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Please use this identifier to cite or link to this item: http://arks.princeton.edu/ark:/88435/dsp01ff3655377
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dc.contributorMarlow, Daniel-
dc.contributor.advisorCalaprice, Frank-
dc.contributor.authorArar, Benjamin-
dc.date.accessioned2013-07-31T20:19:12Z-
dc.date.available2013-07-31T20:19:12Z-
dc.date.created2013-05-06-
dc.date.issued2013-07-31-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/dsp01ff3655377-
dc.description.abstractWeakly Interacting Massive Particles (WIMPs) are a promising solution to the dark matter problem. The DarkSide experiment looks for a scintillation signal produced when WIMPs collide with a liquid argon atoms. Discrimination against background events depends critically on the light yield, defined as the number of photoelectrons detected per unit of recoil energy. The prototype detector DarkSide-10 measured a light yield of 9.142 photoelectrons/keV in 2012. It uses the wavelength shifter Tetraphenylbutadiene (TPB) to convert UV photons to the visible range for detection. In this thesis, we use a liquid argon detector of diameter 3.35 inches and height 1.5 inches with a different wavelength shifter, P-Terphenyl (PTP). A light yield of 9.82 photoelectrons/ keV was measured using the full-absorption peak of a gamma ray source.en_US
dc.format.extent40 pagesen_US
dc.language.isoen_USen_US
dc.titleLight Yield Study for Liquid Argon Dark Matter Detectorsen_US
dc.typePrinceton University Senior Theses-
pu.date.classyear2013en_US
pu.departmentPhysicsen_US
pu.pdf.coverpageSeniorThesisCoverPage-
dc.rights.accessRightsWalk-in Access. This thesis can only be viewed on computer terminals at the <a href=http://mudd.princeton.edu>Mudd Manuscript Library</a>.-
pu.mudd.walkinyes-
Appears in Collections:Physics, 1936-2020

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