Charge amplification concepts for direction-sensitive dark matter detectors

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dc.creatorDujmic, D.
dc.creatorFisher, P.
dc.creatorSciolla, G.
dc.creatorAhlen, S.
dc.creatorDutta, V.
dc.creatorHenderson, S.
dc.creatorKaboth, A.
dc.creatorKohse, G.
dc.creatorLanza, R.
dc.creatorMonroe, J.
dc.creatorRoccaro, A.
dc.creatorSkvorodnev, N.
dc.creatorTomita, H.
dc.creatorVanderspek, R.
dc.creatorWellenstein, H.
dc.creatorYamamoto, R.
dc.date2008-04-30
dc.date2008-08-22
dc.date.accessioned2026-07-07T11:50:25Z
dc.date.available2026-07-07T11:50:25Z
dc.descriptionDirection measurement of weakly interacting massive particles in time-projection chambers can provide definite evidence of their existence and help to determine their properties. This article demonstrates several concepts for charge amplification in time-projection chambers that can be used in direction-sensitive dark matter search experiments. We demonstrate reconstruction of the 'head-tail' effect for nuclear recoils above 100keV, and discuss the detector performance in the context of dark matter detection and scaling to large detector volumes.
dc.description15 pages, 9 figures
dc.identifierhttps://arxiv.org/abs/0804.4827
dc.identifierhttp://arxiv.org/abs/0804.4827
dc.identifierAstropart.Phys.30:58-64,2008
dc.identifierdoi:10.1016/j.astropartphys.2008.06.009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/203556
dc.subjectAstrophysics
dc.titleCharge amplification concepts for direction-sensitive dark matter detectors
dc.typetext

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