969.1/165702
dc.description.abstractUnderstanding background events in a low-energy search for the WIMP dark matter candidate is critical to enable a viable search as these events must be reduced to avoid overwhelming the rare dark matter signal. The βˉ decay spectra from ²¹ºBi and from ⁸⁵Kr have energies in the dark matter search region of ≤100 keV. This work identifies 38.0 ± 6.2 ⁸⁵Kr events via its rare β-γ coincidence decay path in the LUX detector's 332-day dark matter search. Furthermore, the activity of ²¹ºBi which can be tolerated in the detector before it is discernible in the low-energy region of the radioactive background spectrum is determined for a variety of radial cuts to study how the mobile ²¹ºBi infiltrates a dark matter detector's fiducial volume. This sets a limit on acceptable ²¹ºBi activities which will help future low-energy experiments determine the steps they must take to build competitively sensitive detectors.en
dc.format.mimetypeapplication/pdf
dc.language.isoen
dc.subjectdark matteren
dc.subjectradioactive backgroundsen
dc.subject85Kren
dc.subjectKr-85en
dc.subject210Bien
dc.subjectBi-210en
dc.titleMeasuring Backgrounds from ⁸⁵Kr and ²¹ºBi to Improve Sensitivity of Dark Matter Detectorsen
dc.typeThesisen
thesis.degree.departmentPhysics and Astronomyen
thesis.degree.disciplinePhysicsen
thesis.degree.grantorTexas A & M Universityen
thesis.degree.nameDoctor of Philosophyen
thesis.degree.levelDoctoralen
dc.contributor.committeeMemberBraby, Leslie
dc.contributor.committeeMemberDutta, Bhaskar
dc.contributor.committeeMemberToback, David
dc.type.materialtexten
dc.date.updated2018-02-05T16:48:26Z
local.etdauthor.orcid0000-0003-3946-2299


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