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Published on: May 3, 2019
Blackbody radiation shifts in optical atomic clocks
Marianna Safronova1, Mikhail Kozlov, Charles Clark
1Department of Physics and Astronomy, University of Delaware, Newark, DE, USA. msafrono@udel.edu
Theoretical calculations of blackbody radiation (BBR) shifts in optical atomic clocks have been reviewed. New methods improve accuracy for divalent atoms, reducing uncertainties in B+ and In+ clocks to 10-18.
Area of Science:
- Atomic Physics
- Quantum Optics
- Theoretical Chemistry
Background:
- Optical atomic clocks are crucial for precise timekeeping and fundamental physics tests.
- Blackbody radiation (BBR) shifts are a significant source of uncertainty in optical clock frequencies.
- Accurate theoretical calculations are needed to minimize BBR shift effects.
Purpose of the Study:
- To review recent theoretical calculations of BBR shifts in optical atomic clocks.
- To present a new method for calculating BBR shifts in divalent atoms.
- To reduce uncertainties in atomic clock frequencies caused by BBR.
Main Methods:
- Review of relativistic all-order single-double (SD) method for monovalent ions.
- Development of a combined relativistic all-order and configuration interaction (CI) method for divalent atoms.
- Application of these methods to calculate BBR shifts in B+, Al+, and In+.
Main Results:
- Fractional uncertainties reduced to 4 × 10-19 for Al+ and 10-18 for B+ and In+ at room temperature.
- Calculated BBR shifts approach the precision limits of current optical atomic clock designs.
- The new method accurately treats correlation corrections in divalent atoms.
Conclusions:
- Theoretical advancements significantly reduce BBR shift uncertainties in optical clocks.
- The developed methods are vital for achieving next-generation atomic clock precision.
- Future work will focus on further reducing clock uncertainties from BBR shifts.
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