2021
DOI: 10.1088/1361-6382/abf895
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Testing the Einstein equivalence principle with two Earth-orbiting clocks

Abstract: We consider the problem of testing the Einstein equivalence principle (EEP) by measuring the gravitational redshift with two Earth-orbiting stable atomic clocks. For a reasonably restricted class of orbits we find an optimal experiment configuration that provides for the maximum accuracy of measuring the relevant EEP violation parameter. The perigee height of such orbits is ∼1000 km and the period is 3-5 h, depending on the clock type. For the two of the current best space-qualified clocks, the VCH-1010 hydrog… Show more

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Cited by 10 publications
(8 citation statements)
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References 21 publications
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“…We note that variations of such experiments with optical clocks in space have been proposed, e.g. Altschul et al (2015), Litvinov and Pilipenko (2021).…”
Section: Testing Gr and The Standard Model Of Physics With Atomic Clocksmentioning
confidence: 98%
“…We note that variations of such experiments with optical clocks in space have been proposed, e.g. Altschul et al (2015), Litvinov and Pilipenko (2021).…”
Section: Testing Gr and The Standard Model Of Physics With Atomic Clocksmentioning
confidence: 98%
“…Our present proposal does not require an optical link enabling comparing the satellite and Earth-based clocks. If such a link can be achieved, one can also directly test general relativity and provide a direct bound on the anomalous gravitational redshift exceeding present bounds by orders of magnitude [103][104][105].…”
Section: Spatial Variation Of Fundamental Constantsmentioning
confidence: 99%
“…In the lower panel, we observe that even a very small bound mass, of order 10 −16 M , can give rise to a 10 4 increase in the density of DM at 0.1 AU for m φ 10 −13 eV. It has been proposed to put atomic clocks in orbit around the Earth [104,105] and on the moon (see e.g. [110]).…”
mentioning
confidence: 94%
“…Finally, VLBI requires highly stable atomic frequency standards to be used at each of the participating radio telescope, including those in space, to coherently time-tag the signals received from astronomical sources. Those frequency standards not only provide time and frequency reference signals for the on-board electronic equipment but also are usually used to synchronize downlink signal frequencies, which provides for performing high-accuracy radio science experiments with space-VLBI SC (Biriukov et al, 2014;Litvinov et al, 2018;Nunes et al, 2020;Gurvits, 2020;Litvinov & Pilipenko, 2021). Therefore, to evaluate the significance of the changes we introduced to the APCM effect model we apply it to the case of the RadioAstron spacecraft (Kardashev et al, 2013) and the NRAO140 antenna of the Green Bank Earth Station (Ford et al, 2014) which served the RadioAstron SVLBI mission.…”
Section: Introductionmentioning
confidence: 99%