Widths and spectroscopic factors in21O

2012 ◽  
Vol 85 (2) ◽  
Author(s):  
H. T. Fortune ◽  
R. Sherr
Keyword(s):  
Spectroscopic Factors

Spectroscopic factors for alpha decay in the NpNn scheme

2008 ◽  
Vol 665 (4) ◽  
pp. 182-185 ◽  
Author(s):  
Madhubrata Bhattacharya ◽  
Subinit Roy ◽  
G. Gangopadhyay
Keyword(s):  
Alpha Decay ◽  
Spectroscopic Factors

Proton spectroscopic factors of Sm isotopes in the pairing-plus-quadrupole model

1986 ◽  
Vol 448 (1) ◽  
pp. 36-44 ◽  
Author(s):  
Krishna Kumar ◽  
J.B. Gupta ◽  
J.H. Hamilton
Keyword(s):  
Spectroscopic Factors

Intermediate Coupling in 55Fe

1971 ◽  
Vol 49 (13) ◽  
pp. 1832-1835 ◽  
Author(s):  
M. Csürös ◽  
J. A. Cameron ◽  
Z. Zàmori
Keyword(s):  
Collective Model ◽  
Electromagnetic Properties ◽  
Intermediate Coupling ◽  
Spectroscopic Factors ◽  
Good Agreement

Calculations based on the collective model with intermediate coupling between the surface oscillations of the even–even core 54Fe and 29th neutron have been carried out. Level energies, spectroscopic factors, and electromagnetic properties are obtained in good agreement with experiment.

Study of the 33Cl spectroscopic factors via the 32S(3He,d)33Cl one-proton transfer reaction

2021 ◽  
Author(s):  
Ivano Lombardo ◽  
Daniele Dell'Aquila ◽  
Marco Cinausero ◽  
Leandro Romero Gasques ◽  
Mariano Vigilante ◽  
...  
Keyword(s):  
Proton Transfer ◽  
Transfer Reaction ◽  
Proton Transfer Reaction ◽  
Spectroscopic Factors

scholarly journals (d,n) proton-transfer reactions on Be9, B11, C13, N14,15 , and F19 and spectroscopic factors at Ed=16MeV

2017 ◽  
Vol 96 (2) ◽  
Author(s):  
M. Febbraro ◽  
F. D. Becchetti ◽  
R. O. Torres-Isea ◽  
J. Riggins ◽  
C. C. Lawrence ◽  
...  
Keyword(s):  
Proton Transfer ◽  
Transfer Reactions ◽  
Spectroscopic Factors ◽  
Proton Transfer Reactions

scholarly journals The 7Be(p, ?)8B Cross Section at Low Energies

1980 ◽  
Vol 33 (2) ◽  
pp. 177 ◽  
Author(s):  
FC Barker
Keyword(s):  
Cross Section ◽  
Cross Sections ◽  
Solar Neutrinos ◽  
Model Calculations ◽  
Spectroscopic Factors ◽  
Low Energies ◽  
Standard Values ◽  
Experimental Values ◽  
Parameter Values ◽  
Potential Parameters

The nonresonant part of the 7Be(p, )I)8B cross section at low energies is recalculated by means of a direct-capture potential model, using parameter values determined by fitting 7Li(n, n)7Li and 7Li(n, )I)8Li data. Standard values of the potential parameters and spectroscopic factors give values of the 7Li(n,)I) cross section that are too large. Modified values that fit the thermal-neutron capture cross section predict 7Be(p,)I) cross sections that are much less than the experimental values. Also, shell model calculations predict resonant 7Be(p,)I) cross sections that are smaller than the experimental values. It is suggested that the accepted experimental values of the 7Be(p, )I) cross section may be too large, perhaps due partly to an overlarge accepted value for the 7Li(d, p)8Li cross section, which has been used for normalization purposes. A decrease in the 7Be(p,)I) cross section would reduce the calculated detection rate of solar neutrinos and lessen the discrepancy with the measured value.

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