Application of the correlated B-spline basis functions to the leading relativistic and QED corrections of helium

TL;DR

This paper extends correlated B-spline basis functions to accurately compute leading relativistic and QED corrections in helium energy levels, demonstrating consistency with previous results and enabling higher-order effect calculations.

Contribution

The study introduces the application of correlated B-spline basis functions to relativistic and QED correction calculations for helium, enhancing computational accuracy and potential for higher-order effects.

Findings

Accurate calculation of relativistic and QED corrections for helium energy levels.

Results are consistent with previous high-precision calculations.

Method shows promise for higher-order correction computations.

Abstract

B-spline functions have been widely used in computational atomic physics. Different from the traditional B-spline basis (a simple product of two B-splines), the recently developed correlated B-spline basis functions(C-BSBF), in which the interelectronic coordinate $r_{12}$ is included explicitly, have greatly improved the computational accuracy of polarizability [S. J. Yang \textit{et al}., Phys. Rev. A \textbf{95}, 062505 (2017)] and bethe logarithm [ S. J. Yang \textit{et al}., Phys. Rev. A \textbf{100}, 042509 (2019)] for singlet states of helium. Here, we report the extension of the C-BSBF to the leading relativistic and QED correction calculations for energy levels of the $1\,^1S$, $2\,^1S$, $2\,^3S$, and $3\,^3S$ states of helium. The relativistic kinetic term $p_{1}^{4}$, contact potential $\delta^{3}(r_{1})$, $\delta^{3}(r_{12})$ and Araki-Sucher correction $\langle 1/r_{12}^{3} \rangle$ are calculated by using the global operator method, in which $r_{12}^n$ and $r_{12}^n\ln r_{12}$ involved are calculated with the generalization of Laplace's expansions. The obtained values for the ground state are $\delta E_{rel}/\alpha ^{2}=-$1.951 754 7(2) and $\delta E_{QED}/\alpha^{3}=$57.288 165(2), consistent with previous results, which opens the possibility of calculating higher-order relativistic and QED effects using the C-BSBF.