Cosmic-Ray-Induced Nuclear Interactions in Meteorites

2009 ◽  
pp. 21-21-9
Author(s):  
Michael E. Lipschutz
1956 ◽  
Vol 4 (4) ◽  
pp. 826-833 ◽  
Author(s):  
R. Giacconi ◽  
A. Lovati ◽  
A. Mura ◽  
C. Succi

1968 ◽  
Vol 46 (5) ◽  
pp. 343-358 ◽  
Author(s):  
B. Judek

Interaction mean free paths of relativistic secondary particles emitted from interactions of heavy primary cosmic-ray nuclei in emulsions were measured. The results show that among the Be, Li, He, and singly charged secondary nuclei there are particles present which interact with a cross section several times higher than the expected geometrical value. The stars produced by these particles have the characteristics of ordinary nuclear interactions. There appears to be no interpretation of these observations in terms of any known particle phenomena.


2011 ◽  
Vol 38 (6) ◽  
pp. 155-157
Author(s):  
A. S. Borisov ◽  
V. G. Denisova ◽  
K. A. Kotelnikov ◽  
V. S. Puchkov ◽  
Yu. A. Trubkin ◽  
...  

2008 ◽  
Vol 175-176 ◽  
pp. 174-177 ◽  
Author(s):  
H. Aoki ◽  
K. Honda ◽  
N. Inoue ◽  
T. Ishii ◽  
N. Kawasumi ◽  
...  

1969 ◽  
Vol 24 (10) ◽  
pp. 1541-1543
Author(s):  
J. P. Mundra ◽  
D. P. Bhattacharyya ◽  
P. K. Senchaudhury

Abstract Nuclear interactions of cosmic rays under paraffin and lead have been studied by means of a counter controlled multiplate cloud chamber. The lead plates inside the chamber served as producer and analyser. A search has been made for the possible transition effect of nuclear interaction in lighter elements using charged components for triggering and to compare it with a previously observed apparent transition effect in graphite for neutron shower using coincidence of neutron counters. The results show a continuous increase of nuclear interaction with increasing thickness of paraffin absorber up to 30.4 gcm-2. A similar rise is also observed under 11.3 gem-2 of Pb.


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