On the measurement of proper time in general relativity by means of atomic clocks
The quantity τ, which is called the proper time of a particle in the general theory of relativity, has the following meaning: it is the time measured by clocks moving with the particle. The question arises of how proper time is measured by real clocks. At present, atomic clocks are the most accurate, being stabilized by the frequency of intraatomic transitions. In the present paper, the stability of the reference frequency of such clocks is considered, i.e., the possible discrepancies between the proper time and the time measured by atomic clocks.
KeywordsGeneral Relativity General Theory Proper Time Reference Frequency Atomic Clock
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- 1.J. L. Synge, Relativity, the General Theory, Amsterdam (1960).Google Scholar
- 2.M. F. Shirokov and B. V. Bondarev, Preprint ITF-74-140 [in Russian], Kiev (1973).Google Scholar
- 3.V. I. Golikov and M. D. Sherman, in: Gravitation and Relativity Theory, No. 9 [in Russian], Kazan' (1973), p. 9.Google Scholar
- 4.A. A, Sokolov, Yu. M. Loskutov, and I. M. Ternov, Quantum Mechanics [in Russian], Moscow (1965).Google Scholar
- 5.F. K. Manasse and C. W. Misner, J. Math. Phys.,4, 735 (1963).Google Scholar
- 6.I. Audretsch and G. Schäfer, Gen. Rel. Grav.,9, 489 (1978).Google Scholar
- 7.E. Schrödinger, Acta Pont. Acad. Sci.,2, 321 (1937); Physica (Utrecht),6, 899 (1939).Google Scholar
- 8.A. P. Bondarev and K. P. Stanyukovich, in: Abstracts of Proceedings of the Third Soviet Gravitational Conference [in Russian], Erevan (1972), p. 215.Google Scholar