National Physical Laboratory

Optical Frequency Standards & Metrology

New types of atomic clock operating at optical rather than microwave frequencies promise significant advances in both science and technology.

All other things being equal, the stability of an atomic clock is proportional to its operating frequency. Visible light has a frequency roughly 100 000 times higher than that of microwaves. This means that clocks based on narrow absorptions at optical, rather than microwave, frequencies should be much more stable.

Optical clocks have many potential applications. These range from improved satellite navigation systems and better tracking of deep space probes to sensitive tests of general relativity and measurements of fundamental physical constants. In future they could even lead to the SI unit of time, the second, being redefined.

The heart of an optical clock is a highly stable reference frequency provided by a narrow optical absorption in an atom or ion. At NPL we are developing clocks based on transitions in single trapped ions and neutral atoms confined in an optical lattice.

  • The SI unit of length is the metre. Since 1983 the metre has been defined as “the length of the path travelled by light in vacuum during a time interval of 1/299 792 458 of a second.”
  • The most accurate optical frequency measurements are limited by the caesium primary standard itself, raising the prospect of an optical redefinition of the second in the future.