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The top documents tagged [cosmic ray interaction]
Is the Gruneisen "constant C is the specific heat Cosmic ray in the bar: Thermo Acoustical Conversion under the hypothesis that all the deposited energy,
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Neutrino emission =0.27 MeV E=0.39,0.86 MeV =6.74 MeV ppI loss: ~2% ppII loss: 4% note: /Q= 0.27/26.73 = 1% ppIII loss: 28% Total loss: 2.3%
215 views
Anti-hypernuclei production and search for P-odd domain formation at RHIC Gang Wang ( for the STAR Collaboration ) UCLA A colored and flavored system in
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Zhangbu Xu Introduction & Motivation Evidence of first antihypernucleus – and signal (for discovery) – Mass and Lifetime measurements What can we do with
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CBM-China Meeting, Tsinghua U., Nov. 2-5, 2009 1 Zebo Tang, USTC Zebo Tang University of Science and Technology of China (USTC) Hypernucleus production
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Zebo Tang University of Science and Technology of China (USTC)
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13 January, 2005Seminar at UCSC 1 Up-to-date Cosmic p-ISM Interaction Modeling and “Anomalies” in -Rays, Positrons, and Anti-Protons 13 January, 2005
212 views
Zhangbu Xu (for the STAR Collaboration)
54 views