Deuterons from High-Energy Proton Bombardment of Matter

1961 ◽  
Vol 7 (2) ◽  
pp. 69-71 ◽  
Author(s):  
S. T. Butler ◽  
C. A. Pearson
Keyword(s):  
High Energy ◽  
Proton Bombardment ◽  
High Energy Proton ◽  
Energy Proton

Formation Cross Sections of Nucleides Produced from Heavy Elements by High-energy Proton Bombardment

1974 ◽  
Vol 29 (5) ◽  
pp. 822-825
Author(s):  
B. K. Gupta ◽  
S. Das
Keyword(s):  
Cross Sections ◽  
High Energy ◽  
Heavy Elements ◽  
Proton Bombardment ◽  
High Energy Proton ◽  
Energy Proton

Abstract Theoretical cross sections for the production of elements from 209Bi and natural copper by high-energy proton bombardment have been calculated.

Effects of high energy proton bombardment (50-280 MeV) on dc SQUIDS

1995 ◽  
Vol 5 (2) ◽  
pp. 3252-3254 ◽  
Author(s):  
B. Muhlfelder ◽  
G.M. Gutt ◽  
J.M. Lockhart ◽  
P. Carelli ◽  
A. Zehnder ◽  
...  
Keyword(s):  
High Energy ◽  
Proton Bombardment ◽  
High Energy Proton ◽  
Energy Proton

Deuterons from High-Energy Proton Bombardment of Matter

1963 ◽  
Vol 129 (2) ◽  
pp. 836-842 ◽  
Author(s):  
S. T. Butler ◽  
C. A. Pearson
Keyword(s):  
High Energy ◽  
Proton Bombardment ◽  
High Energy Proton ◽  
Energy Proton

Tritiumdiffusionsmessungen an vier Steinmeteoriten

1965 ◽  
Vol 20 (12) ◽  
pp. 1686-1691 ◽  
Author(s):  
H. Fechtig ◽  
W. Gentner
Keyword(s):  
Room Temperature ◽  
Diffusion Constant ◽  
High Energy ◽  
Production Mechanism ◽  
Proton Bombardment ◽  
High Energy Proton ◽  
Tritium Production ◽  
Energy Proton ◽  
Diffusion Constants ◽  
Stony Meteorite

Four stony meteorites have been examined for their tritium diffusion constants. Tritium for the diffusion measurements has been produced in the meteoritic material by neutron activation and high energy proton bombardment. The tritium diffusion constants were found to be different for the two tritium production mechanism. Tritium production by high energetic proton bombardment approaches more easely to the production mechanism caused by cosmic radiation and therefore this diffusion constant should be applied for the calculation of tritium losses. In the case of proton produced tritium, values of D/α2 are of the order of 10-18 sec-1, whereas for tritium produced by n-activation, the values are between 10-10 and 10-14 sec-1. — Using the found D/α2 values only for one stony meteorite (Alfianello) the tritium loss is of the order of 40% within 10 years. For the other meteorites the tritium loss within 10 years at room temperature is below 1%.

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