Relativistic theory for time and frequency transfer to order c-3

被引:93
作者
Blanchet, L [1 ]
Salomon, C
Teyssandier, P
Wolf, P
机构
[1] Observ Paris, Dept Astrophys Relativiste & Cosmol, F-92195 Meudon, France
[2] Ecole Normale Super, Lab Kastler Brossel, F-75231 Paris, France
[3] Observ Paris, DANOF, CNRS UMR 8630, F-75014 Paris, France
[4] Bur Int Poids & Mesures, F-92312 Sevres, France
关键词
relativity; reference systems; time;
D O I
10.1051/0004-6361:20010233
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This paper is motivated by the current development of several space missions (e.g. AGES on International Space Station) that will use Earth-orbit laser cooled atomic clocks, providing a time-keeping accuracy of the order of 5 10(-17) in fractional frequency. We show that to such accuracy, the theory of frequency transfer between Earth and Space must be extended from the currently known relativistic order 1/c(2) (which has been needed in previous space experiments such as GP-A) to the next relativistic correction of order 1/c(3). We find that the frequency transfer includes the first and second-order Doppler contributions, the Einstein gravitational red-shift and, at the order 1/c(3), a mixture of these effects. As for the time transfer, it contains the standard Shapiro time delay, and we present an expression also including the first and second-order Sagnac corrections. Higher-order relativistic corrections, at least O(1/c(4)), are numerically negligible for time and frequency transfers in these experiments, being for instance of order 10(-20) in fractional frequency. Particular attention is paid to the problem of the frequency transfer in the two-way experimental configuration. In this case we find a simple theoretical expression which extends the previous formula (Vessot ct al. 1980) to the next order 1/c(3). In the Appendix we present the detailed proofs of all the formulas which will be needed in such experiments.
引用
收藏
页码:320 / 329
页数:10
相关论文
共 26 条
[1]  
ALLAN DW, 1985, P IAU S, V114, P299
[2]  
[Anonymous], 1981, Theory and Experiment in Gravitational Physics
[3]   Testing relativity with a laser-cooled cesium clock in space [J].
Ashby, N .
PROCEEDINGS OF THE 1998 IEEE INTERNATIONAL FREQUENCY CONTROL SYMPOSIUM, 1998, :320-328
[4]   PRACTICAL IMPLICATIONS OF RELATIVITY FOR A GLOBAL COORDINATE TIME SCALE [J].
ASHBY, N ;
ALLAN, DW .
RADIO SCIENCE, 1979, 14 (04) :649-669
[5]   High-accuracy measurement of the 87Rb ground-state hyperfine splitting in an atomic fountain [J].
Bize, S ;
Sortais, Y ;
Santos, MS ;
Mandache, C ;
Clairon, A ;
Salomon, C .
EUROPHYSICS LETTERS, 1999, 45 (05) :558-564
[6]   RELATIVISTIC TIME SCALES IN THE SOLAR SYSTEM [J].
Brumberg, V. A. ;
Kopejkin, S. M. .
CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY, 1990, 48 (01) :23-44
[7]   POINT CHARACTERISTICS OF SOME STATIC SPHERICALLY SYMMETRIC SPACE-TIMES [J].
BUCHADAH.HA .
OPTICA ACTA, 1970, 17 (09) :707-&
[8]   PERTURBED CHARACTERISTIC FUNCTIONS - APPLICATION TO THE LINEARIZED GRAVITATIONAL-FIELD [J].
BUCHDAHL, HA .
AUSTRALIAN JOURNAL OF PHYSICS, 1979, 32 (04) :405-410
[9]  
FRIDELANCE P, 1996, EXPT ASTRON, P191
[10]  
HETZEL P, 1993, P 7 EUR FREQ TIM FOR, P125