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Particle Physics on the Plains​ 2018

13–14 Oct 2018
University of Kansas
US/Central timezone

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Session

Neutrinos and Dark Matter

14 Oct 2018, 09:00
1160 Integrated Science Building (University of Kansas)

1160 Integrated Science Building

University of Kansas

Department of Physics & Astronomy University of Kansas Malott Hall Lawrence, KS

Conveners

Neutrinos and Dark Matter

  • Bhupal Dev (Washington University in St. Louis)

Presentation materials

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  1. 3. An R-parity Violating Supersymmetric Explanation of the EeV Events at ANITA
    Yicong Sui (Washington University in Saint Louis)
    14/10/2018, 09:00

    The ANITA balloon experiment has observed two EeV-level, upgoing cascade events, which cannot be explained by the Standard Model neutrino interactions that make the Earth opaque to EeV neutrinos. In this paper, we analyze a long-lived bino interpretation in leptonic R-parity violating supersymmetry. In particular, a TeV-scale bino can be resonantly produced through the interaction of the EeV...

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  2. 26. Leptogenesis and neutrino mass generation in LR symmetric model
    Anil Thapa
    14/10/2018, 09:20
  3. 21. Galactic Dark Matter Population as the Source of Neutrino Masses
    Matthew Sullivan (University of Kansas)
    14/10/2018, 09:40

    The extremely small but non-zero neutrino masses has no explanation in the Standard Model. We propose a new mechanism for neutrino mass generation, unrelated to the Higgs mechanism, in which neutrinos get their mass via long range interactions with dark matter. Our model predicts a location dependent neutrino mass and also implies that relic neutrinos are not present in galaxies due to having...

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  4. 30. Reflections On Supersymmetry Searches at the LHC
    Carlos E.M. Wagner (University of Chicago)
    14/10/2018, 10:00
  5. 5. General Treatment of reflection of spherical waves from a spherical surface: Assuming reflected waves as locally plane waves
    Paramita Dasgupta (PhD student at Indian Institute of Technology Kanpur)

    We develop a general formalism to treat reflection of spherical electromagnetic waves from a spherical surface. Our main objective is interpret radio wave signals produced by cosmic ray interactions with Earth’s atmosphere which are observed by the Antarctica based ANITA detector after reflection off the ice surface. The incident wave is decomposed into plane waves and each plane wave is...

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  6. 29. GeV scale messengers of Planck Scale Dark Matter.
    Gopolang Mohlabeng (Brookhaven National Laboratory)
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