Connecting the direct detection of dark matter with observation of sparticles at the LHC

An analysis is given connecting event rates for the direct detection of neutralino dark matter with the possible signatures of supersymmetry at the LHC. It is shown that if an effect is seen in the direct detection experiments at a level of O(10<sup>-</sup><sup>4</sup><sup...

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spelling ndltd-NEU--neu-3321462016-04-25T16:14:48ZConnecting the direct detection of dark matter with observation of sparticles at the LHCAn analysis is given connecting event rates for the direct detection of neutralino dark matter with the possible signatures of supersymmetry at the LHC. It is shown that if an effect is seen in the direct detection experiments at a level of O(10<sup>-</sup><sup>4</sup><sup>4</sup>) cm<sup>2</sup> for the neutralino-proton cross section, then within the mSUGRA model the next heavier particle above the neutralino is either a stau, a chargino, or a CP odd/CP even (A/H) Higgs boson. Further, the collider analysis shows that models with a neutralino-proton cross section at the level of (1 − 5) × 10<sup>-</sup><sup>4</sup><sup>4</sup> cm<sup>2</sup> could be probed with as little as 1 fb<sup>-</sup><sup>1</sup> of integrated luminosity at the LHC at √s = 7, 10 TeV. The most recent limit from the five tower CDMS II result on WIMP-nucleon cross section is discussed in this context. It is argued that the conclusions of the analysis given here are more broadly applicable with inclusion of non-universalities in the SUGRA models.http://hdl.handle.net/2047/d20000422
collection NDLTD
sources NDLTD
description An analysis is given connecting event rates for the direct detection of neutralino dark matter with the possible signatures of supersymmetry at the LHC. It is shown that if an effect is seen in the direct detection experiments at a level of O(10<sup>-</sup><sup>4</sup><sup>4</sup>) cm<sup>2</sup> for the neutralino-proton cross section, then within the mSUGRA model the next heavier particle above the neutralino is either a stau, a chargino, or a CP odd/CP even (A/H) Higgs boson. Further, the collider analysis shows that models with a neutralino-proton cross section at the level of (1 − 5) × 10<sup>-</sup><sup>4</sup><sup>4</sup> cm<sup>2</sup> could be probed with as little as 1 fb<sup>-</sup><sup>1</sup> of integrated luminosity at the LHC at √s = 7, 10 TeV. The most recent limit from the five tower CDMS II result on WIMP-nucleon cross section is discussed in this context. It is argued that the conclusions of the analysis given here are more broadly applicable with inclusion of non-universalities in the SUGRA models.
title Connecting the direct detection of dark matter with observation of sparticles at the LHC
spellingShingle Connecting the direct detection of dark matter with observation of sparticles at the LHC
title_short Connecting the direct detection of dark matter with observation of sparticles at the LHC
title_full Connecting the direct detection of dark matter with observation of sparticles at the LHC
title_fullStr Connecting the direct detection of dark matter with observation of sparticles at the LHC
title_full_unstemmed Connecting the direct detection of dark matter with observation of sparticles at the LHC
title_sort connecting the direct detection of dark matter with observation of sparticles at the lhc
publishDate
url http://hdl.handle.net/2047/d20000422
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