Physics – Condensed Matter – Strongly Correlated Electrons
Scientist
Physics
Condensed Matter
Strongly Correlated Electrons
Scientist
MIchigan State University and JINA
Michigan State University and JINA
MSU
Michigan State Univ. and JINA
Pohang Accelerator Laboratory, POSTECH
Department of Physics and Astronomy and JINA: Joint Institute for Nuclear Astrophysics, Michigan State University, USA of Physics and Astronomy, CSCE: Center for the Study of Cosmic Evolution, and JINA: Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, MI 48824
Department of Chemistry and Department of Astronomy, Kyung Hee University, Suwon 449-701, South Korea
Department of Chemistry, Kyunghee University, Suwon, 449-701, South Korea, KR
Michigan State University & JINA
Michigan State University, USA
Michigan State University / JINA
Department of Physics, Indiana University, Bloomington, Indiana 47405, USA; GSI, Darmstadt, D64291, Germany
Department of Physics, Indiana University, Bloomington, Indiana 47405
Indiana University, Bloomington, Indiana 47408
Department of Physics, Indiana University, Bloomington, IN 47405, USA; GSI, Darmstadt D64291, Germany
Centre for Research in Earth and Space Science, York University, Toronto, Ontario, Canada
Department of Mechanical Engineering, Pohang University of Science and Technology, San 31 Hyoja Dong, Pohang, 790-784, South Korea
Department of Mechanical Engineering, Pohang University of Science and Technology, San 31 Hyoja Dong, Pohang, 790-784 South Korea
Department of Astronomy and Space Science, Chungbuk National University
Michigan State Univ
Michigan State University
Department of Astronomy and Space Science, ChungBuk National University
$T_1$- and $T_2$-spin relaxation time limitations of phosphorous donor electrons near crystalline silicon to silicon dioxide interface defects
A Cu2+ (S = 1/2) Kagomé Antiferromagnet: MgxCu4-x(OH)6Cl2
A Development History and Structural Feature of Sogyupyo in the Joseon Dynasty
A formation of uranium phosphate, ningyoite, by Shewanella p. CN32
A Search for Evidence of an Abundance Gradient in the Galactic Halo Based on Stars from SDSS-I DR-5
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