6533b851fe1ef96bd12aa01a
RESEARCH PRODUCT
Theoretical direct WIMP detection rates for transitions to the first excited state inKr83
Jouni SuhonenPraveen C. SrivastavaJ. D. VergadosJ. D. VergadosMatti J KortelainenMatti J KortelainenF. T. AvignonePekka Pirinensubject
PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsBranching fractionDark matterGamma rayInelastic scattering01 natural sciencesWIMPWeakly interacting massive particlesExcited state0103 physical sciences010306 general physicsSpin (physics)description
The direct detection of dark matter constituents, in particular the weakly interacting massive particles (WIMPs), is central to particle physics and cosmology. In this paper we study transitions to the excited states, possible in some nuclei, which have sufficiently low lying excited states. Examples considered previously were the first excited states of $^{127}\mathrm{I}$ and $^{129}\mathrm{Xe}$. We examine here $^{83}\mathrm{Kr}$, which offers some kinematical advantages and is a possible target. We estimate appreciable rates for the inelastic scattering mediated by the spin cross sections, with an inelastic event rate of $4.4\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}4}\text{ }\text{ }{\mathrm{kg}}^{\ensuremath{-}1}\text{ }{\mathrm{d}}^{\ensuremath{-}1}$. So, the extra signature of the gamma ray following the de-excitation of these states can, in principle, be exploited experimentally. A brief discussion of the experimental feasibility is given.
year | journal | country | edition | language |
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2015-07-16 | Physical Review D |