Physics – Condensed Matter – Mesoscale and Nanoscale Physics
Scientist
Physics
Condensed Matter
Mesoscale and Nanoscale Physics
Scientist
CLEO Collaboration
AIfA Bonn
Argelander-Institut für Astronomie, Universität Bonn;
Shanghai Astronomical Observatory, China
Chicago, University, IL
Shanghai Astronomical Observatory, Shanghai, China
Chicago Univ., IL.
Chicago Univ., Chicago, IL.
NASA Ames / SETI Institute, Mail Stop 239-20 NASA Ames Research Center, Moffett Field, CA 94035, USA; UC- Santa Cruz, Computer Engineering Department School of Engineering 1156 High Street, Santa Cruz, CA 95604, USA University Berlin,Institute of Geodesy and Geoinformation Science, Berlin, Germany
The University of Chicago, Chicago, IL 60637-1433 USA
Berlin, Germany ; Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, China
Boston College, Chestnut Hill, MA
A Type 2 supernovae constraint on neutrinoe - neutrinos mixing
Amplitude analyses of the decays chi_c1 -> eta pi+ pi- and chi_c1 -> eta' pi+ pi-
Amplitude analysis of D0->K+K-pi+pi-
An update on the solar neutrino problem and the three-family MSW effect allowing for astrophysical uncertainties
Analysis of D+ to K- pi+ e+ nu_e and D+ to K- pi+ mu+ nu_mu Semileptonic Decays
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