Search results for "Interferometry"

showing 10 items of 343 documents

Double Bragg Interferometry.

2015

We employ light-induced double Bragg diffraction of delta-kick collimated Bose-Einstein condensates to create three symmetric Mach-Zehnder interferometers. They rely on (i) first-order, (ii) two successive first-order, and (iii) second-order processes which demonstrate the scalability of the corresponding momentum transfer. With respect to devices based on conventional Bragg scattering, these symmetric interferometers double the scale factor and feature a better suppression of noise and systematic uncertainties intrinsic to the diffraction process. Moreover, we utilize these interferometers as tiltmeters for monitoring their inclination with respect to gravity.

Condensed Matter::Quantum GasesDiffractionPhysicsbusiness.industryMomentum transferGeneral Physics and AstronomyBragg's lawScale factor01 natural sciencesNoise (electronics)Collimated light010305 fluids & plasmasInterferometryOptics0103 physical sciencesAstronomical interferometer010306 general physicsbusinessPhysical review letters
researchProduct

Entanglement interferometry for precision measurement of atomic scattering properties.

2003

We report on a two-particle matter wave interferometer realized with pairs of trapped 87Rb atoms. Each pair of atoms is confined at a single site of an optical lattice potential. The interferometer is realized by first creating a coherent spin-mixture of the two atoms and then tuning the inter-state scattering length via a Feshbach resonance. The selective change of the inter-state scattering length leads to an entanglement dynamics of the two-particle state that can be detected in a Ramsey interference experiment. This entanglement dynamics is employed for a precision measurement of atomic interaction parameters. Furthermore, the interferometer allows to separate lattice sites with one or …

Condensed Matter::Quantum GasesPhysicsQuantum PhysicsOptical latticeAtomic Physics (physics.atom-ph)ScatteringFOS: Physical sciencesGeneral Physics and AstronomyScattering lengthQuantum entanglementCondensed Matter - Soft Condensed MatterPhysics - Atomic PhysicsInterferometrySuperposition principleQuantum mechanicsSoft Condensed Matter (cond-mat.soft)Physics::Atomic PhysicsMatter waveAtomic physicsQuantum Physics (quant-ph)Feshbach resonancePhysical review letters
researchProduct

Surface Acoustic Bloch Oscillations, the Wannier-Stark Ladder, and Landau-Zener Tunneling in a Solid

2010

We present the experimental observation of Bloch oscillations, the Wannier-Stark ladder, and Landau-Zener tunneling of surface acoustic waves in perturbed grating structures on a solid substrate. A model providing a quantitative description of our experimental observations, including multiple Landau-Zener transitions of the anticrossed surface acoustic Wannier-Stark states, is developed. The use of a planar geometry for the realization of the Bloch oscillations and Landau-Zener tunneling allows a direct access to the elastic field distribution. The vertical surface displacement has been measured by interferometry.

Condensed Matter::Quantum GasesPhysicsSurface (mathematics)Condensed matter physicsCondensed Matter::OtherGeneral Physics and AstronomyAcoustic waveEnginyeria acústicaCiència dels materialsGratingCondensed Matter::Mesoscopic Systems and Quantum Hall EffectInterferometryDistribution (mathematics)Quantum mechanicsBloch oscillationsPhysics::Atomic PhysicsRealization (systems)Quantum tunnellingPhysical Review Letters
researchProduct

High Precision Astrometry Over Large Angular Scales with Closure Constraints: The Triplet 1803+784/1928+738/2007+777

1996

The technique of differential astrometry using the phase-delay VLBI observable promises fractional precisions of ~2 × 10−9 in the determination of the separation of sources 5° or 6° apart on the sky (Guirado et al. 1995a; Lara et al. 1996). In our present research we seek further improvement in this technique through using triplets of radio sources, which provide a closure constraint in the determination of relative angular positions. This constraint not only eases the resolution of the phase-cycle ambiguities (a major problem in the least-squares approach to astrometry with phase delays), but it also strongly constrains the space of allowable parameter values.

Constraint (information theory)PhysicsAngular distanceSkymedia_common.quotation_subjectVery-long-baseline interferometryClosure (topology)Phase (waves)ObservableAstrophysicsAstrometrymedia_common
researchProduct

What causes the large extensions of red-supergiant atmospheres? Comparisons of interferometric observations with 1-D hydrostatic, 3-D convection, and…

2015

We present the atmospheric structure and the fundamental parameters of three red supergiants, increasing the sample of RSGs observed by near-infrared spectro-interferometry. Additionally, we test possible mechanisms that may explain the large observed atmospheric extensions of RSGs. We carried out spectro-interferometric observations of 3 RSGs in the near-infrared K-band with the VLTI/AMBER instrument at medium spectral resolution. To comprehend the extended atmospheres, we compared our observational results to predictions by available hydrostatic PHOENIX, available 3-D convection, and new 1-D self-excited pulsation models of RSGs. Our near-infrared flux spectra are well reproduced by the P…

ConvectionPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicslaw.inventionInterferometryAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencelawAstrophysics::Solar and Stellar AstrophysicsRed supergiantChristian ministryAstrophysics::Earth and Planetary AstrophysicsSupergiantHydrostatic equilibriumSolar and Stellar Astrophysics (astro-ph.SR)
researchProduct

Spatially-multiplexed interferometric microscopy (SMIM): converting a standard microscope into a holographic one

2014

We report on an extremely simple, low cost and highly stable way to convert a standard microscope into a holographic one. The proposed architecture is based on a common-path interferometric layout where the input plane is spatially-multiplexed to allow reference beam transmission in a common light-path with the imaging branch. As consequence, the field of view provided by the layout is reduced. The use of coherent illumination (instead of the broadband one included in the microscope) and a properly placed one-dimensional diffraction grating (needed for the holographic recording) complete the experimental layout. The proposed update is experimentally validated in a regular Olympus BX-60 upri…

Conventional transmission electron microscopeMicroscopeMaterials sciencebusiness.industryComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONHolographyInterferometric microscopyAtomic and Molecular Physics and Opticslaw.inventionInterferometryOpticslawReference beamMicroscopyDigital holographic microscopybusinessOptics Express
researchProduct

Studies of Relativistic Jets in Active Galactic Nuclei with SKA

2014

Relativistic jets in active galactic nuclei (AGN) are among the most powerful astrophysical objects discovered to date. Indeed, jetted AGN studies have been considered a prominent science case for SKA, and were included in several different chapters of the previous SKA Science Book (Carilli & Rawlings 2004). Most of the fundamental questions about the physics of relativistic jets still remain unanswered, and await high-sensitivity radio instruments such as SKA to solve them. These questions will be addressed specially through analysis of the massive data sets arising from the deep, all-sky surveys (both total and polarimetric flux) from SKA1. Wide-field very-long-baseline-interferometri…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleus010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsJet (particle physics)01 natural sciencesAstrophysical jet0103 physical sciencesVery-long-baseline interferometryInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsStar formationAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstrophysics - Astrophysics of GalaxiesGalaxyCharacterization (materials science)13. Climate actionAstrophysics of Galaxies (astro-ph.GA)Brightness temperatureAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsProceedings of Advancing Astrophysics with the Square Kilometre Array — PoS(AASKA14)
researchProduct

The transient gravitational-wave sky

2013

Interferometric detectors will very soon give us an unprecedented view of the gravitational-wave sky, and in particular of the explosive and transient Universe. Now is the time to challenge our theoretical understanding of short-duration gravitational-wave signatures from cataclysmic events, their connection to more traditional electromagnetic and particle astrophysics, and the data analysis techniques that will make the observations a reality. This paper summarizes the state of the art, future science opportunities, and current challenges in understanding gravitational-wave transients.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Explosive materialmedia_common.quotation_subjectELECTROMAGNETIC COUNTERPARTSFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologySPIN-DOWN LIMIT0103 physical sciencesPRESUPERNOVA EVOLUTIONCORE-COLLAPSE010306 general physics010303 astronomy & astrophysicsARMED SPIRAL INSTABILITYmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Astroparticle physicsPhysicsGAMMA-RAY BURSTSNEUTRINO PAIR ANNIHILATIONGravitational waveAstronomyMASS BLACK-HOLESUniverseBAR-MODE INSTABILITYInterferometrySkyData analysisTransient (oscillation)Astrophysics - High Energy Astrophysical PhenomenaDRIVEN SUPERNOVAgravitational waves neutron stars black holesAstrophysics - Cosmology and Nongalactic AstrophysicsClassical and Quantum Gravity
researchProduct

All-Optical Fiber Hanbury Brown & Twiss Interferometer to study 1300 nm single photon emission of a metamorphic InAs Quantum Dot

2016

[EN] New optical fiber based spectroscopic tools open the possibility to develop more robust and efficient characterization experiments. Spectral filtering and light reflection have been used to produce compact and versatile fiber based optical cavities and sensors. Moreover, these technologies would be also suitable to study N-photon correlations, where high collection efficiency and frequency tunability is desirable. We demonstrated single photon emission of a single quantum dot emitting at 1300 nm, using a Fiber Bragg Grating for wavelength filtering and InGaAs Avalanche Photodiodes operated in Geiger mode for single photon detection. As we do not observe any significant fine structure s…

DYNAMICS0301 basic medicinePhotonOptical fiberRECOMBINATIONPhysics::Optics02 engineering and technologyArticlelaw.invention03 medical and health sciencesOpticsSpontaneous parametric down-conversionFiber Bragg gratinglawTEORIA DE LA SEÑAL Y COMUNICACIONESAstronomical interferometerPhysicsSPECTROSCOPYMultidisciplinarybusiness.industryNew optical fiber based spectroscopicHanbury Brown and Twiss effectCondensed Matter::Mesoscopic Systems and Quantum Hall Effect021001 nanoscience & nanotechnologyInterferometryLIGHT030104 developmental biologyQuantum dot0210 nano-technologybusinessScientific Reports
researchProduct

Digital holographic microscopy with pure-optical spherical phase compensation

2011

Telecentric architecture is proposed for circumventing, by the pure-optical method, the residual parabolic phase distortion inherent to standard configuration of digital holographic microscopy. This optical circumvention produces several important advantages. One is that there is no need for computer compensation of the parabolic phase during the phase map recovering procedure. The other is that in off-axis configuration, the spatial frequency useful domain is enlarged. The validity of the method is demonstrated by performing quantitative measurement of depth differences with high axial resolution. (C) 2011 Optical Society of America

DYNAMICSMaterials sciencebusiness.industryPhase distortionPhase (waves)Image processingResidualCONTRAST MICROSCOPYAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsCompensation (engineering)INTERFEROMETRYIMAGE-RECONSTRUCTIONOpticsNUMERICAL RECONSTRUCTIONDigital holographic microscopyComputer Vision and Pattern RecognitionSpatial frequencybusinessDigital holographyJournal of the Optical Society of America A
researchProduct