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dc.contributor.authorLeman, Steven W.
dc.contributor.authorMcCarthy, Kevin Ahmad
dc.contributor.authorFigueroa-Feliciano, Enectali
dc.contributor.authorCabrera, B.
dc.contributor.authorPyle, M.
dc.contributor.authorResch, R.
dc.contributor.authorSadoulet, B.
dc.contributor.authorSundqvist, K. M.
dc.contributor.authorBrink, P. L.
dc.contributor.authordo Couto e Silva, Eduardo
dc.contributor.authorMirabolfathi, N.
dc.contributor.authorSerfass, B.
dc.contributor.authorTomada, A.
dc.date.accessioned2013-01-22T21:21:18Z
dc.date.available2013-01-22T21:21:18Z
dc.date.issued2011-02
dc.date.submitted2010-04
dc.identifier.issn1003-7713
dc.identifier.urihttp://hdl.handle.net/1721.1/76334
dc.description.abstractWe present results on quasidi usion studies in large, 3 inch diameter, 1 inch thick [100] high purity germanium crystals, cooled to 50 mK in the vacuum of a dilution refrigerator, and exposed with 59.5 keV gamma-rays from an Am-241 calibration source. We compare data obtained in two di erent detector types, with di erent phonon sensor area coverage, with results from a Monte Carlo. The Monte Carlo includes phonon quasidi usion and the generation of phonons created by charge carriers as they are drifted across the detector by ionization readout channels.en_US
dc.description.sponsorshipUnited States. Dept. of Energy (Grant DE-FG02-04ER41295)en_US
dc.description.sponsorshipUnited States. Dept. of Energy (Grant DE-FG02-07ER41480)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant PHY-0542066)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant PHY-0503729)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant PHY-0503629)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant PHY-0504224)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant PHY-0705078)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant PHY-0801712)en_US
dc.language.isoen_US
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://psroc.phys.ntu.edu.tw/cjp/download.php?type=full&vol=49&num=1&page=349en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alike 3.0en_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/en_US
dc.sourcearXiven_US
dc.titlePhonon Quasidiffusion in Cryogenic Dark Matter Search Large Germanium Detectorsen_US
dc.typeArticleen_US
dc.identifier.citationLeman, S. W. et al. “Phonon Quasidi usion in Cryogenic Dark Matter Search Large Germanium Detectors.” Chinese Journal of Physics 49.1 (2011): 349–358.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorLeman, Steven W.
dc.contributor.mitauthorMcCarthy, Kevin Ahmad
dc.contributor.mitauthorFigueroa-Feliciano, Enectali
dc.relation.journalChinese Journal of Chemical Physicsen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.identifier.orcidhttps://orcid.org/0000-0001-9285-5556
mit.licenseOPEN_ACCESS_POLICYen_US
mit.metadata.statusComplete


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