Physics – High Energy Physics – High Energy Physics - Theory
Scientist
Physics
High Energy Physics
High Energy Physics - Theory
Scientist
School of Informatics and Computing, Indiana University, Bloomington, IN, USA
ITP Acadimia Sinica
Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma
University of Virginia
SETI Institute, Mountain View, California
Department of Geology, University of Illinois, Urbana, IL 61801, USA; Department of Geological Sciences, University of Michigan, Ann Arbor, MI 48109, USA
NASA Ames Research Ctr., USA
Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, P. R. China
National Astronomical Observatoires, Chinese Academy of Sciences;, Graduate University of Chinese Academy of Sciences
The University of Oklahoma
National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, China; Also at: Department of Astronomy, University of Virginia, Charlottesville, VA 22904 of California, Santa Cruz, USA and NASA Ames Research Ctr., USA
Department of Geology, University of Illinois at Urbana-Champaign, Urbana, Illinois, USA
Seismological Laboratory, California Institute of Technology, M / C 252-21, Pasadena, CA 91125, USA
National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, China
School of Earth and Space Sciences Peking University Beijing 100871 P. R. China
Institute of Atmospheric Physics, Chinese Academy of Sciences, Beijing, China
$N=2$ and $4$ Super Yang-Mills Theories on $M_4 \times Z_2 \times Z_2$ Geometry
$N=2$ and $N=4$ SUSY Yang-Mills action on $M^4\times (Z_2\oplus Z_2)$ non-commutative geometry
$α$-vacuum and inflationary bispectrum
3D Radiative Transfer with PHOENIX
A 3D radiative transfer framework: V. Homologous Flows
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