Abstract:The model-QED-operator approach [Phys. Rev. A 88, 012513 (2013)] to calculations of the radiative corrections to binding and transition energies in atomic systems is extended to the range of nuclear charges 110 Z 170. The self-energy part of the model operator is represented by a nonlocal potential based on diagonal and off-diagonal matrix elements of the ab initio self-energy operator with the Dirac-Coulomb wave functions. The vacuum-polarization part consists of the Uehling contribution which is readily comp… Show more
“…Reference [383] contains the values of F (1) n,κ (Zα) for nd 3/2 to ng 9/2 up to n = 5 for a point nucleus. The finite size of correction for 2s states and 2p 1/2 states can be found in [142,143,378] for 26 ≤ Z ≤ 100, for 10 ≤ Z ≤ 120 in [68] and for 100 ≤ Z ≤ 170 in [340]. The comparison between different theoretical values with and without finite size correction for 2s, 2p 1/2 and 2p 3/2 states is shown in Fig.…”
Section: A Comparison Between the Different Values Of Fmentioning
confidence: 91%
“…It was followed by the calculation of the self-energy contribution of the 1s 1/2 level for finite nuclei up to Z = 170 [339]. This evaluation has recently been extended to all states up to n = 5 and J = 5/2 [340]. The method described in Ref.…”
Section: Quantum Electrodynamic Effectsmentioning
confidence: 99%
“…The work from Ref. [68] has been extended recently to Z = 170 [340]. In both works, the selfenergy for a given Z value is calculated for a specific nuclear size, using the Fermi model.…”
“…The Welton approximation [414] was introduced in the MDFGME code in 1987 [65] for s-states and generalized to ≥ 0 in [66]. Effective operators directly based on BSQED have been introduced more recently [68,340].…”
Section: Effective Qed Hamiltoniansmentioning
confidence: 99%
“…A recent extension to superheavy elements up to nuclear charge Z = 170 has been carried out in Ref. [340]. This scheme gives very accurate results for the self-energy.…”
We review the progress in atomic structure theory with a focus on superheavy elements and the aim to predict their ground state configuration and element's placement in the periodic table. To understand the electronic structure and correlations in the regime of large atomic numbers, it is important to correctly solve the Dirac equation in strong Coulomb fields, and also to take into account quantum electrodynamic effects. We specifically focus on the fundamental difficulties encountered when dealing with the many-particle Dirac equation. We further discuss the possibility for future many-electron atomic structure calculations going beyond the critical nuclear charge Z crit ≈ 170, where levels such as the 1s shell dive into the negative energy continuum (E nκ < −m e c 2 ). The nature of the resulting Gamow states within a rigged Hilbert space formalism is highlighted.* Here we define the starting point of the superheavy element region at the transactinides, Z ≥ 103
“…Reference [383] contains the values of F (1) n,κ (Zα) for nd 3/2 to ng 9/2 up to n = 5 for a point nucleus. The finite size of correction for 2s states and 2p 1/2 states can be found in [142,143,378] for 26 ≤ Z ≤ 100, for 10 ≤ Z ≤ 120 in [68] and for 100 ≤ Z ≤ 170 in [340]. The comparison between different theoretical values with and without finite size correction for 2s, 2p 1/2 and 2p 3/2 states is shown in Fig.…”
Section: A Comparison Between the Different Values Of Fmentioning
confidence: 91%
“…It was followed by the calculation of the self-energy contribution of the 1s 1/2 level for finite nuclei up to Z = 170 [339]. This evaluation has recently been extended to all states up to n = 5 and J = 5/2 [340]. The method described in Ref.…”
Section: Quantum Electrodynamic Effectsmentioning
confidence: 99%
“…The work from Ref. [68] has been extended recently to Z = 170 [340]. In both works, the selfenergy for a given Z value is calculated for a specific nuclear size, using the Fermi model.…”
“…The Welton approximation [414] was introduced in the MDFGME code in 1987 [65] for s-states and generalized to ≥ 0 in [66]. Effective operators directly based on BSQED have been introduced more recently [68,340].…”
Section: Effective Qed Hamiltoniansmentioning
confidence: 99%
“…A recent extension to superheavy elements up to nuclear charge Z = 170 has been carried out in Ref. [340]. This scheme gives very accurate results for the self-energy.…”
We review the progress in atomic structure theory with a focus on superheavy elements and the aim to predict their ground state configuration and element's placement in the periodic table. To understand the electronic structure and correlations in the regime of large atomic numbers, it is important to correctly solve the Dirac equation in strong Coulomb fields, and also to take into account quantum electrodynamic effects. We specifically focus on the fundamental difficulties encountered when dealing with the many-particle Dirac equation. We further discuss the possibility for future many-electron atomic structure calculations going beyond the critical nuclear charge Z crit ≈ 170, where levels such as the 1s shell dive into the negative energy continuum (E nκ < −m e c 2 ). The nature of the resulting Gamow states within a rigged Hilbert space formalism is highlighted.* Here we define the starting point of the superheavy element region at the transactinides, Z ≥ 103
A simple procedure to incorporate one‐loop quantum electrodynamic (QED) corrections into the generalized (Gatchina) nonlocal shape‐consistent relativistic pseudopotential model is described. The pseudopotentials for Lu, Tl, and Ra replacing only inner core shells (with principal quantum numbers n ≤ 3 for the two former elements and n ≤ 4 for the latter one) are derived from the solutions of reference atomic SCF problems with the Dirac–Coulomb–Breit Hamiltonian to which the model Lamb shift operator added. QED contributions to atomic valence excitation energies evaluated at the SCF level are demonstrated to exceed the errors introduced by the pseudopotential approximation itself by an order of magnitude. Pilot applications of the new model to calculations of excitation energies of two‐valence‐electron atomic systems using the intermediate‐Hamiltonian relativistic Fock space coupled cluster method reformulated here for incomplete main model spaces are reported. Implications for high‐accuracy molecular excited state calculations are discussed.
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