Nov 12 – 15, 2013
Pagoda Hotel & Restaurant
Pacific/Honolulu timezone

Session

Dark Matter IV

Nov 14, 2013, 4:20 PM
C'est Si Bon (Pagoda Hotel & Restaurant)

C'est Si Bon

Pagoda Hotel & Restaurant

1525 Rycroft St. Honolulu, HI 96814

Description

Chair: Hai-Bo Yu (University of California, Riverside)

Presentation materials

There are no materials yet.

  1. Prof. Ariel Zhitnitsky (University of British Columbia)
    11/14/13, 4:20 PM
    Dark Matter
    oral
    I review a testable dark matter model outside of the standard WIMP paradigm in which the observed ratio Omega_{DM}~ 5 Omega_{B} for visible and dark matter densities finds its natural explanation as a result of their common QCD origin. Special emphasis is placed on the observational consequences of this model and on the detection prospects for present or planned experiments. In...
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  2. Dr Shinta Kasuya (Kanagawa University)
    11/14/13, 4:45 PM
    Dark Matter
    oral
    We consider the Q-ball decay and investigate the scenario that the amount of the baryons and the gravitino dark matter is at the same time naturally explained by the decay of the Q balls in the gauge-mediated SUSY breaking. We show the decay rates into baryons, NLSPs, and gravitinos, and estimate their branching ratios based on the consideration of Pauli blocking. Although the NLSPs...
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  3. Patrick Stengel (University of Hawaii)
    11/14/13, 5:10 PM
    Dark Matter
    oral
    We consider a class of leptogenesis models in which the lepton asymmetry arises from dark matter annihilation processes which violate CP and lepton number. Importantly, a necessary one-loop contribution to the annihilation matrix element arises from absorptive final state interactions. We elucidate the relationship between this one-loop contribution and the CP-violating phase. As we show, the...
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  4. Mr Keita Fukushima (University of Hawaii at Manoa)
    11/14/13, 5:35 PM
    Dark Matter
    oral
    g-2 correction has been accurately measured in the E821 experiment at Brookhaven National Lab (BNL). Yet, there remains a 3 sigma difference between experiment and theory. One way that this discrepancy can be interpreted is by new particles running in the loop. The smallness of this discrepancy provides a tight constraint on its coupling. This bound is then applied to constrain the...
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