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PreprintCC BY 4.0arXiv

Sympathetic Cooling of Ionic Fullerenes with Ultracold Atoms to Millikelvin Temperatures

Abstract

Cooling complex molecular ions to millikelvin temperatures remains a major challenge because their intricate internal structures prevent laser cooling. Here, we propose to use an ultracold gas of Cd atoms to efficiently cool C60+ ions to average kinetic energies of approximately 20 mK, following an initial precooling stage with He buffer gas. Our approach is based on full molecular dynamics simulations using accurate ion-atom interaction potentials derived from high-level electronic structure methods. Furthermore, using a Monte Carlo approach, we predict the formation of C60+ Coulomb crystals supported solely by collisions with the buffer gas. The probability of reaching these cold states shows a pronounced dependence on the number of trapped ions, revealing the competition between neutral-atom cooling and many-ion dynamics in radio-frequency traps.

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BibTeX
@misc{chowdhury2026sympathetic,
  title = {{Sympathetic Cooling of Ionic Fullerenes with Ultracold Atoms to Millikelvin Temperatures}},
  author = {Saajid Chowdhury and Zhongqi Liang and Yu Wang and Jesús Pérez-Ríos},
  howpublished = {arXiv},
  year = {2026},
  month = nov,
  doi = {10.48550/arxiv.2611.05815},
  eprint = {2611.05815},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2611.05815},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Sympathetic Cooling of Ionic Fullerenes with Ultracold Atoms to Millikelvin Temperatures
AU  - Saajid Chowdhury
AU  - Zhongqi Liang
AU  - Yu Wang
AU  - Jesús Pérez-Ríos
PY  - 2026
DA  - 2026/11/04
PB  - arXiv
DO  - 10.48550/arxiv.2611.05815
UR  - https://arxiv.org/abs/2611.05815
AB  - Cooling complex molecular ions to millikelvin temperatures remains a major challenge because their intricate internal structures prevent laser cooling. Here, we propose to use an ultracold gas of Cd atoms to efficiently cool C_60^+ ions to average kinetic energies of approximately 20 mK, following an initial precooling stage with He buffer gas. Our approach is based on full molecular dynamics simulations using accurate ion-atom interaction potentials derived from high-level electronic structure methods. Furthermore, using a Monte Carlo approach, we predict the formation of C_60^+ Coulomb crystals supported solely by collisions with the buffer gas. The probability of reaching these cold states shows a pronounced dependence on the number of trapped ions, revealing the competition between neutral-atom cooling and many-ion dynamics in radio-frequency traps.
ER  -