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

Plenary Session 7

3 Jul 2018, 09:00
IBS HQ, Daejeon, Korea

IBS HQ, Daejeon, Korea

Conveners

Plenary Session 7: DM/ SNNS

  • Stefano Scopel (Sogang University)

Presentation materials

There are no materials yet.

  1. Prof. Rybka Gray (University of Washington)
    03/07/2018, 09:00
    Oral
    The axion is a well-motivated dark matter candidate inspired by the Peccei-Quinn solution to the Strong-CP problem. After decades of work, the US DOE flagship axion dark matter search, ADMX G2, is the first experiment to be sensitive to dark matter axions from the plausible DFSZ coupling model, and has begun to search the theoretically-favored axion mass region 2-40 micro-eV. ADMX G2...
    Go to contribution page
  2. Dr Yannis K. Semertizidis (CAPP/IBS)
    03/07/2018, 09:30
    Oral
    The center for axion and precision physics (IBS/CAPP) is moving from the construction phase into operation mode regarding a number of axion dark matter experiments. I will describe our status in setting up the ultimate axion dark matter experiments in a wide frequency range. We are commissioning high-field, high-volume magnets and we are developing the required quantum-noise-limited amplifiers...
    Go to contribution page
  3. Dr Motohiko Kusakabe (Beihang University)
    03/07/2018, 10:00
    Oral
    A huge number of neutrinos are emitted from a neutron star at the core-collapse supernova (SN) explosion. These neutrinos interact with nucleons and nuclei, and proton and neutron abundances are affected via charged-current (CC) reactions of electron neutrinos and antineutrinos in the inner region of SNe. As a result, some of light proton-rich nuclei (p-nuclei) are produced in a proton-rich...
    Go to contribution page
Building timetable...