Closing in on asymmetric dark matter I: model independent limits for interactions with quarks

High Energy Physics - Phenomenology High Energy Physics - Phenomenology (hep-ph) Cosmology and Nongalactic Astrophysics (astro-ph.CO) 0103 physical sciences FOS: Physical sciences 01 natural sciences Astrophysics - Cosmology and Nongalactic Astrophysics
DOI: 10.1007/jhep08(2012)029 Publication Date: 2012-08-08T03:17:36Z
ABSTRACT
18+6 pages, 18 figures. v2: version accepted for publication<br/>It is argued that experimental constraints on theories of asymmetric dark matter (ADM) almost certainly require that the DM be part of a richer hidden sector of interacting states of comparable mass or lighter. A general requisite of models of ADM is that the vast majority of the symmetric component of the DM number density must be removed in order to explain the observed relationship $��_B\sim��_{DM}$ via the DM asymmetry. Demanding the efficient annihilation of the symmetric component leads to a tension with experimental limits if the annihilation is directly to Standard Model (SM) degrees of freedom. A comprehensive effective operator analysis of the model independent constraints on ADM from direct detection experiments and LHC monojet searches is presented. Notably, the limits obtained essentially exclude models of ADM with mass 1GeV$\lesssim m_{DM} \lesssim$ 100GeV annihilating to SM quarks via heavy mediator states. This motivates the study of portal interactions between the dark and SM sectors mediated by light states. Resonances and threshold effects involving the new light states are shown to be important for determining the exclusion limits.<br/>
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