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      Demonstration of Time Delay Interferometry and Spacecraft Ranging in a Space-based Gravitational Wave Detector using the UF-LISA Interferometry Simulator

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          Abstract

          Space-based gravitational-wave observatories such as the Laser Interferometer Space Antenna (LISA) use time-shifted and time-scaled linear combinations of differential laser-phase beat signals to cancel the otherwise overwhelming laser frequency noise. Nanosecond timing precision is needed to accurately form these Time-Delay Interferometry (TDI) combinations which defines a ~1 meter requirement on the inter-spacecraft ranging capability. The University of Florida Hardware-in-the-loop LISA Interferometry Simulator (UFLIS) has been used to test Time-Delay Interferometry in a configuration which incorporates variable delays, realistic Doppler shifts, and simulated gravitational-wave signals. The TDI 2.0 combinations are exploited to determine the time-changing delays with nanosecond accuracy using a TDI-ranging reference tone. These variable delays are used in forming the TDI combinations to achieve the LISA interferometry sensitivity resulting from 10 orders of magnitude laser frequency noise cancellation.

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          Confusion noise level due to galactic and extragalactic binaries

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            Space-based gravitational wave detection with LISA

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              The LISA benchtop simulator at the University of Florida

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                Author and article information

                Journal
                09 May 2012
                2012-11-05
                Article
                10.1103/PhysRevD.86.122006
                1205.1934
                d33a50a0-75e1-42c6-aada-e4e847bf6385

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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                Custom metadata
                Accepted: Physical Review D, 12 pages, 12 figures
                astro-ph.IM

                Instrumentation & Methods for astrophysics
                Instrumentation & Methods for astrophysics

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