Alpha decay from excited states of samarium isotopes

1966 ◽  
Vol 22 (2) ◽  
pp. 186-188 ◽  
Author(s):  
J. Kvítek ◽  
Yu.P. Popov
Keyword(s):  
1973 ◽  
Vol 28 (10) ◽  
pp. 1635-1641 ◽  
Author(s):  
A. G. de Pinho ◽  
M. Weksler

The X-ray spectra resulting from the internal conversion of electric quadrupole transitions following the alpha decay of Th230 and Ra226 were analysed with a Si (Li) spectrometer. From the knowledge of the Coster-Kronig and fluorescence yields, the internal conversion coefficients of the E2 transitions from the first excited states in Ra226 and Rn222 could be deduced. Results are in good agreement with theoretical values.


2011 ◽  
Vol 850 (1) ◽  
pp. 34-52 ◽  
Author(s):  
K.P. Santhosh ◽  
Sabina Sahadevan ◽  
Jayesh George Joseph

2011 ◽  
Vol 321 ◽  
pp. 012036
Author(s):  
M Freer ◽  
S Almaraz-Calderon ◽  
A Aprahamian ◽  
N I Ashwood ◽  
M Barr ◽  
...  

2010 ◽  
Vol 44 (2) ◽  
pp. 287-295 ◽  
Author(s):  
Y. Z. Wang ◽  
J. Z. Gu ◽  
J. M. Dong ◽  
B. B. Peng

2006 ◽  
Vol 765 (3-4) ◽  
pp. 263-276 ◽  
Author(s):  
D.L. Price ◽  
M. Freer ◽  
S. Ahmed ◽  
N.I. Ashwood ◽  
N.M. Clarke ◽  
...  

2010 ◽  
Vol 37 (3) ◽  
pp. 035103 ◽  
Author(s):  
P J Haigh ◽  
M Freer ◽  
N I Ashwood ◽  
T Bloxham ◽  
N Curtis ◽  
...  

1988 ◽  
Vol 102 ◽  
pp. 239
Author(s):  
M.S.Z. Chaghtai

Using R.D. Cowan’s computations (1979) and parametric calculations of Meinders et al (1982), old analyses are thoroughly revised and extended at Aligarh, of Zr III by Khan et al (1981), of Nb IV by Shujauddin et Chaghtai (1985), of Mo V by Tauheed at al (1985). Cabeza et al (1986) confirmed the last one largely.Extensive studies have been reported of the 1–e spectra, Zr IV (Rahimullah et al 1980; Acquista and Reader 1980), Nb V (Shujauddin et al 1982; Kagan et al 1981) and Mo VI (Edlén et al 1985). Some interacting 4p54d2levels of these spectra have been reported from our laboratory, also.Detailed spectral analyses of transitions between excited states have furnished complete energy values for J ≠ 1 levels of these spectra during 1970s and 80s. Shujauddin et al (1982) have worked out Nb VI and Tauheed et al (1984) Mo VII from our lab, while Khan et al (1981) share the work on Zr V with Reader and Acquista (1979).


Physica ◽  
1952 ◽  
Vol 18 (2) ◽  
pp. 1101-1104
Author(s):  
B FLOWERS
Keyword(s):  

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