Professor Yong-Hamb Kim’s research interest is in the development and applications of low temperature detectors. Particularly, Yong-Hamb is intrigued by new physics and detector developments using micro-calorimeters. Applications include high resolution alpha and Q spectroscopies, direct detection of dark matter, and search for neutrinoless double beta decay. He is an active member of AMoRE, KIMS+, and XMASS.
■ Experience
2013 - Present: Group Leader
Institute of Basic Science, Center for Underground Physics
2011 - Present: Professor
University of Science and Technology, Nano Science
2011 - 2012: Visiting Scientist
NASA Goddard Space Flight Center, Astrophysics division
2005 - Present: Senior/Principal Research Scientist
Korea Research Institute of Standards and Science
2003 - 2005: Postdoctoral Research Associate, Brown University
2003 Ph.D. Brown University, USA
■ Major Activities
2013 – Present: International Advisory Committee of LTD conference
2012 – Present: International Advisory Committee of IWSSD workshop
2006 – Present: Steering Committee Member of the AMoRE experiment
2006 – Present: Member of Korean Physical Society
I have been interested in searching for anything beyond the standard model to understand what the Universe is. Now I am after the dark matter of the Universe by searching for axion. Then, the next after the dark matter will be the rest of the Universe.
My research interests lie in modern particle physics, focussing especially on the strong CP problem and one of its great candidate solutions, the axion.
Recently, I have started simulating the results of the spin-dependent interaction experiment motivated by Moody and Wilczek by the finite element method (FEM) software, OPERA.