Light Dark World International Forum 2016

Session

Afternoon Session

11 Jul 2016, 14:30

CTPU seminar room (Daejeon, Korea)

5. New Electron Fixed Target Experiments to Search for Light Dark Matter

Gordan Krnjaic (Fermilab)

11/07/2016, 14:30

This talk analyzes the present status of sub-GeV thermal dark matter annihilating through Standard Model mixing. In these scenarios, the requirement that dark matter be a thermal relic sets a sharp sensitivity target for terrestrial experiments, and that one of the simplest and best-motivated interactions between the SM and light dark matter the vector portal remains viable. Moreover,...

6. Right-handed neutrino dark matter and the B-L gauge boson

Kunio Kaneta (IBS-CTPU)

11/07/2016, 15:20

11. Disappearance of dancing reactor neutrinos at RENO

Soo-Bong Kim (SNU)

12/07/2016, 14:30

The RENO collaboration has observed energy and baseline distance dependent disappearance of reactor neutrinos that are emitted from the Hanbit nuclear power plant in South Korea. The experimental group has measured a neutrino squared-mass difference and the smallest neutrino mixing probability more precisely. Both of them are essential for understanding the unknown nature of neutrinos. The...

12. Interacting Dark Matter and Radiation in Cosmology

Tang Yong (KIAS)

12/07/2016, 15:20

17. Searches for axion and sterlile neutrino from the CUP (Center for Undergroud Physics), IBS

Hyang Kyu Park (IBS CUP)

13/07/2016, 14:30

The CUP at IBS has performed two experiments, KIMS (Korean Invisible Mass Search) at Yangyang Underground Laboratory and NEOS (Neutrino Experiment for Oscillation at Short baseline) in the tendon gallery of 3 GWth nuclear reactor at Yeounggwang. In this talk, we will will present results for solar axion search from the KIMS and for sterile neutrino search from the NEOS.

22. Search for Dark Interactions at the LHC

Ketevi Assamagan (BNL)

14/07/2016, 14:30

Hidden sector or dark sector states appear in many extensions to the Standard Model, to provide a candidate for the dark matter in the universe or to explain astrophysical observations of positron excesses. A hidden or dark sector can be introduced with an additional $U(1)_d$ dark gauge symmetry. The presence of the dark sector could be inferred either from deviations from the SM-predicted...