509 research outputs found
Experimental Demonstration of Time-Delay Interferometry for the Laser Interferometer Space Antenna
We report on the first demonstration of time-delay interferometry (TDI) for
LISA, the Laser Interferometer Space Antenna. TDI was implemented in a
laboratory experiment designed to mimic the noise couplings that will occur in
LISA. TDI suppressed laser frequency noise by approximately 10^9 and clock
phase noise by 6x10^4, recovering the intrinsic displacement noise floor of our
laboratory test bed. This removal of laser frequency noise and clock phase
noise in post-processing marks the first experimental validation of the LISA
measurement scheme.Comment: 4 pages, 4 figures, to appear in Physical Review Letters end of May
201
High-sensitivity optical monitoring of a micro-mechanical resonator with a quantum-limited optomechanical sensor
We experimentally demonstrate the high-sensitivity optical monitoring of a
micro-mechanical resonator and its cooling by active control. Coating a
low-loss mirror upon the resonator, we have built an optomechanical sensor
based on a very high-finesse cavity (30000). We have measured the thermal noise
of the resonator with a quantum-limited sensitivity at the 10^-19 m/rootHz
level, and cooled the resonator down to 5K by a cold-damping technique.
Applications of our setup range from quantum optics experiments to the
experimental demonstration of the quantum ground state of a macroscopic
mechanical resonator.Comment: 4 pages, 5 figure
Continuous variable polarization entanglement, experiment and analysis
We generate and characterise continuous variable polarization entanglement
between two optical beams. We first produce quadrature entanglement, and by
performing local operations we transform it into a polarization basis. We
extend two entanglement criteria, the inseparability criteria proposed by Duan
{\it et al.}\cite{Duan00} and the Einstein-Podolsky-Rosen paradox criteria
proposed by Reid and Drummond\cite{Reid88}, to Stokes operators; and use them
to charactise the entanglement. Our results for the Einstein-Podolsky-Rosen
paradox criteria are visualised in terms of uncertainty balls on the
Poincar\'{e} sphere. We demonstrate theoretically that using two quadrature
entangled pairs it is possible to entangle three orthogonal Stokes operators
between a pair of beams, although with a bound times more stringent
than for the quadrature entanglement.Comment: 12 pages, 13 figure
Optimal statistic for detecting gravitational wave signals from binary inspirals with LISA
A binary compact object early in its inspiral phase will be picked up by its
nearly monochromatic gravitational radiation by LISA. But even this innocuous
appearing candidate poses interesting detection challenges. The data that will
be scanned for such sources will be a set of three functions of LISA's twelve
data streams obtained through time-delay interferometry, which is necessary to
cancel the noise contributions from laser-frequency fluctuations and
optical-bench motions to these data streams. We call these three functions
pseudo-detectors. The sensitivity of any pseudo-detector to a given sky
position is a function of LISA's orbital position. Moreover, at a given point
in LISA's orbit, each pseudo-detector has a different sensitivity to the same
sky position. In this work, we obtain the optimal statistic for detecting
gravitational wave signals, such as from compact binaries early in their
inspiral stage, in LISA data. We also present how the sensitivity of LISA,
defined by this optimal statistic, varies as a function of sky position and
LISA's orbital location. Finally, we show how a real-time search for inspiral
signals can be implemented on the LISA data by constructing a bank of templates
in the sky positions.Comment: 22 pages, 15 eps figures, Latex, uses iopart style/class files. Based
on talk given at the 8th Gravitational Wave Data Analysis Workshop,
Milwaukee, USA, December 17-20, 2003. Accepted for publication in Class.
Quant. Gra
Measurement of Optical Response of a Detuned Resonant Sideband Extraction Interferometer
We report on the optical response of a suspended-mass detuned resonant
sideband extraction (RSE) interferometer with power recycling. The purpose of
the detuned RSE configuration is to manipulate and optimize the optical
response of the interferometer to differential displacements (induced by
gravitational waves) as a function of frequency, independently of other
parameters of the interferometer. The design of our interferometer results in
an optical gain with two peaks: an RSE optical resonance at around 4 kHz and a
radiation pressure induced optical spring at around 41 Hz. We have developed a
reliable procedure for acquiring lock and establishing the desired optical
configuration. In this configuration, we have measured the optical response to
differential displacement and found good agreement with predictions at both
resonances and all other relevant frequencies. These results build confidence
in both the theory and practical implementation of the more complex optical
configuration being planned for Advanced LIGO.Comment: 6 pages, 4 figures, for submission to Phys Rev Letter
Experimental demonstration of a squeezing enhanced power recycled Michelson interferometer for gravitational wave detection
Interferometric gravitational wave detectors are expected to be limited by
shot noise at some frequencies. We experimentally demonstrate that a power
recycled Michelson with squeezed light injected into the dark port can overcome
this limit. An improvement in the signal-to-noise ratio of 2.3dB is measured
and locked stably for long periods of time. The configuration, control and
signal readout of our experiment are compatible with current gravitational wave
detector designs. We consider the application of our system to long baseline
interferometer designs such as LIGO.Comment: 4 pages 4 figure
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