corner
corner

Phys. Rev. A 81, 031611(R) (2010) [3 pages]

Experimental observation of magic-wavelength behavior of 87Rb atoms in an optical lattice

Download: PDF (149 kB) Buy this article Export: BibTeX or EndNote (RIS)

N. Lundblad1,2,*, M. Schlosser3, and J. V. Porto2
1Department of Physics & Astronomy, Bates College, Lewiston, Maine 04240, USA
2Joint Quantum Institute, National Institute of Standards and Technology and University of Maryland, Gaithersburg, Maryland 20899, USA
3Institut für Angewandte Physik, Technische Universität Darmstadt, Schlossgartenstraße 7, D-64289 Darmstadt, Germany

See Also: Publisher's Note

Received 8 December 2009; published 29 March 2010; corrected 13 April 2010

See accompanying Physics Synopsis

We demonstrate the cancellation of the differential ac Stark shift of the microwave hyperfine clock transition in trapped 87Rb atoms. Recent progress in metrology exploits so-called magic wavelengths, whereby an atomic ensemble can be trapped with laser light whose wavelength is chosen so that both levels of an optical atomic transition experience identical ac Stark shifts. Similar magic-wavelength techniques are not possible for the microwave hyperfine transitions in the alkali metals due to their simple electronic structure. We show, however, that ac Stark shift cancellation is indeed achievable for certain values of wavelength, polarization, and magnetic field. The cancellation comes at the expense of a small magnetic-field sensitivity. The technique demonstrated here has implications for experiments involving the precise control of optically trapped neutral atoms.

© 2010 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevA.81.031611
DOI:
10.1103/PhysRevA.81.031611
PACS:
67.85.Hj, 06.30.Ft, 32.10.Dk, 37.10.Jk

*nlundbla@bates.edu

See Also

Publisher's Note: N. Lundblad, M. Schlosser, and J. V. Porto, Publisher’s Note: Experimental observation of magic-wavelength behavior of 87Rb atoms in an optical lattice [Phys. Rev. A 81, 031611 (2010)], Phys. Rev. A 81, 049904 (2010).