Quantum noise in differential-type gravitational-wave interferometer and signal recycling
Journal Article
·
· Physical Review. D, Particles Fields
- Graduate School of Human and Environmental Studies, Kyoto University, Kyoto 606-8501 (Japan)
There exists the standard quantum limit (SQL), derived from Heisenberg's uncertainty relation, in the sensitivity of laser interferometer gravitational-wave (GW) detectors. However, in the context of a full quantum-mechanical approach, SQL can be overcome using the correlation of shot noise and radiation-pressure noise. So far, signal recycling, which is one of the methods to overcome SQL, is considered only in a recombined-type interferometer such as Advanced LIGO, LCGT, and GEO600. In this paper, we investigated quantum noise and the possibility of signal recycling in a differential-type interferometer. As a result, we found that signal recycling is possible and creates at most three dips in the sensitivity curve of the detector due to two coupled resonators. The additional third dip makes it possible to decrease quantum noise at low frequencies, keeping the moderate sensitivity at high frequencies. Then, taking advantage of the third dip and comparing the sensitivity of a differential-type interferometer with that of a next-generation Japanese GW interferometer, LCGT, we found that signal-to-noise ratio (SNR) of inspiral binary is improved by a factor of {approx_equal}1.43 for neutron star binary, {approx_equal}2.28 for 50M{sub {center_dot}} black hole binary, and {approx_equal}2.94 for 100M{sub {center_dot}} black hole binary. We also found that power recycling to increase laser power is possible in our signal-recycling configuration of a detector.
- OSTI ID:
- 21027553
- Journal Information:
- Physical Review. D, Particles Fields, Journal Name: Physical Review. D, Particles Fields Journal Issue: 4 Vol. 76; ISSN PRVDAQ; ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
Similar Records
Frequency noise and intensity noise of next-generation gravitational-wave detectors with RF/DC readout schemes
Samurai project: Verifying the consistency of black-hole-binary waveforms for gravitational-wave detection
HIGH-FREQUENCY GRAVITATIONAL WAVES FROM SUPERMASSIVE BLACK HOLES: PROSPECTS FOR LIGO-VIRGO DETECTIONS
Journal Article
·
Thu Jun 15 00:00:00 EDT 2006
· Physical Review. D, Particles Fields
·
OSTI ID:20774850
Samurai project: Verifying the consistency of black-hole-binary waveforms for gravitational-wave detection
Journal Article
·
Wed Apr 15 00:00:00 EDT 2009
· Physical Review. D, Particles Fields
·
OSTI ID:21308320
HIGH-FREQUENCY GRAVITATIONAL WAVES FROM SUPERMASSIVE BLACK HOLES: PROSPECTS FOR LIGO-VIRGO DETECTIONS
Journal Article
·
Thu Feb 14 23:00:00 EST 2013
· Astrophysical Journal
·
OSTI ID:22167120
Related Subjects
46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
BINARY STARS
BLACK HOLES
CORRELATIONS
GRAVITATIONAL WAVE DETECTORS
GRAVITATIONAL WAVES
INTERFEROMETERS
LASERS
NEUTRON STARS
NOISE
QUANTUM GRAVITY
QUANTUM MECHANICS
RADIATION PRESSURE
RESONATORS
SENSITIVITY
SIGNAL-TO-NOISE RATIO
SIGNALS
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
BINARY STARS
BLACK HOLES
CORRELATIONS
GRAVITATIONAL WAVE DETECTORS
GRAVITATIONAL WAVES
INTERFEROMETERS
LASERS
NEUTRON STARS
NOISE
QUANTUM GRAVITY
QUANTUM MECHANICS
RADIATION PRESSURE
RESONATORS
SENSITIVITY
SIGNAL-TO-NOISE RATIO
SIGNALS