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Spin Dependence of Dark Matter Scattering

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arxiv 0806.1962 v1 pith:3CU6LAK5 submitted 2008-06-11 hep-ph astro-phhep-ex

Spin Dependence of Dark Matter Scattering

classification hep-ph astro-phhep-ex
keywords spinscatteringcrossdarkdependentmattermodelsenergy
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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New experiments designed to discover a weakly interacting dark matter (DM) particle via spin dependent scattering can distinguish models of electroweak symmetry breaking. The plane of spin dependent versus spin independent DM scattering cross sections is a powerful model diagnostic. We detail representative predictions of mSUGRA, singlet extended SM and MSSM, a new Dirac neutrino, Littlest Higgs with T-parity (LHT) and Minimal Universal Extra Dimensions (mUED) models. Of these models, the nMSSM has the largest spin dependent (SD) cross section. It has a very light neutralino which would give lower energy nuclear recoils. The Focus Point region of mSUGRA, mUED and the right handed neutrino also predict a very large SD cross section and predict a large signal of high energy neutrinos in the IceCube experiment from annihilations of dark matter in the Sun. We also describe a model independent treatment of the scattering of DM particles of different intrinsic spins.

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