Pseudo-spin–orbit potential in the relativistic Hartree–Fock formalism

2003 ◽  
Vol 727 (3-4) ◽  
pp. 269-298 ◽  
Author(s):  
M. López-Quelle ◽  
L.N. Savushkin ◽  
S. Marcos ◽  
P. Bernardos ◽  
R. Niembro
2001 ◽  
Author(s):  
M. LÓPEZ-QUELLE ◽  
L. N. SAVUSHKIN ◽  
S. MARCOS ◽  
P. BERNARDOS

2005 ◽  
Vol 14 (03) ◽  
pp. 451-456 ◽  
Author(s):  
H. ZDUŃCZUK ◽  
W. SATUŁA ◽  
R. A. WYSS

A systematic study of the terminating states in A~50 mass region using the self-consistent Skyrme-Hartree-Fock model is presented. The objective is to use the intrinsic simplicity of the terminating states to constrain certain parameters of the local nuclear energy functional. In particular, the work focuses on the spin fields and the spin-orbit term and constrain the appropriate Landau parameters and the strength of the spin-orbit potential.


1960 ◽  
Vol 76 (6) ◽  
pp. 1002-1002
Author(s):  
D W L Sprung ◽  
J B Willis

2018 ◽  
Vol 25 (3) ◽  
pp. 899-905 ◽  
Author(s):  
Patric Zimmermann ◽  
Robert J. Green ◽  
Maurits W. Haverkort ◽  
Frank M. F. de Groot

Some initial instructions for theQuanty4RIXSprogram written in MATLAB®are provided. The program assists in the calculation of 1s 2p RIXS and 1s 2p RIXS–MCD spectra usingQuanty. Furthermore, 1s XAS and 2p 3d RIXS calculations in different symmetries can also be performed. It includes the Hartree–Fock values for the Slater integrals and spin–orbit interactions for several 3dtransition metal ions that are required to create the .lua scripts containing all necessary parameters and quantum mechanical definitions for the calculations. The program can be used free of charge and is designed to allow for further adjustments of the scripts.


Atoms ◽  
2020 ◽  
Vol 8 (4) ◽  
pp. 67
Author(s):  
Stéphane Carniato ◽  
Jean-Marc Bizau ◽  
Denis Cubaynes ◽  
Eugene T. Kennedy ◽  
Ségolène Guilbaud ◽  
...  

This article presents N2+ fragment yields following nitrogen K-shell photo-absorption in the NH+ molecular ion measured at the SOLEIL synchrotron radiation facility in the photon energy region 390–450 eV. The combination of the high sensitivity of the merged-beam, multi-analysis ion apparatus (MAIA) with the high spectral resolution of the PLEIADES beamline helped to resolve experimentally vibrational structures of highly excited [N1s−1H]*+ electronic states with closed or open-shell configurations. The assignment of the observed spectral features was achieved with the help of density functional theory (DFT) and post-Hartree Fock Multiconfiguration Self-Consistent-Field/Configuration Interaction (MCSCF/CI) ab-initio theoretical calculations of the N1s core-to-valence and core-to-Rydberg excitations, including vibrational dynamics. New resonances were identified compared to previous work, owing to detailed molecular modeling of the vibrational, spin-orbit coupling and metastable state effects on the spectra. The latter are evidenced by spectral contributions from the 4Σ− electronic state which lies 0.07 eV above the NH+2Π ground state.


2019 ◽  
Vol 28 (09) ◽  
pp. 1950074
Author(s):  
Zakaria M. M. Mahmoud ◽  
Awad A. Ibraheem ◽  
M. A. Hassanain

In this work, we simultaneously reanalyzed the differential elastic scattering cross-sections ([Formula: see text]) and the vector analyzing power ([Formula: see text]) of [Formula: see text]He elastic scattering. This analysis was performed using the folded optical model for both real central and spin-orbit (SO) potentials, respectively. For the imaginary central, we used the usual Woods-Saxon (WS) form. Three different model density distributions are used to calculate the potential. We aimed to examine the applicability of the microscopically derived SO potential and the structure effect of 6He nucleus. The presence of the [Formula: see text] experimental data of [Formula: see text]He makes it interesting for this study. Our calculations showed that the three densities gave similar predictions for the cross-sections data. The three microscopic SO potentials calculations of [Formula: see text] are not in a good agreement with the experimental data. We concluded that the SO formalism in its current form needs more investigations for exotic halo nuclei.


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