Comparison of the E(5) Critical Point Symmetry to the γ-Rigid Solution of The Bohr Hamiltonian for γ =30°

2007 ◽  
Author(s):  
D. Bonatsos ◽  
D. Lenis ◽  
D. Petrellis ◽  
P. A. Terziev ◽  
I. Yigitoglu
2019 ◽  
Vol 14 ◽  
pp. 71
Author(s):  
Dennis Bonatsos ◽  
D. Lenis ◽  
D. Petrellis ◽  
P. Terziev ◽  
I. Yigitoglu

A γ-rigid solution of the Bohr Hamiltonian for 7 = 30° is derived, its ground state band being related to the second order Casimir operator of the Euclidean algebra E(4). Parameter-free (up to overall scale factors) predictions for spectra and B(E2) transition rates are in close agreement to the E (5) critical point symmetry, as well as to experimental data in the Xe region around A = 130.


2005 ◽  
Vol 621 (1-2) ◽  
pp. 102-108 ◽  
Author(s):  
Dennis Bonatsos ◽  
D. Lenis ◽  
D. Petrellis ◽  
P.A. Terziev ◽  
I. Yigitoglu

2006 ◽  
Vol 15 (08) ◽  
pp. 1735-1740 ◽  
Author(s):  
D. L. BALABANSKI ◽  
K. A. GLADNISHKI ◽  
G. LO BIANCO ◽  
A. SALTARELLI ◽  
N. V. ZAMFIR ◽  
...  

Lifetimes of excited states in 128 Ce were measured using the recoil distance Doppler-shift (RDDS) and the Doppler-shift attenuation (DSAM) methods. The experiments were performed at the Wright Nuclear Structure Laboratory of Yale University. Excited states of 128 Ce were populated in the 100 Mo (32 Si ,4 n ) reaction at 120 MeV and the nuclear γ decay was measured with an array of eight Clover detectors positioned at forward and backward angles. The deduced yrast transition strengths together with the energies of the levels within the ground-state (gs) band of 128 Ce are in agreement with the predicted values for the X (5) critical point symmetry. Thus, we suggest 128 Ce as a benchmark X (5) nucleus in the mass A ≈ 130 region.


2014 ◽  
Vol 44 (5) ◽  
pp. 501-505
Author(s):  
Jia XU ◽  
ShengXin LI ◽  
Yang AN ◽  
Yun ZHAO ◽  
DongQi YU ◽  
...  

2004 ◽  
Vol 69 (3) ◽  
Author(s):  
D. Tonev ◽  
A. Dewald ◽  
T. Klug ◽  
P. Petkov ◽  
J. Jolie ◽  
...  

2002 ◽  
Vol 88 (23) ◽  
Author(s):  
R. Krücken ◽  
B. Albanna ◽  
C. Bialik ◽  
R. F. Casten ◽  
J. R. Cooper ◽  
...  

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