Direct Excitation of the Forbidden Clock Transition in Neutral 174Yb Atoms Confined to an Optical Lattice
Creators
- 1. Institute of Laser Physics SB RAS, Novosibirsk 630090 (Russian Federation) and Novosibirsk State University, Novosibirsk 630090 (Russian Federation)
- 2. National Institute of Standards and Technology, 325 Broadway, Boulder, Colorado 80305 (United States)
Description
We report direct single-laser excitation of the strictly forbidden (6s2)1S0↔(6s6p)3P0 clock transition in 174Yb atoms confined to a 1D optical lattice. A small (∼1.2 mT) static magnetic field was used to induce a nonzero electric dipole transition probability between the clock states at 578.42 nm. Narrow resonance linewidths of 20 Hz (FWHM) with high contrast were observed, demonstrating a resonance quality factor of 2.6x1013. The previously unknown ac Stark shift-canceling (magic) wavelength was determined to be 759.35±0.02 nm. This method for using the metrologically superior even isotope can be easily implemented in current Yb and Sr lattice clocks and can create new clock possibilities in other alkaline-earth-like atoms such as Mg and Ca
Additional details
Identifiers
- DOI
- 10.1103/PhysRevLett.96.083002;
- arXiv
- arXiv:physics/0512084v2;
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 96
- Journal Issue
- 8
- Journal Page Range
- p. 083002-083002.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37083022
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS;
- Descriptors DEI
- ATOMIC CLOCKS; ATOMS; COOLING; E1-TRANSITIONS; EXCITATION; LASERS; LIFETIME; LINE WIDTHS; MAGNETIC FIELDS; PROBABILITY; QUALITY FACTOR; RESONANCE; STARK EFFECT; WAVELENGTHS; YTTERBIUM 174
- Descriptors DEC
- DIMENSIONLESS NUMBERS; ENERGY-LEVEL TRANSITIONS; EVEN-EVEN NUCLEI; INTERMEDIATE MASS NUCLEI; ISOTOPES; MULTIPOLE TRANSITIONS; NUCLEI; RARE EARTH NUCLEI; STABLE ISOTOPES; YTTERBIUM ISOTOPES
Optional Information
- Notes
- (c) 2006 American Institute of Physics