The reduced transition probabilities for excited states of rare-earths and actinide even-even nuclei

2015 ◽  
Author(s):  
S. S. Ghumman
2016 ◽  
Vol 94 (4) ◽  
Author(s):  
T. Grahn ◽  
S. Stolze ◽  
D. T. Joss ◽  
R. D. Page ◽  
B. Sayğı ◽  
...  

2018 ◽  
Vol 33 (32) ◽  
pp. 1850188
Author(s):  
Rajesh Kharab

The dependence of reduced transition probabilities corresponding to electric quadrupole [B(E2)] and magnetic dipole [B(M1)] transition occurring in [Formula: see text]F nucleus on excitation energy and spin parity of the states involved in the transition has been investigated within the framework of simple potential model based on M3Y interaction. It is found that B(E2) increases with increasing excitation energy irrespective of the spin of excited states while B(M1) is very sensitive to the spin of the excited states and is independent of excitation energy.


1977 ◽  
Vol 15 (5) ◽  
pp. 1671-1678 ◽  
Author(s):  
R. M. Ronningen ◽  
J. H. Hamilton ◽  
A. V. Ramayya ◽  
L. Varnell ◽  
G. Garcia-Bermudez ◽  
...  

Solar Physics ◽  
1975 ◽  
Vol 44 (2) ◽  
pp. 257-267 ◽  
Author(s):  
T. Andersen ◽  
O. Poulsen ◽  
P. S. Ramanujam ◽  
A. Petrakiev Petkov
Keyword(s):  

2018 ◽  
Vol 178 ◽  
pp. 02028 ◽  
Author(s):  
Erin E. Peters ◽  
Timothy J. Ross ◽  
Benjamin P. Crider ◽  
Steven W. Yates

The stable isotopes of xenon, which have attracted interest for a number of reasons, span a transitional region that evolves from γ-soft structures for the lighter mass isotopes to nearly spherical 136Xe with a closed neutron shell. The nature of this transition, which is gradual, is not well understood. To provide detailed spectroscopic information on the Xe isotopes, we have studied 130,132,134,136Xe at the University of Kentucky Accelerator Laboratory using inelastic neutron scattering and γ-ray detection. These measurements yielded γ-ray angular distributions, branching ratios, multipole mixing ratios, and level lifetimes (from the Doppler-shift attenuation method), which allowed the determination of reduced transition probabilities and provided insight into the structure of these nuclei.


1988 ◽  
Vol 124 (3) ◽  
pp. 371-382 ◽  
Author(s):  
Peter W. Sengeløv ◽  
Jens Oddershede

2005 ◽  
Vol 25 (S1) ◽  
pp. 409-413 ◽  
Author(s):  
K. Yamada ◽  
T. Motobayashi ◽  
N. Aoi ◽  
H. Baba ◽  
K. Demichi ◽  
...  

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