2015
DOI: 10.1007/s10714-014-1845-5
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Optical cavity resonator in an expanding universe

Abstract: We study the cosmological evolution of frequency of a standing electromagnetic wave in a resonant optical cavity placed to the expanding manifold described by the Robertson-Walker metric. Because of the Einstein principle of equivalence (EEP), one can find a local coordinate system (a local freely falling frame), in which spacetime is locally Minkowskian. However, due to the conformal nature of the Robertson-Walker metric the conventional transformation to the local inertial coordinates introduces ambiguity in… Show more

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Cited by 6 publications
(7 citation statements)
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References 52 publications
(98 reference statements)
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“…As we show in the following, this is not the case for the other observers that we consider, which do not follow the Hubble flow. Note that, in the limit m(t)/r → 0, i.e., when the usual FLRW metric is recovered, we remain with corrections quadratic in H 0 in agreement with previous results in the literature [10].…”
Section: Cosmological Observersupporting
confidence: 91%
“…As we show in the following, this is not the case for the other observers that we consider, which do not follow the Hubble flow. Note that, in the limit m(t)/r → 0, i.e., when the usual FLRW metric is recovered, we remain with corrections quadratic in H 0 in agreement with previous results in the literature [10].…”
Section: Cosmological Observersupporting
confidence: 91%
“…For example, the frequency spectrum of a resonator depends on its dimensions and hence knowledge of the precise values of these dimensions is of utmost importance. Cases in which the effects of gravitational fields and acceleration must be considered include those in which the gravitational field is to be measured, such as in proposals for the measurement of gravitational waves with electromagnetic cavity resonators [1][2][3][4][5][6][7] or other extended matter systems [8][9][10][11][12][13][14], tests of GR [15,16] or the expansion of the universe [17,18]. Other situations are those in which the metrological system is significantly accelerated [19][20][21].…”
Section: Introductionmentioning
confidence: 99%
“…Ref. [21] discusses that such an effect is absent if General Relativity holds. To arrive at such a bound we first discuss how bounds of LPI violation and time-variation of fundamental constants contribute.…”
mentioning
confidence: 99%