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dc.contributor.authorMartoff, C. J.
dc.contributor.authorSciolla, Gabriella
dc.date.accessioned2012-05-07T19:37:21Z
dc.date.available2012-05-07T19:37:21Z
dc.date.issued2009-10
dc.date.submitted2009-05
dc.identifier.issn1367-2630
dc.identifier.urihttp://hdl.handle.net/1721.1/70532
dc.description.abstractDark matter (DM) detectors with directional sensitivity have the potential of yielding an unambiguous positive observation of WIMPs as well as discriminating between galactic DM halo models. In this paper, we introduce the motivation for directional detectors, discuss the experimental techniques that make directional detection possible, and review the status of the experimental effort in this field.en_US
dc.description.sponsorshipMassachusetts Institute of Technology. Dept. of Physicsen_US
dc.description.sponsorshipUnited States. Dept. of Energy (contract number DE-FG02-05ER41360)en_US
dc.description.sponsorshipUnited States. Dept. of Energy (Fermilab)en_US
dc.language.isoen_US
dc.publisherInstitute of Physics Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/1367-2630/11/10/105018en_US
dc.rightsCreative Commons Attribution 3.0en_US
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/en_US
dc.sourceNew Journal of Physicsen_US
dc.titleGaseous dark matter detectorsen_US
dc.typeArticleen_US
dc.identifier.citationSciolla, G, and C J Martoff. “Gaseous Dark Matter Detectors.” New Journal of Physics 11.10 (2009): 105018. Web.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.approverSciolla, Gabriella
dc.contributor.mitauthorSciolla, Gabriella
dc.relation.journalNew Journal of Physicsen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsSciolla, G; Martoff, C Jen
mit.licensePUBLISHER_CCen_US
mit.metadata.statusComplete


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