Strong magnetic fields
such as those found on white dwarfs have
significant effects on the electronic structures of atoms and molecules.
However, the vast majority of molecular studies in the literature
in such fields are carried out with Gaussian basis sets designed for
zero field, leading to large basis set truncation errors [Lehtola
et al.,
Mol. Phys
.
2020
,
118
, e1597989]. In this work, we aim to identify the failures of the
Gaussian basis sets in atomic calculations to guide the design of
new basis sets for strong magnetic fields. We achieve this by performing
fully numerical electronic structure calculations at the complete
basis set (CBS) limit for the ground state and low lying excited states
of the atoms 1 ≤
Z
≤ 18 in weak to
intermediate magnetic fields. We also carry out finite-field calculations
for a variety of Gaussian basis sets, introducing a real-orbital approximation
for the magnetic-field Hamiltonian. Our primary focus is on the aug-cc-pVTZ
basis set, which has been used in many works in the literature. A
study of the differences in total energies of the fully numerical
CBS limit calculations and the approximate Gaussian basis calculations
is carried out to provide insight into basis set truncation errors.
Examining a variety of states over the range of magnetic field strengths
from
B
= 0 to
B
= 0.6
B
0
, we observe significant differences for the aug-cc-pVTZ
basis set, while much smaller errors are afforded by the benchmark-quality
AHGBSP3-9 basis set [Lehtola,
J. Chem. Phys
.
2020
,
152
, 134108]. This suggests that there
is considerable room to improve Gaussian basis sets for calculations
at finite magnetic fields.