P. Lemonde
Centre national de la recherche scientifique
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Featured researches published by P. Lemonde.
Physical Review Letters | 2011
Philip G. Westergaard; J. Lodewyck; Luca Lorini; Arnaud Lecallier; Eric A. Burt; M. Zawada; J. Millo; P. Lemonde
We present a comprehensive study of the frequency shifts associated with the lattice potential in a Sr lattice clock by comparing two such clocks with a frequency stability reaching 5×10(-17) after a 1 h integration time. We put the first experimental upper bound on the multipolar M1 and E2 interactions, significantly smaller than the recently predicted theoretical upper limit, and give a 30-fold improved upper limit on the effect of hyperpolarizability. Finally, we report on the first observation of the vector and tensor shifts in a Sr lattice clock. Combining these measurements, we show that all known lattice related perturbations will not affect the clock accuracy down to the 10(-17) level, even for lattices as deep as 150 recoil energies.
Physical Review Letters | 2004
M. Fischer; Nikolai N. Kolachevsky; Marcus Zimmermann; Ronald Holzwarth; Thomas Udem; T. W. Hänsch; M. Abgrall; J. Grunert; I. Maksimovic; S. Bize; H. Marion; F. Pereira Dos Santos; P. Lemonde; G. Santarelli; P. Laurent; A. Clairon; Christophe Salomon; Martin Haas; Ulrich D. Jentschura; Christoph H. Keitel
We have remeasured the absolute 1S-2S transition frequency nu(H) in atomic hydrogen. A comparison with the result of the previous measurement performed in 1999 sets a limit of (-29+/-57) Hz for the drift of nu(H) with respect to the ground state hyperfine splitting nu(Cs) in 133Cs. Combining this result with the recently published optical transition frequency in 199Hg+ against nu(Cs) and a microwave 87Rb and 133Cs clock comparison, we deduce separate limits on alpha/alpha=(-0.9+/-2.9) x 10(-15) yr(-1) and the fractional time variation of the ratio of Rb and Cs nuclear magnetic moments mu(Rb)/mu(Cs) equal to (-0.5+/-1.7) x 10(-15) yr(-1). The latter provides information on the temporal behavior of the constant of strong interaction.
Physical Review Letters | 2003
H. Marion; F. Pereira Dos Santos; M. Abgrall; S. Zhang; Y. Sortais; S. Bize; I. Maksimovic; Davide Calonico; J. Grunert; C. Mandache; P. Lemonde; G. Santarelli; Ph. Laurent; A. Clairon; Christophe Salomon
Over five years, we have compared the hyperfine frequencies of 133Cs and 87Rb atoms in their electronic ground state using several laser-cooled 133Cs and 87Rb atomic fountains with an accuracy of approximately 10(-15). These measurements set a stringent upper bound to a possible fractional time variation of the ratio between the two frequencies: d/dt ln([(nu(Rb))/(nu(Cs))]=(0.2+/-7.0)x 10(-16) yr(-1) (1sigma uncertainty). The same limit applies to a possible variation of the quantity (mu(Rb)/mu(Cs))alpha(-0.44), which involves the ratio of nuclear magnetic moments and the fine structure constant.
Physical Review Letters | 2008
Sebastian Blatt; Andrew D. Ludlow; Gretchen K. Campbell; Jan Thomsen; Tanya Zelevinsky; Martin M. Boyd; J. Ye; X. Baillard; Mathilde Fouché; R. Le Targat; A. Brusch; P. Lemonde; Masao Takamoto; Feng-Lei Hong; Hidetoshi Katori; V. V. Flambaum
The 1S0-3P0 clock transition frequency nuSr in neutral 87Sr has been measured relative to the Cs standard by three independent laboratories in Boulder, Paris, and Tokyo over the last three years. The agreement on the 1 x 10(-15) level makes nuSr the best agreed-upon optical atomic frequency. We combine periodic variations in the 87Sr clock frequency with 199Hg+ and H-maser data to test local position invariance by obtaining the strongest limits to date on gravitational-coupling coefficients for the fine-structure constant alpha, electron-proton mass ratio mu, and light quark mass. Furthermore, after 199Hg+, 171Yb+, and H, we add 87Sr as the fourth optical atomic clock species to enhance constraints on yearly drifts of alpha and mu.
Physical Review A | 2009
J. Millo; Daniel Varela Magalhães; C. Mandache; Y. Le Coq; E. M. L. English; Philip G. Westergaard; Jérôme Lodewyck; S. Bize; P. Lemonde; G. Santarelli
We present two ultrastable lasers based on two vibration insensitive cavity designs, one with vertical optical axis geometry, the other horizontal. Ultrastable cavities are constructed with fused silica mirror substrates, shown to decrease the thermal noise limit, in order to improve the frequency stability over previous designs. Vibration sensitivity components measured are equal to or better than
Journal of The Optical Society of America B-optical Physics | 2008
Haifeng Jiang; Fabien Kéfélian; Scott Crane; O. Lopez; M. Lours; J. Millo; D. Holleville; P. Lemonde; Christian Chardonnet; A. Amy-Klein; Georgio Santarelli
1.5\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}11}/\text{m}\text{ }{\text{s}}^{\ensuremath{-}2}
Journal of Physics B | 2005
S. Bize; P. Laurent; M. Abgrall; H. Marion; I. Maksimovic; L. Cacciapuoti; J. Grunert; C. Vian; F. Pereira Dos Santos; P. Rosenbusch; P. Lemonde; G. Santarelli; Peter Wolf; A. Clairon; Andre Luiten; Michael E. Tobar; C. Salomon
for each spatial direction, which shows significant improvement over previous studies. We have tested the very low dependence on the position of the cavity support points, in order to establish that our designs eliminate the need for fine tuning to achieve extremely low vibration sensitivity. Relative frequency measurements show that at least one of the stabilized lasers has a stability better than
Optics Communications | 2006
X. Baillard; A. Gauguet; S. Bize; P. Lemonde; Ph. Laurent; A. Clairon; P. Rosenbusch
5.6\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}16}
Nature Communications | 2013
R. Le Targat; Luca Lorini; Y. Le Coq; M. Zawada; J. Guéna; M. Abgrall; Mikhail Gurov; P. Rosenbusch; Daniele Rovera; Bartłomiej Nagórny; R. Gartman; Philip G. Westergaard; Michael Tobar; M. Lours; G. Santarelli; A. Clairon; S. Bize; P. Laurent; P. Lemonde; J. Lodewyck
at 1 s, which is the best result obtained for this length of cavity.
Experimental Astronomy | 2009
Peter Wolf; Ch. J. Bordé; A. Clairon; Loic Duchayne; Arnaud Landragin; P. Lemonde; G. Santarelli; W. Ertmer; Ernst M. Rasel; F. S. Cataliotti; M. Inguscio; G. M. Tino; P. Gill; H. A. Klein; Serge Reynaud; C. Salomon; E. Peik; Orfeu Bertolami; P. J. S. Gil; Jorge Páramos; C. Jentsch; Ulrich Johann; A. Rathke; Philippe Bouyer; L. Cacciapuoti; D. Izzo; P. De Natale; Bruno Christophe; Pierre Touboul; Slava G. Turyshev
We transferred the frequency of an ultra-stable laser over 86 km of urban fiber. The link is composed of two cascaded 43-km fibers connecting two laboratories, LNE-SYRTE and LPL in Paris area. In an effort to realistically demonstrate a link of 172 km without using spooled fiber extensions, we implemented a recirculation loop to double the length of the urban fiber link. The link is fed with a 1542-nm cavity stabilized fiber laser having a sub-Hz linewidth. The fiber-induced phase noise is measured and cancelled with an all fiber-based interferometer using commercial off the shelf pigtailed telecommunication components. The compensated link shows an Allan deviation of a few 10-16 at one second and a few 10-19 at 10,000 seconds.