12–13 Oct 2019
University of Kansas
US/Central timezone

Session

Neutrinos

13 Oct 2019, 10:50
2048 Mallot Hall (University of Kansas)

2048 Mallot Hall

University of Kansas

Department of Physics & Astronomy University of Kansas Lawrence, KS

Conveners

Neutrinos

  • Bhupal Dev (Washington University in St. Louis)

Presentation materials

There are no materials yet.

  1. Paramita Dasgupta (PhD student at Indian Institute of Technology Kanpur)
    13/10/2019, 10:50

    The NASA sponsored balloon-borne ANITA detector operating in Antarctica is designed to detect ultra high energy cosmic rays (UHECR) with energies exceeding 1 EeV ($10^{18}$ eV) by collecting the radio pulse generated through the interaction of the primary particle with Earth’s atmosphere. The radio pulse is detected after reflection from the Antarctic ice surface. For calibration and...

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  2. Garv Chauhan (Washington University in St. Louis)
    13/10/2019, 11:10

    Non-Standard Interactions (NSI) of neutrinos with matter are important to understand, as they could significantly alter the standard 3-neutrino oscillation paradigm. While vector NSI contribute as a change in the matter potential for the propagating neutrinos, scalar NSI show up as a correction to the neutrino mass matrix. In this talk, we will discuss the field-theoretic origin of scalar NSI...

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  3. anil thapa (Oklahoma State University)
    13/10/2019, 11:30

    Models of radiative Majorana neutrino masses require new scalars and/or fermions to induce lepton number violating interactions. We show that these new particles also generate observable neutrino nonstandard interactions (NSI) with the matter. We classify radiative models as type-I or II, with type-I models containing at least one Standard Model (SM) particle inside the loop diagram generating...

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  4. Mr Yicong Sui (Department of Physics and McDonnell Center for the Space Sciences, Washington University, St. Louis)
    13/10/2019, 11:50

    We propose a new way to probe non-standard interactions (NSI) of neutrinos with matter using the ultra-high energy (UHE) neutrino data at current and future neutrino telescopes. We consider the Zee model of radiative neutrino mass generation as a prototype, which allows two charged scalars -- one $SU(2)_L$-doublet and one a singlet, both being leptophilic, to be as light as 100 GeV, thereby...

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  5. Mr Vishnu Padmanabhan Kovilakam (OKLAHOMA STATE UNIVERSITY)
    13/10/2019, 12:10

    We carry out a systematic investigation of the minimal Dirac neutrino mass models emerging from generic one-loop and two-loop topologies that arise from $d=5$ effective operator with a singlet scalar, $\sigma$. To ensure that the tree-level Dirac mass, as well as Majorana mass terms at all order are absent for the neutrinos, we work in the framework where the Standard Model is supplemented by...

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  6. K.C. Kong (University of Kansas)
    13/10/2019, 12:30
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