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 2-8

3 Jul 2018, 16:30
IBS HQ, Daejeon, Korea

IBS HQ, Daejeon, Korea

Conveners

Parallel Session 2-8: DM

  • Ken-Ichi Fushimi (Tokushima University)

Presentation materials

There are no materials yet.

  1. Dr giomataris ioannis (cea)
    03/07/2018, 16:30
    Oral
    The Spherical Proportional Detector is a new type of radiation detector based on a spherical geometry. It consists of a large spherical gas volume with a central electrode forming a radial electric field. A small spherical sensor located at the center is acting as a proportional amplification structure. Combination of sub-keV energy threshold and versatility of the target (Ne, He, H) opens...
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  2. Dr Osamu Sato (Nagoya University)
    03/07/2018, 17:00
    Oral
    A variety of experiments have been developed over the past decades, aiming at the detection of Weakly Interactive Massive Particles (WIMPs) via their scattering in an instrumented medium. The sensitivity of these experiments has improved with a tremendous speed, thanks to a constant development of detectors and analysis methods. Detectors capable of reconstructing the direction of...
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  3. Prof. Jong-Chul Park (Chungnam National University)
    03/07/2018, 17:30
    Oral
    Searching for cosmic-origin rare new physics signals at Earth-surface-based detectors is usually challenging because of huge cosmic backgrounds. In order to avoid such a challenge, underground experiments are thus strongly motivated. If a signal of interest involves many features, however it becomes possible to isolate signal events from background ones. Along this line, I discuss boosted...
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  4. Kyu Jung Bae (Center for Theoretical Physics of the Universe, Institute for Basic Science)
    03/07/2018, 18:00
    Oral
    We consider a model of decaying dark matter whose lifetime is comparable to the age of the universe. Its late decay to slightly lighter dark matter particle plus "non-interacting" particle can solve small scale problems. We will also show a smoking-gun signature of "non-interacting" particles from the dark matter decay.
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