Physics – Condensed Matter – Strongly Correlated Electrons
Scientist
Physics
Condensed Matter
Strongly Correlated Electrons
Scientist
Colorado Research Associates Division, NorthWest Research Associates, Boulder, Colorado, USA
The Supernova Cosmology Project
Texas A&M University
Lawrence Berkeley
IFW Dresden, Dresden, Germany
Lawrence Berkeley Laboratory
LANL
Astronomy Centre, Dept. of Physics and Astronomy, University of Sussex, Brighton, UK
Institute of Physics, Chinese Academy of Sciences, Beijing, PRC
ZIMP Zhejiang U
MCTP and
Max-Planck-Institut für Festkörperforschung, Stuttgart, Germany
Colorado Researh Associates, a division of NorthWest Research Associates, Colorado Research Associates 3380 Mitchell Lane, Boulder, CO 80301, USA Department, U.C. Berkeley, University of California at Berkeley, Berkeley, CA 94720-7300, USA; Space Science Laboratory, 7 Gauss Way, Berkeley, CA 94720-7450, USA Sciences Lab, UCB, 7 Gauss Way University of California, Berkeley, Berkeley, CA 94720-7450, USA; Physics Department, UCB, 366 Le Conte Hall #7300, Berkeley, CA 94720-730, USA of Astronomy, University of Texas, Austin, TX 78712, USA Microstructures Facility, Rutherford Appleton Laboratory, Chilton, Oxon, UK
Laurence Berkeley Lab, 1 Cyclotron Rd., Berkeley, CA 94720, USA
University of Florida, Gainesville, FL, US
Space Sciences Lab, Univ California Berkeley, Berkeley, CA, USA; Sciences Laboratory Berkeley, Ca, Berkeley, CA, USA; Sciences Laboratory, University of California, Berkeley, CA, USA; of Mechanical and Electrical Engineering, Harbin Institute of Technology, Harbin 150001, China Centre, Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH
Space Sciences Laboratory, University of California Berkeley, Centennial Dr Grizzly Peak Blv, Berkeley, CA 94720, USA Sciences Lab University of California, Berkeley, 7 Gauss Way, Berkeley, CA 94720-
26Al, 10Be and U-Th isotopes in Blake Outer Ridge sediments: implications for past changes in boundary scavenging
3D Reconstruction of the 22 May 2007 Magnetic Cloud: How Much Can We Trust the Flux- Rope Geometry of CMEs?
3D Signatures of off-center Delayed-Detonation Models
86 Herschel sources SED model parameters (Rowan-Robinson+, 2010)
A complete line list for methane at 80 K (1.27 -1.71 micron) for planetary applications
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