Reduction of optimum light power with Heisenberg-limited photon-counting noise in interferometric gravitational-wave detectors

Physics Letters, Section A: General, Atomic and Solid State Physics

Volumn 263, Issue 1-2, 1999, Pages 15-20

  Brif, Constantin ^a,b  

^a PRINCETON UNIVERSITY   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

GRAVITATIONAL EFFECTS; INTERFEROMETRY; PHOTONS; QUANTUM NOISE; SIGNAL DETECTION;

GRAVITATIONAL WAVE DETECTORS; HEISENBERG; HEISENBERG LIMIT; INPUT STATE; LIGHT POWER; PHOTON-COUNTING NOISE; STANDARD QUANTUM LIMITS;

GRAVITY WAVES;

EID: 0347245360     PISSN: 03759601     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0375-9601(99)00714-8     Document Type: Article

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