Ionic charge dependence of the internal conversion coefficient and nuclear lifetime of the first excited state in125Te

1997 ◽  
Vol 55 (4) ◽  
pp. 1665-1675 ◽  
Author(s):  
F. Attallah ◽  
M. Aiche ◽  
J. F. Chemin ◽  
J. N. Scheurer ◽  
W. E. Meyerhof ◽  
...  
1975 ◽  
Vol 11 (4) ◽  
pp. 1455-1458 ◽  
Author(s):  
F. K. Wohn ◽  
W. L. Talbert ◽  
R. S. Weinbeck ◽  
M. D. Glascock ◽  
J. K. Halbig

1. Introduction .—The Internal Conversion Coefficient of γ-rays has recently been calculated by Hulme and by Taylor and Mott. The assumptions on which both of these calculations rest may be analysed as follows. I.—A nucleus, originally in an excited state of energy W n , radiates, corresponding to the transition to each lower state of energy W m , an electromagnetic field which may be either that of a dipole or that of a quadripole. For a dipole such a field has scalar and vector potentials given by


1986 ◽  
Vol 91 (4) ◽  
pp. 352-358 ◽  
Author(s):  
N. Venkateswara Rao ◽  
Ch. Suryanarayana ◽  
D. G. S. Narayana ◽  
S. Bhuloka Reddy ◽  
G. Satynarayana ◽  
...  

1949 ◽  
Vol 27a (2) ◽  
pp. 17-25 ◽  
Author(s):  
J. P. Stanley

Hulme's formula for the internal conversion of γ-radiation is simplified and used to calculate the internal conversion coefficient in the electric dipole case for electrons in the K-shell. For each of the elements Z = 69, 74, 79, 84, 89, IK is calculated for 10 values of the variable [Formula: see text] and a table obtained by interpolation is given for θ = 0.05 to θ = 1.70.


2014 ◽  
Vol 87 ◽  
pp. 192-194 ◽  
Author(s):  
Izabela T. Matos ◽  
Marina F. Koskinas ◽  
Tatiane S. Nascimento ◽  
Ione M. Yamazaki ◽  
Mauro S. Dias

1972 ◽  
Vol 50 (19) ◽  
pp. 2348-2354 ◽  
Author(s):  
S. K. Sen ◽  
D. L. Salie ◽  
E. Tomchuk

The decay of 169Yb was investigated using several Ge(Li) detectors of different sizes. The following gamma rays (energies in keV and intensities within brackets) were definitely identified with the 169Yb decay: 20.7 (0.66 ± 0.04), 63.1 (124 ± 5), 93.6 (7.2 ± 0.3), 109.8 (50 ± 2), 117.3 (0.08 ± 0.04), 118.2 (5.4 ± 0.2), 130.5 (34 ± 2), 156.7 (0.023 ± 0.004), 177.2(59 ± 3), 198.0 (100), 240.4 (0.33 ± 0.02), 261.0 (4.7 ± 0.2), and 307.7 (28 ± 1). The recently reported weak gamma-ray peaks at 515 (0.008 ± 0.002) and 625 (0.010 ± 0.002) were also observed and could not be ruled out as not belonging to 169Yb. The recently reported gamma-ray peaks at 140, 160, 207, 288, 295, 316, 320, 328, 355, 371, 379, 396, and 417 were detected and shown not to be from the decay of 169Yb while those at 218, 229, 285, 304, 335, 388, 411, and 425 were not observed and upper limits were placed on their intensities. The presence of very weak peaks at 515 and 625 establishes the formation of the 633 keV state of 169Tm following electron capture decay of 169Yb as reported by George. (This level has been previously observed only in Coulomb excitation of 169Tm.) The total internal conversion coefficient for the 20.7 keV transition was determined for the first time from the direct measurement of the gamma-ray intensity as 51 ± 10 corresponding to an M1 transition.


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