1. PHARAO : le premier étalon primaire de fréquence, à atomes froids, spatial
- Author
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Isabelle Zenone, S. Leon, T. Potier, Christophe Salomon, J.F. Vega, Ch. Macé, S. Julien, A. Ratsimandresy, Ch.M. de Graeve, Michel Abgrall, Ch. Delaroche, Pierre Lemonde, F. Gonzalez, Didier Massonnet, M. Chaubet, C. Luitot, Ph. Guillemot, O. Grosjean, D. Blonde, J. Guéna, Y. Cossart, F. Picard, B. Vivian, M. Aubourg, Ph. Larivière, J.-P. Granier, André Clairon, A. Granget, J. P. Lelay, Stéphane Thomin, Ph. Chatard, Giorgio Santarelli, Th. Nauleau, Muriel Saccoccio, Benoit Faure, S. Bize, Ph. Laurent, D. Rovera, Fabrice Buffe, N. Ladiette, B. Leger, I. Moric, Ch. Sirmain, S. Béraud, C. Escandes, Institut des Biomolécules Max Mousseron [Pôle Chimie Balard] (IBMM), Ecole Nationale Supérieure de Chimie de Montpellier (ENSCM)-Institut de Chimie du CNRS (INC)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Laboratoire national de métrologie et d'essais - Systèmes de Référence Temps-Espace (LNE - SYRTE), Systèmes de Référence Temps Espace (SYRTE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Spectroscopie Hertzienne de l'ENS (LSH-ENS), École normale supérieure - Paris (ENS-PSL), Joint ALMA Observatory (JAO), European Southern Observatory (ESO)-National Radio Astronomy Observatory (NRAO), Centre National d'Études Spatiales [Toulouse] (CNES), UCCS Équipe Catalyse Supramoléculaire, Unité de Catalyse et Chimie du Solide - UMR 8181 (UCCS), Université d'Artois (UA)-Centrale Lille-Institut de Chimie du CNRS (INC)-Université de Lille-Centre National de la Recherche Scientifique (CNRS)-Université d'Artois (UA)-Centrale Lille-Institut de Chimie du CNRS (INC)-Université de Lille-Centre National de la Recherche Scientifique (CNRS), Régulations cellulaires et oncogenèse (RCO), Institut Curie [Paris]-Centre National de la Recherche Scientifique (CNRS), CEA-Direction des Energies (ex-Direction de l'Energie Nucléaire) (CEA-DES (ex-DEN)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), École normale supérieure - Paris (ENS Paris), Centrale Lille Institut (CLIL)-Université d'Artois (UA)-Centrale Lille-Centre National de la Recherche Scientifique (CNRS)-Institut de Chimie du CNRS (INC)-Université de Lille-Centrale Lille Institut (CLIL)-Université d'Artois (UA)-Centrale Lille-Centre National de la Recherche Scientifique (CNRS)-Institut de Chimie du CNRS (INC)-Université de Lille, CNRS UMR 146 - Institut Curie - Developmental Genetics of Melanocytes (CNRS), and Centre National de la Recherche Scientifique (CNRS)
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Physics ,[PHYS]Physics [physics] ,business.industry ,Clock signal ,General Medicine ,Frequency standard ,Mean frequency ,01 natural sciences ,7. Clean energy ,010309 optics ,Optics ,0103 physical sciences ,Fundamental physics ,External field ,010306 general physics ,business ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,Hyperfine structure ,Fabry–Pérot interferometer ,Order of magnitude ,ComputingMilieux_MISCELLANEOUS - Abstract
CNES, LKB and SYRTE are developing a primary frequency standard, called PHARAO, which is specially designed for space applications. The clock signal is referenced on the frequency measurement of the hyperfine transition performed on a cloud of cold cesium PHARAO : LE PREMIER ETALON PRIMAIRE DE FREQUENCE, A ATOMES FROIDS, SPATIAL 3 atoms (∼1 μK). The transition is induced by an external field feeding a Ramsey cavity. In microgravity the interaction time inside the cavity can be adjusted over two orders of magnitude by changing the atomic velocity (5 cm·s−1–5 m·s−1) in order to study the ultimate performances of the clock. An engineering model has been assembled to validate the architecture of the clock. This model has been fully tested on ground for operation faults. Of course the clock performances are reduced by the effect of the gravity on the moving atoms. The main results are a frequency stability of 3.3× 10−13t−1/2. The main systematic effects have been analyzed and their frequency uncertainties contribution is 1.6 × 10−15. The clock has been compared with the primary frequency standard, the mobile fountain of SYRTE. The mean frequency shift is lower than 2 × 10−15. The mechanical and thermal space qualifications have been carried out by testing a representative mechanical model of the clock and by using refined calculations. The design of the clock has been improved and now the flight model is being assembled. The PHARAO clock is a key instrument of the European ESA space mission called ACES. This mission is dedicated to perform space-time measurements in order to test some fundamental physics aspects.
- Published
- 2014