29 June 2018 to 4 July 2018
IBS HQ, Daejeon, Korea
Asia/Seoul timezone
There will be Welcome Reception at 18:00 on June 28, 2018

Session

Parallel Session 2-1

29 Jun 2018, 14:00
IBS HQ, Daejeon, Korea

IBS HQ, Daejeon, Korea

Conveners

Parallel Session 2-1: NNR/ DM

  • Jouni Suhonen (University of Jyväskylä)

Presentation materials

There are no materials yet.

  1. Prof. Myung-Ki Cheoun (Soongsil University)
    29/06/2018, 14:00
    Oral
    In this talk, we discuss some feasible low energy neutrino sources and possible physics by the neutrinos emitted from them. One of them is the search for the existence of the fourth neutrino, we propose two experimental methods for short baseline electron antineutrino disappearance study. One is a source from 8Li generator under non-accelerator system. For 8Li production, we suggest to...
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  2. Dr Teppei Katori (Queen Mary University of London)
    29/06/2018, 14:30
    Oral
    Neutrino oscillation physics has been entered in the precision era. In this context accelerator-based neutrino experiments need a reduction of systematic errors to the level of a few percent. Today one of the most important sources of systematic errors are neutrino-nucleus cross sections which in the hundreds-MeV to few-GeV energy region are known with a precision not exceeding 10-20%. In this...
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  3. Ms ALEENA RAFIQUE (Kansas State University)
    29/06/2018, 15:00
    Oral
    MicroBooNE is an 85-tonne active mass Liquid Argon Time Projection Chamber (LArTPC) neutrino experiment on the Booster Neutrino Beamline at the Fermi National Accelerator Laboratory. One of MicroBooNE’s primary physics goals is to understand neutrino-argon scattering in the [0.5-2] GeV neutrino energy. This knowledge, in addition to being of intrinsic scientific interest, will be used in the...
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  4. Dr Arnab Dasgupta (Seoul National University of Science and Technology)
    29/06/2018, 15:30
    Oral
    In this letter we have explored the possibility of embedding the genesis of lepton asymmetry within the well studied *Scotogenic* model. We have shown that in this model one can have a Dark Matter in the TeV scale. The model is highly constrained in the context of dark matter,neutrino mass, Flavor Physics and now also gets an additional constraint on the relative complex phases from the...
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