Dipole γ-ray emission in fusion heavy-ion reactions: beam energy dependence

Author(s):  
B. Martin
2003 ◽  
Vol 67 (3) ◽  
Author(s):  
B. Fornal ◽  
R. Broda ◽  
K. H. Maier ◽  
P. J. Daly ◽  
P. Bhattacharyya ◽  
...  

1988 ◽  
Vol 37 (1) ◽  
pp. 163-168 ◽  
Author(s):  
K. G. R. Doss ◽  
H.-A. Gustafsson ◽  
H. H. Gutbrod ◽  
D. Hahn ◽  
K.-H. Kampert ◽  
...  

1989 ◽  
Vol 40 (4) ◽  
pp. 1685-1699 ◽  
Author(s):  
M. Betty Tsang ◽  
George F. Bertsch ◽  
William G. Lynch ◽  
Mitsuru Tohyama

1978 ◽  
Vol 56 (3) ◽  
pp. 321-326 ◽  
Author(s):  
I. M. Ladenbauer-Bellis ◽  
P. Sen ◽  
H. Bakhru

181Ir activity was produced via the following heavy-ion reactions: 169Tm (16O,4n)181Ir and 169Tm(19F,7n)181Pt (51 s) decaying to 181Ir. The half-life of 181Ir was found to be 4.90 ± 0.15 min. Singles and coincidence γ-ray measurements were performed using 30–40 cm3 Ge(Li) detectors. X-Ray measurements were carried out using an intrinsic Ge-detector. Additionally the helium jet system was used to study the properties of this isotope. The following γ rays were found to belong to the decay of 181Ir: 19.6, 65.3, 93.8, 107.6, 117.9, 123.5, 184.6, 189.9, 227.0, 231.6, 239.2, 309.0, 318.9, 350.5, 352.8, 375.2, 576.5, 700.1, 871.2, 1182.3, 1192.6, 1347.1, 1381.0, 1528.8, 1545.0, 1565.6, 1593.4, 1639.6, 1646.4, 1652.5, and 1714.9 keV. A tentative decay scheme is proposed for 181Ir, verifying levels in l8lOs that have been obtained by reaction work. The proposed decay scheme as well as spin and parity assignments of some of the 181Os levels are discussed.


1987 ◽  
Vol 02 (03) ◽  
pp. 163-168 ◽  
Author(s):  
P. BECKMANN ◽  
H.A. GUSTAFSSON ◽  
H.H. GUTBROD ◽  
K.H. KAMPERT ◽  
B. KOLB ◽  
...  

The collective azimuthal alignment of charged particles is observed inside of two groups of particles, one emitted to the backward and one emitted to the forward hemisphere in the center of mass of symmetric heavy ion collisions. Whereas for Ca+Ca collisions no effect is observed, the alignment is present for Nb+Nb, and is even more pronounced for Au+Au. There exists also a distinct multiplicity and energy dependence of this collective azimuthal alignment.


2019 ◽  
Vol 99 (6) ◽  
Author(s):  
J. Adam ◽  
L. Adamczyk ◽  
J. R. Adams ◽  
J. K. Adkins ◽  
G. Agakishiev ◽  
...  

1982 ◽  
Vol 25 (5) ◽  
pp. 2504-2511 ◽  
Author(s):  
R. L. Auble ◽  
J. B. Ball ◽  
F. E. Bertrand ◽  
R. L. Ferguson ◽  
C. B. Fulmer ◽  
...  

2003 ◽  
Vol 17 (1) ◽  
pp. 71-76 ◽  
Author(s):  
D. Pierroutsakou ◽  
A. Boiano ◽  
A. De Rosa ◽  
M. Di Pietro ◽  
G. Inglima ◽  
...  
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