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NIST-F2

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NIST-F2
NIST-F2
National Institute of Standards and Technology - Physics Laboratory: Time and Fr · Public domain · source
NameNIST-F2
CaptionCesium fountain primary frequency standard at NIST
MakerNational Institute of Standards and Technology
Introduced2014
TypeAtomic fountain clock
Frequency9,192,631,770 Hz (hyperfine transition)
Uncertainty1.1×10−16 (systematic)

NIST-F2 NIST-F2 is a primary cesium fountain atomic clock developed by the National Institute of Standards and Technology for realization of the SI second and timekeeping at the United States Naval Observatory and international time scales such as Coordinated Universal Time. It serves as a laboratory frequency standard alongside devices at institutions like the Physikalisch-Technische Bundesanstalt, the Bureau International des Poids et Mesures, and the National Physical Laboratory (United Kingdom), contributing to comparisons with standards at Time and Frequency Division, NIST, European Space Agency, and National Research Council (Canada). The clock influences technologies supported by agencies and companies such as NASA, European Organisation for Nuclear Research, Google, and IBM.

Overview

NIST-F2 operates as a cesium fountain using cold atoms launched in an optical molasses prepared by methods pioneered at Bell Labs, Massachusetts Institute of Technology, and Stanford University; the device builds on prior primary standards including those from NIST, PTB, and LNE-SYRTE. It realizes the hyperfine transition of the cesium-133 atom defined in the SI system and participates in international timekeeping via contributions to BIPM reports, International Atomic Time, and the International Committee for Weights and Measures. Laboratories such as NPL, METAS, VNIIFTRI, and KRISS perform intercomparisons using techniques like two-way satellite time and frequency transfer developed with partners including USNO and ESA.

Design and Technical Specifications

NIST-F2's architecture incorporates a vacuum chamber, magnetically shielded interrogation region, and microwave cavity designed in collaboration with teams from NIST, JILA, and Harvard University. The fountain employs laser cooling with diode lasers influenced by work at Bell Labs and University of Colorado Boulder, optical components from groups at Caltech and University of Oxford, and microwave synthesis referenced to hydrogen masers similar to designs used at MIT and Yale University. Its systematic uncertainty budget includes shifts first analyzed by researchers at PTB, LNE-SYRTE, NPL, and BIPM, covering blackbody radiation, collisional shifts, microwave lensing, and Zeeman effects studied in publications from PhysRevLett, Nature, and Physical Review A.

Calibration and Performance

Calibration procedures for NIST-F2 align with protocols issued by BIPM, CIPM, and committees including the CCM; intercomparisons employ time transfer methods developed by USNO, NIST, and ESA using carriers like GLONASS, Galileo, and GPS signals analyzed with algorithms from NIST and NPL. Performance metrics—Allan deviation, stability, and accuracy—are reported in papers coauthored with researchers from JILA, PTB, LNE-SYRTE, and NRC and benchmarked against hydrogen masers at USNO and optical clocks at NIST and JILA. Reported uncertainties reference collaborative studies involving National Institute of Standards and Technology, BIPM, METAS, and KRISS showing systematic uncertainty on the order of 1×10−16 and demonstrated operational stability across campaigns documented with software from IEEE and data archives at NIST.

Applications and Uses

NIST-F2 underpins realization of the SI second employed by dissemination systems at USNO, BIPM, and national laboratories such as NPL, PTB, and NRCan for timekeeping in telecommunications by companies including AT&T, Verizon, and Deutsche Telekom. It supports fundamental physics tests conducted with teams at Harvard, MIT, Stanford, and Max Planck Institute exploring temporal variation of constants, searches for dark matter with collaborations linked to CERN and LIGO, and precision spectroscopy efforts in partnership with NIST and JILA. NIST-F2’s outputs assist navigation systems like GPS and scientific missions at NASA Jet Propulsion Laboratory, ESA, and NOAA while contributing to metrology services used by IEEE and standards bodies such as IEC.

History and Development

Development of NIST-F2 traces to earlier cesium fountain projects at NIST and international efforts at PTB and LNE-SYRTE building on laser cooling breakthroughs by teams at Bell Labs, MIT, and Stanford. Key milestones include construction and commissioning at NIST with collaborative input from JILA, validation campaigns compared against primary standards at BIPM and USNO, and publications in journals like Physical Review Letters and Metrologia. Funding and program oversight involved agencies and institutions including Department of Commerce, NIST, and collaborations with academic groups at University of Colorado, Harvard University, and University of Maryland.

Controversies and Criticisms

Critiques of NIST-F2 center on comparative cost and complexity versus emerging optical clocks developed at NIST, JILA, PTB, and NIST Boulder, and debates within panels convened by BIPM and CIPM about the roadmap for redefining the second. Stakeholders including representatives from USNO, NIST, BIPM, and national laboratories such as NPL and PTB have discussed uncertainties, reproducibility, and allocation of resources between microwave and optical primary standards in technical meetings influenced by publications in Nature and Science.

Category:Atomic clocks