Determination of the atomic number density of Rb vapor by using spectral Faraday rotation measurements

2013 ◽  
Vol 62 (5) ◽  
pp. 731-733 ◽  
Author(s):  
M. M. Tehranchi ◽  
S. M. Hamidi ◽  
B. Abaie
1986 ◽  
Vol 25 (23) ◽  
pp. 4483 ◽  
Author(s):  
Z. Wu ◽  
M. Kitano ◽  
W. Happer ◽  
M. Hou ◽  
J. Daniels

1994 ◽  
Vol 95 (1) ◽  
pp. 77-85 ◽  
Author(s):  
Jian‐Feng Chen ◽  
Ernest L. Madsen ◽  
James A. Zagzebski

Leaving out of consideration those nuclei of small atomic number it is possible to develop a statistical theory of nuclei. Bethe and Bacher (1936, p. 149), as well as many other writers, have treated this subject in great detail starting from the Hartree approximation. All these investigations were mainly concerned with the binding energy, and not much attention has been paid so far to the stability of nuclei according to the statistical theory, except the determination of the most stable nucleus with a given atomic number: this is due to the fact that previous investigators have always neglected to distinguish between quantum states with opposite spin, thereby losing the distinction between “odd” and “even” nuclei, which is essential for stability considerations.


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