-
Abstract:
An experiment, using a large magnetic cloud chamber to search for new Particlesin horizontal cosmic rays is described. The result is: the flux of particles with unitcharge, β<0.7, m>1 GeV/c2 or the flux of relativistic fractional charge particiles isless than 3×10-8cm-2sr-1sec-1.
-
-
References
[1]
|
原子能研究所云南站,物理,1(1972),57.[2] 袁余奎、霍安祥等,高能物理与核物理,2,(1978), 478.[3] Yuan, C. L. Luck and C. S. Wu, Nuclear Physics, Vol. 5, Academic Pr., New York, 1961.[4] R. E. Kepler et al., Nuovo Cim., 7(1958), 71.[5] 中国科学院高能物理研究所三室,u介子在氦氛混合气体中的游离能损曲线(1974)未发表.
|
-
[1] |
GUO Yun-Jun
, HE Kang-Lin
. Muon Identification Using the Efficiencies Ratio Method at BESⅡ. Chinese Physics C,
2007, 31(11): 1050-1055. |
[2] |
HU Xi-Duo
, SHAO Ming-Zhu
, LUO Shi-Yu
, LIU Yong-Sheng
, ZHU De-Hai
. Average Field Idea and Single Particle Model for 2 Dimension Crystallization Beams(Ⅱ). Chinese Physics C,
2004, 28(2): 196-199. |
[3] |
LI Ming-Liang
, ZHU Sheng-Jiang
, CHE Xing-Lai
, YU Ying-Nan
. Research on Two-Quasiparticle Bands in 98Sr. Chinese Physics C,
2004, 28(S1): 75-77. |
[4] |
CHANG KONG-LIANG
. DIMENSIONAL METHOD TO SOLVE THE DIFFUSION CONVECTION EQUATION OF SOLAR COSMIC RAYS. Chinese Physics C,
1978, 2(3): 200-210. |
-
Access
-
-