Rotational excitation in sympathetic cooling of diatomic molecular ions by laser-cooled atomic ions
J. Martin Berglund, Michael Drewsen, Christiane P. Koch
TL;DR
This work investigates whether rotational excitations induced by Coulomb coupling during sympathetic cooling degrade internal-state purity of diatomic molecular ions. It develops a framework separating translational and rotational dynamics, modeling translational cooling for two setups—a single atomic ion and a Coulomb crystal—via classical 1/r scattering and impact-parameter averaging, to estimate energy transfer per collision and cooling times. For rotational dynamics, apolar and polar diatomic ions are treated with perturbative and adiabatic approaches, respectively, yielding closed-form estimates for apolar accumulated excitation and adiabatic bounds for polar cases; in many practical scenarios, apolar ions experience only modest rotation, whereas polar ions require careful handling depending on dipole moment and collision energy. The results offer actionable guidance for trap-depth and ion selection to preserve rotational state during cooling and point to broader applicability to polyatomic species, where rotational structure may pose greater challenges.
Abstract
Sympathetic cooling of molecular ions through the Coulomb interaction with laser-cooled atomic ions is an efficient tool to prepare translationally cold molecules without, ideally, affecting the internal state of the molecular ions. However, the electric field due to the Coulomb interaction may induce rotational transitions that change the purity of initially quantum state prepared molecules. Here, we use estimates of rotational state changes in single collisions of diatomic ions with atomic ions [arXiv:1905.02130] to determine the overall rotational excitation accumulated over the sympathetic cooling. Considering two different experimental scenarios, that of a molecular ion co-trapped with a single atomic ion and a molecular ion immersed in a Coulomb crystal of atomic ions, we also estimate the cooling time.
