Generalized Pairing in Light Nuclei. I. Solutions of Hartree-Fock-Bogoliubov Equations inN=ZEven-Even Nuclei

1969 ◽  
Vol 178 (4) ◽  
pp. 1670-1681 ◽  
Author(s):  
J. BAR-TOUV ◽  
A. GOSWAMI ◽  
A. L. GOODMAN ◽  
G. L. STRUBLE
Universe ◽  
2021 ◽  
Vol 7 (12) ◽  
pp. 470
Author(s):  
Valentin Allard ◽  
Nicolas Chamel

Temperature and velocity-dependent 1S0 pairing gaps, chemical potentials and entrainment matrix in dense homogeneous neutron–proton superfluid mixtures constituting the outer core of neutron stars, are determined fully self-consistently by solving numerically the time-dependent Hartree–Fock–Bogoliubov equations over the whole range of temperatures and flow velocities for which superfluidity can exist. Calculations have been made for npeμ in beta-equilibrium using the Brussels–Montreal functional BSk24. The accuracy of various approximations is assessed and the physical meaning of the different velocities and momentum densities appearing in the theory is clarified. Together with the unified equation of state published earlier, the present results provide consistent microscopic inputs for modeling superfluid neutron-star cores.


2000 ◽  
Vol 665 (1-2) ◽  
pp. 71-91 ◽  
Author(s):  
Javid A. Sheikh ◽  
Peter Ring

1996 ◽  
Vol 600 (3) ◽  
pp. 371-386 ◽  
Author(s):  
J. Terasaki ◽  
P.-H. Heenen ◽  
H. Flocard ◽  
P. Bonche

2006 ◽  
Vol 15 (02) ◽  
pp. 333-338 ◽  
Author(s):  
P. OLBRATOWSKI ◽  
J. DOBACZEWSKI ◽  
P. POWAŁOWSKI ◽  
M. SADZIAK ◽  
K. ZBERECKI

Hartree-Fock-Bogolyubov solutions corresponding to the tetrahedral deformation are found in six tetrahedrally doubly-magic nuclei. Values of the β32 deformation, depths of the tetrahedral minima, and their energies relative to the co-existing quadrupole minima are determined for several versions of the Skyrme force. Reduction of the tetrahedral deformation energies by pairing correlations is quantitatively analysed. In light nuclei, shallow tetrahedral minima are found to be the lowest in energy, while in heavy nuclei, the minima are deeper but appear at a few MeV of excitation.


1967 ◽  
Vol 153 (4) ◽  
pp. 1099-1107 ◽  
Author(s):  
J. Bar-Touv ◽  
C. A. Levinson
Keyword(s):  

1974 ◽  
Vol 52 (6) ◽  
pp. 541-553 ◽  
Author(s):  
W. Y. Ng ◽  
L. E. H. Trainor

The Hartree–Fock–Skyrme approach to calculations of the nuclear moment of inertia is generalized. It is shown that a different formula than the usual Skyrme formula can be expected to give better results. This result is illustrated by calculations on even–even nuclei in the sd shell.


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