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个人简介
PhD in Physics, Stanford University, 9/82-6/88. Specialization: Experimental particle physics. Thesis: Baryon production in e +e − Annihilation at an Ecm of 29 GeV. Advisor: Professor Tom Himel. Graduate minor in anthropology, concentrating in archaeology. BA in Physics, University of California, San Diego, 9/79 - 6/81. Minor in history.
Senior Scientist, 2008-present, and Staff Physicist, 1994-2008, Lawrence Berkeley Laboratory. Deputy Director, Nuclear Science Division, 2010-present. Group Leader for Neutrino Astronomy. Lead 10-person LBNL group working on the 250 member international IceCube 1 km3 neutrino observatory, 2007- present. Co-lead Diffuse and Atmospheric Neutrino Physics Working Group, 2007- present. Co-convenor, STAR ultra-peripheral collisions (UPCs) working group, 1997-2000 & 2002-2007.
My research interests focus on neutrino astronomy with the 1 km3
IceCube detector
now being constructed at the South Pole. Our group is searching for high-energy
extra-terrestrial neutrinos, particularly electron and tau neutrinos. We are also interested
in high pT particle (specifically muons) production in cosmic-ray air showers
and, more generally, in phenomenology of high-energy nuclear astrophysics. We are
also involved with prototypes for the proposed ARIANNA detector; this is a 100 km3
neutrino detector on the Ross Ice Shelf, sensitive to neutrinos with energies above
1017 eV. In addition to the astrophysics, I am also interested in how ultra-high energy
particles interact in matter.
I also study ultra-peripheral collisions (UPCs) of relativistic nuclei, such as twophoton
and photonuclear interactions. UPCs probe a wide range of physics topics,
from strong field electrodynamics to meson spectroscopy to entangled quantum states.
Awards and Honors:
Named Fellow of the American Physical Society, Nov. 2009.
Publications:
1. Muon Acceleration in Cosmic-ray Sources, S. R. Klein, R. Mikkelsen, J. K.Becker
Tjus, arXiv:1208.2056, submitted to Phys. Rev. Lett.
2. Lateral Distribution of Muons in IceCube Cosmic Ray Events, R. Abbasi et al.,
arXiv:1208.2979, accepted by Phys. Rev. D.
3. An improved method for measuring muon energy using the truncated mean
of dE/dx, R. Abbasi et al., arXiv:1208.3430, accepted by Nuclear Instrum. &
Meth.
4. ρ
0 Photoproduction in AuAu Collisions at √
sNN =62.4 GeV with STAR, G.
Agakishiev et al., Phys. Rev. C85, 014910 (2012).
研究兴趣
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