scholarly journals ANGULAR DISTRIBUTION OF NUCLEAR INTERACTIONS OF HIGH ENERGY COSMIC RAY PARTICLES WITH PARAFFIN

1965 ◽  
Vol 21 (5) ◽  
pp. 976
Author(s):  
KUANG HAO-HWAI ◽  
LI RU-BAI ◽  
TAN YUE-HEN ◽  
LIU YUNG-YUIH
1956 ◽  
Vol 4 (4) ◽  
pp. 826-833 ◽  
Author(s):  
R. Giacconi ◽  
A. Lovati ◽  
A. Mura ◽  
C. Succi

2000 ◽  
Vol 195 ◽  
pp. 303-310
Author(s):  
A. V. Olinto

The surprising lack of a high energy cutoff in the cosmic ray spectrum at the highest energies, together with an apparently isotropic distribution of arrival directions, have strongly challenged most models proposed for the acceleration of ultrahigh energy cosmic rays. Young neutron star winds may be able to explain the mystery. We discuss this recent proposal after summarizing the observational challenge and plausible acceleration sites. Young neutrons star winds differ from alternative models in the predictions for composition, spectrum, and angular distribution, which will be tested in future experiments.


1952 ◽  
Vol 88 (6) ◽  
pp. 1277-1283 ◽  
Author(s):  
H. S. Green ◽  
H. Messel ◽  
B. A. Chartres

1963 ◽  
Vol 19 (4) ◽  
pp. 205
Author(s):  
WANG SHIH-WEI ◽  
KUANG HAO-HWAI ◽  
YUAN YU-KUEI

1963 ◽  
Vol 28 (6) ◽  
pp. 1238-1245 ◽  
Author(s):  
E. Farrow ◽  
C. F. Gauld ◽  
C. B. A. McCusker ◽  
J. Malos ◽  
K. Nishikawa ◽  
...  

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