Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientist
Physics
High Energy Physics
High Energy Physics - Phenomenology
Scientist
University of California, Berkeley
UIUC
U. Chicago
Harvard-Smithsonian Center for Astrophysics
University of Illinois Department of Physics
U. of Illinois, Urbana-Champaign
Lawrence Berkeley National Lab
Fermilab
UC Berkeley
Depts Physics and Astronomy, UC Berkeley
with input from the SDSS-III collaboration
Enrico Fermi Institute
U. Illinois Urbana-Champaign
CfA
Harvard-CfA
UCB
UCBerkeley
Yale University.
Department of Earth and Ocean Sciences, National University of Ireland, Galway, Ireland
Yale University, New Haven, CT
Yale University., New Haven, CT
Enrico Fermi Institute, University of Chicago
Harvard-Smithsonian
Departments of Physics and Astronomy, University of Illinois at Urbana-Champaign 1110 West Green St, Urbana, Illinois 61801-3080
Department of Astronomy, 601 Campbell Hall, UC Berkeley, Berkeley, California 94720
Berkeley
CfPA
CfA, Harvard
Harvard-Smithsonian Center for Astrophysics, 60 Garden St, Cambridge, MA 02138, USA
Durham, University, Durham, England
Depts. of Physics and Astronomy, University of Illinois, Urbana-Champaign, 61801-3080, USA
Johnson Space Center, 2101 NASA Parkway, Houston, TX 77058, USA of California at Berkeley / Lawrence Berkeley National Lab
University of California
JPL
LBNL
Department of Physics, University of California at Berkeley, Berkeley, CA 94720, USA
University of California, Berkeley, CA, USA
Lawrence Berkeley National Laboratory
UC, Berkeley
Harvard-Smithsonian, CfA
UC Berkeley, LBNL
JPL, Pasadena, CA, USA
"Sample Variance" in Small-Scale CMB Anisotropy Experiments
$SU(3)$ vs. $SU(3) \times SU(3)$ Breaking in Weak Hyperon Decays
A Characteristic Scale on the Cosmic Microwave Sky
A CMB Polarization Primer
A comparison of cosmological Boltzmann codes: are we ready for high precision cosmology?
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Profile ID: LFWR-SCP-P-15916