scholarly journals Finite-temperature mean-field approximations for shell model Hamiltonians: the code HF-SHELL

2021 ◽  
Vol 57 (2) ◽  
Author(s):  
W. Ryssens ◽  
Y. Alhassid
1992 ◽  
Vol 277 (1-2) ◽  
pp. 18-22 ◽  
Author(s):  
R. Rossignoli ◽  
R.M. Quick ◽  
H.G. Miller

1993 ◽  
Vol 71 (5-6) ◽  
pp. 285-294
Author(s):  
M. H. Thoma

Various mean field approximations at finite temperature are used for calculating ground state energies and propagators of the [Formula: see text] theory in two dimensions and quantum chromodynamics (QCD). In the case of the [Formula: see text] theory a symmetry restoration is observed above a critical coupling constant if a temperature independent renormalization is used. In the case of QCD the mean field approximation is insufficient but can be regarded as a starting point for more complicated approximations, which are discussed qualitatively.


2006 ◽  
Vol 15 (08) ◽  
pp. 1695-1709 ◽  
Author(s):  
YANG SUN

Performing shell model calculations for heavy nuclei is a long-standing problem in nuclear physics. The shell model truncation in the configuration space is an unavoidable step. The Projected Shell Model (PSM) truncates the space under the guidance of the deformed mean-field solutions. This implies that the PSM uses a novel and efficient way to bridge the two conventional methods: the deformed mean-field approximations, which are widely applied to heavy nuclei but able to describe the physics only in the intrinsic frame, and the spherical shell model diagonalization method, which is most fundamental but feasible only for small systems. We discuss the basic philosophy in construction of the PSM (or generally PSM-like) approach. Several examples from the PSM calculations are presented. Astrophysical applications are emphasized.


1995 ◽  
Vol 591 (1) ◽  
pp. 15-40 ◽  
Author(s):  
R. Rossignoli ◽  
N. Canosa ◽  
P. Ring

1994 ◽  
Vol 570 (1-2) ◽  
pp. 217-224 ◽  
Author(s):  
H.G. Miller ◽  
R.M. Quick ◽  
R.R. Rossignoli ◽  
G.D. Yen

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