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Creators/Authors contains: "Sinclair, Laura"

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  1. ; ; ; ; ; ; ; ; ; ; et al (, SPIE)
    Coyle, Laura E; Perrin, Marshall D; Matsuura, Shuji (Ed.)
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  2. ; ; ; ; (, Water Resources Research)
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  3. ; ; ; ; ; ; ; (, Nature)
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  4. ; ; ; (, Nature)
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  5. ; ; ; ; ; ; ; (, Quantum Science and Technology)
    Abstract Recent advances in optical atomic clocks and optical time transfer have enabled new possibilities in precision metrology for both tests of fundamental physics and timing applications. Here we describe a space mission concept that would place a state-of-the-art optical atomic clock in an eccentric orbit around Earth. A high stability laser link would connect the relative time, range, and velocity of the orbiting spacecraft to earthbound stations. The primary goal for this mission would be to test the gravitational redshift, a classical test of general relativity, with a sensitivity 30 000 times beyond current limits. Additional science objectives include other tests of relativity, enhanced searches for dark matter and drifts in fundamental constants, and establishing a high accuracy international time/geodesic reference. 
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  6. ; ; ; ; ; ; ; ; ; ; et al (, SPIE)
    Coyle, Laura E; Perrin, Marshall D; Matsuura, Shuji (Ed.)
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  7. ; ; ; ; ; ; ; ; ; ; et al (, SPIE)
    Coyle, Laura E; Perrin, Marshall D; Matsuura, Shuji (Ed.)
    Full Text Available 
  8. ; ; ; ; ; ; ; ; ; ; et al (, Quantum Science and Technology)
    Abstract We present a concept for a high-precision optical atomic clock (OAC) operating on an Earth-orbiting space station. This pathfinder science mission will compare the space-based OAC with one or more ultra-stable terrestrial OACs to search for space-time-dependent signatures of dark scalar fields that manifest as anomalies in the relative frequencies of station-based and ground-based clocks. This opens the possibility of probing models of new physics that are inaccessible to purely ground-based OAC experiments where a dark scalar field may potentially be strongly screened near Earth’s surface. This unique enhancement of sensitivity to potential dark matter candidates harnesses the potential of space-based OACs. 
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