Javascript must be enabled to continue!
Two-component relativistic methods for the heaviest elements
View through CrossRef
Different generalized Douglas-Kroll transformed Hamiltonians (DKn, n=1, 2,…,5) proposed recently by Hess et al. are investigated with respect to their performance in calculations of the spin–orbit splittings. The results are compared with those obtained in the exact infinite-order two-component (IOTC) formalism which is fully equivalent to the four-component Dirac approach. This is a comprehensive investigation of the ability of approximate DKn methods to correctly predict the spin–orbit splittings. On comparing the DKn results with the IOTC (Dirac) data one finds that the calculated spin–orbit splittings are systematically improved with the increasing order of the DK approximation. However, even the highest-order approximate two-component DK5 scheme shows certain deficiencies with respect to the treatment of the spin–orbit coupling terms in very heavy systems. The meaning of the removal of the spin-dependent terms in the so-called spin-free (scalar) relativistic methods for many-electron systems is discussed and a computational investigation of the performance of the spin-free DKn and IOTC methods for many-electron Hamiltonians is carried out. It is argued that the spin-free IOTC rather than the Dirac-Coulomb results give the appropriate reference for other spin-free schemes which are based on approximate two-component Hamiltonians. This is illustrated by calculations of spin-free DKn and IOTC total energies, r−1 expectation values, ionization potentials, and electron affinities of heavy atomic systems.
Title: Two-component relativistic methods for the heaviest elements
Description:
Different generalized Douglas-Kroll transformed Hamiltonians (DKn, n=1, 2,…,5) proposed recently by Hess et al.
are investigated with respect to their performance in calculations of the spin–orbit splittings.
The results are compared with those obtained in the exact infinite-order two-component (IOTC) formalism which is fully equivalent to the four-component Dirac approach.
This is a comprehensive investigation of the ability of approximate DKn methods to correctly predict the spin–orbit splittings.
On comparing the DKn results with the IOTC (Dirac) data one finds that the calculated spin–orbit splittings are systematically improved with the increasing order of the DK approximation.
However, even the highest-order approximate two-component DK5 scheme shows certain deficiencies with respect to the treatment of the spin–orbit coupling terms in very heavy systems.
The meaning of the removal of the spin-dependent terms in the so-called spin-free (scalar) relativistic methods for many-electron systems is discussed and a computational investigation of the performance of the spin-free DKn and IOTC methods for many-electron Hamiltonians is carried out.
It is argued that the spin-free IOTC rather than the Dirac-Coulomb results give the appropriate reference for other spin-free schemes which are based on approximate two-component Hamiltonians.
This is illustrated by calculations of spin-free DKn and IOTC total energies, r−1 expectation values, ionization potentials, and electron affinities of heavy atomic systems.
Related Results
Relativistic Hydrodynamics
Relativistic Hydrodynamics
AbstractThe book provides a lively and approachable introduction to the main concepts and techniques of relativistic hydrodynamics in a form which will appeal to physicists at adva...
The effective relativistic coupling by asymptotic representation approach for molecules with multiple relativistic atoms
The effective relativistic coupling by asymptotic representation approach for molecules with multiple relativistic atoms
The Effective Relativistic Coupling by Asymptotic Representation (ERCAR) approach is a method to generate fully coupled diabatic potential energy surfaces (PESs) including relativi...
Relativistic Milne-Eddington Type Solutions with a Variable Eddington Factor for Relativistic Spherical Winds
Relativistic Milne-Eddington Type Solutions with a Variable Eddington Factor for Relativistic Spherical Winds
Relativistic radiative transfer in a relativistic spherical flow is examined in the fully special relativistic treatment. Under the assumption of a constant flow speed and using a ...
Artificial Neural Network Approach versus Analytical Solutions for Relativistic Polytropes
Artificial Neural Network Approach versus Analytical Solutions for Relativistic Polytropes
Abstract
Over the last few decades, artificial neural networks (ANN) have played an important role in many areas of human activity and have found application in many branch...
Fundamental Notions in Relativistic Geodesy - physics of a timelike Killing vector field
Fundamental Notions in Relativistic Geodesy - physics of a timelike Killing vector field
<p>The Earth&#8217;s geoid is one of the most important fundamental concepts to provide a gravity field- related height reference in geodesy and associated sc...
Reply to Comment on ‘Bulk properties of nuclear matter in a modified relativistic Dirac formalism’
Reply to Comment on ‘Bulk properties of nuclear matter in a modified relativistic Dirac formalism’
Abstract
We sincerely thank the Editorial Board for forwarding the comments regarding our published paper [Panda
et al
...
Geodetic Precession of the Sun, Solar System Planets, and their Satellites
Geodetic Precession of the Sun, Solar System Planets, and their Satellites
Abstract
The effect of the geodetic precession is the most significant relativistic effect in the rotation of celestial bodies. In this article, the new geodetic pre...
Relativistic electronic structure studies on the heaviest elements
Relativistic electronic structure studies on the heaviest elements
AbstractSpectacular developments in relativistic quantum theory and computational algorithms in the last two decades allowed for accurate predictions of properties of the heaviest ...

