An extension to the noise theory of RF SQUIDs with implications for gravitational radiation detectors

Details An extension to the noise theory of RF SQUIDs with implications for gravitational radiation detectors An extension to the noise theory of RF SQUIDs with implications for gravitational radiation detectors

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977jphe...10..993h&link_type=abstract

Journal of Physics E - Scientific Instruments, vol. 10, Oct. 1977, p. 993-997. Research supported by the University of Glasgow

Physics

3

Gravitational Waves, Noise Intensity, Radiation Detectors, Radio Reception, Superconductors, Phase Shift, Quantum Theory, Rlc Circuits, Thermal Noise, Volt-Ampere Characteristics

Scientific paper

The noise theory of an RF SQUID is extended to include those components of flux noise which appear physically linking the SQUID loop. This noise is a consequence of phase fluctuations of the quantum transitions in the SQUID and can react on the system whose parameters are being measured by the SQUID sensor. In particular, we consider a gravitational wave detector whose motion is sensed by an RF SQUID system; and we show that the back-reaction, combined with other noise, imposes a limit to the detector sensitivity.

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