10–15 Apr 2016
UZ Obergurgl
Europe/Zurich timezone

Session

WED2

13 Apr 2016, 18:20
UZ Obergurgl

UZ Obergurgl

University Center Obergurgl Gaisbergweg 5 6456 Obergurgl Austria

Presentation materials

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  1. Michael Duerr (DESY)
    13/04/2016, 18:20
    Dark Matter
    Talk
    I present an extension of the Standard Model where baryon number is a local gauge symmetry that is spontaneously broken. In such a setup, anomaly cancellation requires the introduction of new fermion fields, the lightest of which is an attractive dark matter candidate. Dark matter stability is an automatic consequence of the gauge symmetry, and proton decay never occurs even if baryon number...
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  2. Dan Levin (University of Michigan (US))
    13/04/2016, 18:40
    Dark Matter
    Talk
    Signatures of large missing transverse momentum recoiling against jets at the LHC provide powerful probe to strongly produced dark matter (DM), complementary to direct and indirect DM detection experiments. This talk presents recent results on dark matter searches with the ATLAS detector in LHC Run 2, focusing on signatures with jets, photons or hadronically decaying bosons.
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  3. Manfred Jeitler (Austrian Academy of Sciences (AT))
    13/04/2016, 19:00
    Dark Matter
    Talk
    The existence of dark matter, indicated by astronomical observations, is one of the main proofs of physics beyond the standard model. Despite its abundance, dark matter has not been directly observed yet. This talk presents several searches for dark matter production in proton-proton collisions at 7, 8, and 13 TeV at the LHC, performed by the CMS collaboration. They are interpreted in terms of...
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  4. Giorgio Busoni
    Talk
    The Sun may act as a gravitational well and capture Dark Matter at a constant rate: DM would therefore accrete inside the Sun. In absence of Annihilation (for example, for Asymmetric Dark Matter) the total number of captured DM particles at $t=t_{sun}$ may have stabilised to a constant number only if capture goes in equilibrium with evaporation, for DM masses below 5-10 GeV, while for higher...
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