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    德国美因茨大学刘佳博士报告

    发布时间:2015.06.11

    来源: 本站

    Seminar Talk at CTP-SCU / 理论物理中心学术报告

    Speaker: Dr. Jia Liu (刘佳 博士) (Johannes Gutenberg-University Mainz 德国美因茨大学)

    Title: Boosted Dark Matter in IceCube and at the Galactic Center

    Abstract:
    We show that the event excess observed by the IceCube collaboration at TeV--PeV
    energies, usually interpreted as evidence for astrophysical neutrinos, can be
    explained alternatively by the scattering of highly boosted dark matter
    particles. Specifically, we consider a scenario where a $\sim 4$~PeV scalar
    dark matter particle $\phi$ can decay to a much lighter dark fermion $\chi$,
    which in turn scatters off nuclei in the IceCube detector. Besides these
    events, which are exclusively shower-like, the model also predicts a secondary
    population of events at $\mathcal{O}(100\ \text{TeV})$ originating from the
    3-body decay $\phi \to \chi \bar\chi a$, where $a$ is a pseudoscalar which
    mediates dark matter--Standard Model interactions and whose decay products
    include neutrinos.  This secondary population also includes track-like events,
    and both populations together provide an excellent fit to the IceCube data.  We
    then argue that a relic abundance of light Dark Matter particles $\chi$, which
    may constitute a subdominant component of the Dark Matter in the Universe, can
    have exactly the right properties to explain the observed excess in GeV gamma
    rays from the galactic center region.

    Time: 6/11 (Thu) 4:00pm 

    Venue: Physics building 323, CTP-SCU