10–14 Jun 2024
ETH Zurich- Hönggerberg Campus
Europe/Zurich timezone

Towards the self-energy correction of the no-pair Dirac$-$Coulomb energy for two-electron systems

10 Jun 2024, 18:00
2h
ETH Zurich- Hönggerberg Campus

ETH Zurich- Hönggerberg Campus

Speaker

Adam Margocsy (ELTE, Budapest)

Description

Among the leading Quantum Electrodynamical (QED) corrections to atomic-molecular energy levels, the effect of one-loop electron self-energy has proven to be one of the most challenging to compute.
There are well-established techniques to calculate it in two extreme cases (for predominantly non-relativistic[1] and highly relativistic[2] systems, like low-charged and highly charged ions, respectively), but no general method to a correlated relativistic reference state is known.

Finding a self-energy calculating approach generally applicable regardless of the strength of relativistic effects is part of our ongoing research effort to build QED corrections on highly accurate relativistic two-particle wave functions[3]. Our starting point is the equal-time formulation of the Bethe$-$Salpeter equation[4], and its first approximation, the no-pair Dirac$-$Coulomb($-$Breit) equation; radiative and non-radiative QED corrections are then included perturbatively.

In my poster, I present our current progress towards the calculation of self-energy with a relativistic two-electron wave function. The reference is a no-pair Dirac$-$Coulomb wave function obtained from an explicitly correlated variational procedure, providing an all-order description of (instantaneous, non-radiative) relativistic effects[5].
Working in the framework of the dipole approximation while using such a reference leads to a simple relativistic extension of the so-called Bethe logarithm, and endows the low-frequency part of the self-energy (plus transverse photon exchange) with higher-order binding corrections[3]. An example calculation is given for the ground state of the helium atom.
Moving beyond the dipole approximation raises several questions concerning the renormalization, the role of negative-energy states and permutational symmetry issues of inner states. A fully numerical renormalization scheme is proposed, reminiscent of partial wave renormalization[2]. The new challenges and obstacles associated with the relativistic treatment of self energy beyond the dipole approximation are discussed, with preliminary numerical results.

References

[1] Schwartz: Phys. Rev. 123 1700 (1961)
Pachucki: J. Phys. B: At. Mol. Opt. Phys. 31 5123 (1998)
Korobov: Phys. Rev. A 100 012517 (2019)
Ferenc, Mátyus: J. Phys. Chem. A 127 3 627 (2023)

[2] Lindgren, Persson, Salomonson, Ynnerman: Phys. Rev. A 47 R4555 (1993)
Grant, Quiney: Atoms 10 108 (2022)

[3] Mátyus, Ferenc, Jeszenszki, Margócsy: ACS Phys. Chem. Au 3 3 222 (2023)
Margócsy, Mátyus: arXiV 2312.13887 (2023)

[4] Salpeter: Phys. Rev. 87 328 (1952)
Sucher: PhD Thesis, Columbia University (1958)

[5] Ferenc, Jeszenszki, Mátyus: J. Chem. Phys. 157 094113 (2022)
Jeszenszki, Ferenc, Mátyus: J. Chem. Phys. 165 084111 (2022)

Authors

Adam Margocsy (ELTE, Budapest) Prof. Edit Matyus (ELTE, Eotvos Lorand University)

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