Cross Section of Slow Neutrons on Parahydrogen

1971 ◽  
Vol 26 (25) ◽  
pp. 1581-1585 ◽  
Author(s):  
Theodore L. Houk ◽  
David Shambroom ◽  
Richard Wilson
Keyword(s):  
1935 ◽  
Vol 48 (4) ◽  
pp. 367-372 ◽  
Author(s):  
J. H. van Vleck

1975 ◽  
Vol 12 (5) ◽  
pp. 1423-1427 ◽  
Author(s):  
J. Callerame ◽  
D. J. Larson ◽  
S. J. Lipson ◽  
R. Wilson
Keyword(s):  

Author(s):  
W. E. Burcham ◽  
M. Goldhaber

The disintegration of nitrogen by slow neutrons has been studied in photographic emulsions of different sensitivity, which enable an unambiguous distinction to be made between the emission of α-particles and protons. Evidence has been obtained that the disintegration takes place according to the reactionwith a cross-section of about 10−24 cm.2


The neutron velocity selector of the Cavendish Laboratory has been used to measure the scattering cross-sections of ortho- and para -hydrogen for slow neutrons. The triplet and singlet scattering amplitudes of the neutron-proton interaction may be deduced from these cross-sections. The values obtained are a t = (0·537 ± 0·004) x 10 -12 cm, a s = -(2·373 ±0·007) x 10 -12 cm, where a t and a s are the triplet and singlet scattering amplitudes respectively. The values of the coherent scattering amplitude ƒ = 2(3/4 a +1/4 a ), and of the free proton cross-section σ ƒ = 4π(3/4 a 2 t + 1/4 a 2 s given by the above values of a t and a s , are ƒ = -(0·380 ± 0·005) x 10 -12 cm, σ ƒ = (20·41 ± 0·14) x 10 -24 cm 2 .


1935 ◽  
Vol 31 (1) ◽  
pp. 145-152 ◽  
Author(s):  
C. H. Westcott ◽  
T. Bjerge

The discovery of Fermi and his collaborators, that neutrons are much more readily captured by various atoms, e.g. silver, when their kinetic energies, originally of the order of 106 e.v., have been reduced by collisions with hydrogen nuclei, has been confirmed.The process of slowing down of the neutrons has been studied in some detail, and the nuclear cross-section for collisions with hydrogen nuclei has been determined for the primary neutrons and for the slow neutrons which are readily captured by silver atoms.The nature of the “gas” of slow neutrons was also discussed, but it was not found possible to reach a definite conclusion as to the energy of the neutrons concerned.


The adsorption and scattering of slow neutrons have been studied by various methods. In their first survey, Amaldi, D'Agostino, Fermi, Pontecorvo, Rasetti and Segré (1935) investigated the absorption of slow neutrons by different elements inside a paraffin block. The number of slow neutrons capture in an indicator (e. g. silver). The values for the absorption coefficients which they obtained with this arrangement can be regarded as a measure of the ''true'' absorption of slow neutrons. Later, Dunning, Pegram, Fink and Mitchell (1935) measured the "total" cross-sections, i. e. the sum of the well-defined beam of slow neutrons, and a lithium-coated ionization chamber as indicator. Recently, Griffiths and Szilard (1937) have determined the cross-section of some strongly absorbing elements using the captured γ-rays from cadmium as indicator. The scattering of slow neutrons was studied for some elements by MItchell and Murphy (1935), Mitchell, Murphy and Whitaker (1936), Budnitzky and Kurtschatow (1935) Pontecorvo and Wick (1936), and others. In these experiments, the slow neutrons issuing from a paraffin block passed through an indicator (e. g. silver), and were scattered backwards from the substance under investigation. When thin scattered are used, the percentage increase of the radioactivity produced in the indicator gives a measure of the scattering cross-section. This method has the disadvantage, even in the case of good scatters, that the increase in the radioactivity of the indicator is usually small compared with the effect due to the primary neutrons. A quantitative interpretation of the results may be further complicated by the fact that the neutrons leave the surface of the paraffin block at angles from 0 to 90°. Also, multiple scattering is not avoided.


1975 ◽  
Vol 12 (5) ◽  
pp. 1428-1431 ◽  
Author(s):  
J. Callerame ◽  
D. J. Larson ◽  
S. J. Lipson ◽  
R. Wilson
Keyword(s):  

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