Self-consistent study of the proton shell effects near 146Gd

1980 ◽  
Vol 338 (1) ◽  
pp. 77-85 ◽  
Author(s):  
F. Tondeur
1972 ◽  
Vol 6 (1) ◽  
pp. 370-372 ◽  
Author(s):  
W. H. Bassichis ◽  
A. K. Kerman

1965 ◽  
Vol 43 (9) ◽  
pp. 2493-2507 ◽  
Author(s):  
P. O. Strom ◽  
G. R. Grant ◽  
A. C. Pappas

The independent fission yields in thermal neutron induced fission of 235U have been measured to be (9.5 ± 1.4)•10−6% and (1.04 ± 0.17)•10−3% for 124gSb and 126gSb, respectively. The total independent yields for all isomers of these nuclides are estimated to be (1.2 ± 0.2)•10−5% for 124Sb and (3.7 ± 0.6)•10−3% for 126Sb using a Huizenga–Vandenbosch approach for estimating population of isomeric states.These data do not seem to support a 50 proton shell effect on the Zp function, using the "unique" charge distribution curve of Wahl. A revised Wahl plot based on recent information on neutron emission from individual fission fragments is given and discussed in view of shell effects in fission. It is shown that the effect of the Zp function of the 50 proton shell is very small.


2004 ◽  
Vol 69 (5) ◽  
Author(s):  
A. K. Dutta ◽  
M. Onsi ◽  
J. M. Pearson

1970 ◽  
Vol 2 (5) ◽  
pp. 1768-1776 ◽  
Author(s):  
W. H. Bassichis ◽  
A. K. Kerman

1970 ◽  
Vol 25 (12) ◽  
pp. 1977
Author(s):  
S.M. Qaim

Abstract The systematics of cross sections for (n,p) and (n,a) re-actions induced by 14 - 15 MeV neutrons have been reinvesti-gated. No clear evidence for the existence of any proton shell effects in these two reactions was found. The existence of shell effects in nuclear reactions induced by 14 - 15 MeV neutrons has been postulated by several workers1-4 , but the evidence presented has been rather weak. With the availability of more and better experimental data in recent years, a fresh look at this postulate seemed highly desirable. In case of (n,p) and (n,2n) reactions, the claim for the occurence of shell effects has already been recently repudiated5,6 ; but for (n,α) reactions there seems to exist no evidence against the original claims1,2 that the cross section shows a minimum when the atomic number of the re-sidual nucleus is a magic number. The present article describes briefly a reinvestigation of the systematics of the (n,p) and (n,α) reaction cross sections in the light of the latest experimental data. At 14 MeV neutron energy there appears to be no conclusive evidence for any significant proton shell effects in these two re-actions.


1985 ◽  
Vol 38 (4) ◽  
pp. 555 ◽  
Author(s):  
MP Fewell ◽  
RH Spear ◽  
GK Adam ◽  
MT Esat

Values of B(E3; ot --+31) for the stable isotopes of Cd have been determined from particle spectra obtained using Coulomb excitation by 160 projectiles. The results are: 0�16 �O �04 e2 b3 (106Cd), 0.150�0.01O e2 b3 (108Cd), 0.1l5�0.013 e2 b3 (llOCd), 0.1l4�0.009 e2 b3 e12 Cd), 0.131 �0�015 'e2 b3 (114Cd) and 0-l00�0.01l e2b3 (1l6Cd). The corresponding E3 strengths are 34, 31,23,22,24 and 18 single particle units (s.p.u.) respectively. Examination of these and other data reveals no evidence for shell effects in B(E3; ot --+31) values near the Z = 50 proton shell, in contrast to the situation for B(E2; ot --+2 t) values.


1999 ◽  
Vol 173 ◽  
pp. 37-44
Author(s):  
M.D. Melita ◽  
A. Brunini

AbstractA self-consistent study of the formation of planetary bodies beyond the orbit of Saturn and the evolution of Kuiper disks is carried out by means of an N-body code where accretion and gravitational encounters are considered. This investigation is focused on the aggregation of massive bodies in the outer planetary region and on the consequences of such process in the corresponding cometary belt. We study the link between the bombardment of massive bodies and mass depletion and eccentricity excitation.


2002 ◽  
Vol 5 ◽  
pp. 65-65
Author(s):  
S. Liberatore ◽  
J.-P.J. Lafon ◽  
N. Berruyer

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