Search results for "Acceleration"

showing 10 items of 345 documents

Acceleration radiation, transition probabilities, and trans-Planckian physics

2010

An important question in the derivation of the acceleration radiation, which also arises in Hawking's derivation of black hole radiance, is the need to invoke trans-Planckian physics in describing the creation of quanta. We point out that this issue can be further clarified by reconsidering the analysis in terms of particle detectors, transition probabilities and local two-point functions. By writing down separate expressions for the spontaneous-and induced-transition probabilities of a uniformly accelerated detector, we show that the bulk of the effect comes from the natural (non-trans-Planckian) scale of the problem, which largely diminishes the importance of the trans-Planckian sector. T…

High Energy Physics - TheoryPhysicsAstrofísicaPhysics::General Physics010308 nuclear & particles physicsGeneral Physics and AstronomyFOS: Physical sciencesAcceleration (differential geometry)Scale (descriptive set theory)General Relativity and Quantum Cosmology (gr-qc)RadiationLorentz covariance01 natural sciencesGeneral Relativity and Quantum CosmologyPartícules (Física nuclear)Black holeTheoretical physicsHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHawkingHigh Energy Physics - Theory (hep-th)0103 physical sciencesRadianceQuantum field theory010306 general physics
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Cosmological waveguides for gravitational waves

1997

We study the linearized equations describing the propagation of gravitational waves through dust. In the leading order of the WKB approximation, dust behaves as a non-dispersive, non-dissipative medium. Taking advantage of these features, we explore the possibility that a gravitational wave from a distant source gets trapped by the gravitational field of a long filament of galaxies of the kind seen in the large scale structure of the Universe. Such a waveguiding effect may lead to a huge magnification of the radiation from distant sources, thus lowering the sensitivity required for a successful detection of gravitational waves by detectors like VIRGO, LIGO and LISA.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsGravitational-wave observatoryGravitational waveSpeed of gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGravitational accelerationGeneral Relativity and Quantum CosmologyLIGOGravitational energyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Gravitational fieldGravitational redshiftPhysical Review D
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Acceleration radiation and the Planck scale

2008

A uniformly accelerating observer perceives the Minkowski vacuum state as a thermal bath of radiation. We point out that this field-theory effect can be derived, for any dimension higher than two, without actually invoking very high energy physics. This supports the view that this phenomenon is robust against Planck-scale physics and, therefore, should be compatible with any underlying microscopic theory.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsQuantum field theory in curved spacetime010308 nuclear & particles physicsVacuum stateFOS: Physical sciencesAcceleration (differential geometry)RadiationObserver (physics)01 natural sciencesPartícules (Física nuclear)Classical mechanicsHigh Energy Physics - Theory (hep-th)0103 physical sciencesMinkowski spaceThermalMicroscopic theory010306 general physicsPhysical Review D
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Continuous-variable entanglement sharing in noninertial frames

2007

We study the distribution of entanglement between modes of a free scalar field from the perspective of observers in uniform acceleration. We consider a two-mode squeezed state of the field from an inertial perspective, and analytically study the degradation of entanglement due to the Unruh effect, in the cases of either one or both observers undergoing uniform acceleration. We find that for two observers undergoing finite acceleration, the entanglement vanishes between the lowest frequency modes. The loss of entanglement is precisely explained as a redistribution of the inertial entanglement into multipartite quantum correlations among accessible and unaccessible modes from a non-inertial p…

High Energy Physics - TheoryPhysicsQuantum PhysicsInertial frame of referenceStatistical Mechanics (cond-mat.stat-mech)FOS: Physical sciencesAcceleration (differential geometry)General Relativity and Quantum Cosmology (gr-qc)Quantum PhysicsQuantum entanglementSquashed entanglementGeneral Relativity and Quantum CosmologyAtomic and Molecular Physics and OpticsMultipartiteUnruh effectClassical mechanicsHigh Energy Physics - Theory (hep-th)Quantum mechanicsQuantum Physics (quant-ph)Scalar fieldCondensed Matter - Statistical MechanicsSqueezed coherent state
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Forward acceleration of the centre of mass during ski skating calculated from force and motion capture data

2016

The purpose of this paper was to present and evaluate a methodology to determine the contribution of bilateral leg and pole thrusts to forward acceleration of the centre of mass (COM) of cross-country skiers from multi-dimensional ground reaction forces and motion capture data. Nine highly skilled cross-country (XC) skiers performed leg skating and V2-alternate skating (V2A) under constant environmental conditions on snow, while ground reaction forces measured from ski bindings and poles and 3D motion with high-speed cameras were captured. COM acceleration determined from 3D motion analyses served as a reference and was compared to the results of the proposed methodology. The obtained value…

Highly skilled3d motion analysisMechanical Engineering0206 medical engineeringBiomedical EngineeringPhysical Therapy Sports Therapy and Rehabilitation030229 sport sciences02 engineering and technologyGeodesy020601 biomedical engineeringMotion captureMean differenceMotion (physics)03 medical and health sciencesAcceleration0302 clinical medicineClassical mechanicsPosition (vector)Mechanics of MaterialsModeling and SimulationModelling and SimulationOrthopedics and Sports MedicineGround reaction forceMathematicsSports Engineering
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Carbon nanotubes embedded in a polyimide foil for proton acceleration with a sub-ns laser

2021

A series of thin films made of aligned carbon nanotubes (CNTs) embedded in a polyimide substrate was designed, fabricated and used for the first time to accelerate protons and C ions by interaction with a sub-nanosecond, high power laser beam (600 J energy and 300 ps pulse width) with peak intensity of about 3 × 1016 W/cm2 on target. Each target was 5 μm thick, and the composite material contained CNTs aligned in different directions in the substrate. The results obtained from the analysis of a Thomson Parabola spectrometer, and of the spots imprinted by ions on a series of PM355 nuclear track detectors, indicate high energies (up to 3 MeV for protons and 9 MeV for C ions) and a marked infl…

Ion sources (positive ionsMaterials scienceProtonbusiness.industrySettore ING-IND/20 - Misure E Strumentazione NucleariCarbon nanotubeLaserNegative ionsSettore FIS/03 - Fisica Della Materialaw.inventionElectron beam (EBIS))AccelerationManufacturinglawOptoelectronicsPolyimide foilbusinessElectron cyclotron resonance (ECR)InstrumentationMathematical Physics
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The Highly Collimated Radio Jet of HH 80–81: Structure and Nonthermal Emission

2017

Radio emission from protostellar jets is usually dominated by free-free emission from thermal electrons. However, in some cases, it has been proposed that non-thermal emission could also be present. This additional contribution from non-thermal emission has been inferred through negative spectral indices at centimeter wavelengths in some regions of the radio jets. In the case of HH 80-81, one of the most powerful protostellar jets known, linearly polarized emission has also been detected, revealing that the non-thermal emission is of synchrotron nature from a population of relativistic particles in the jet. This result implies that an acceleration mechanism should be taking place in some pa…

JETS AND OUTFLOWS [ISM]Astrophysics::High Energy Astrophysical PhenomenaCiencias FísicasFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesCollimated lightACCELERATION OF PARTICLES//purl.org/becyt/ford/1 [https]FORMATION [STARS]0103 physical sciences010306 general physics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Astronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]Astrophysics - Astrophysics of GalaxiesAstronomíaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASThe Astrophysical Journal
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Cosmic ray composition and energy spectrum from 1–30 PeV using the 40-string configuration of IceTop and IceCube

2012

Astroparticle physics 42, 15 - 32 (2013). doi:10.1016/j.astropartphys.2012.11.003

Knee regionAstrophysicsTracking (particle physics)01 natural sciencesParticle identificationIceCubeTRACKINGWATERCherenkovNeutrino energyNEUTRINO TELESCOPEUltra-high-energy cosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSEADetectorAstrophysics::Instrumentation and Methods for AstrophysicsLIGHTComposition; Cosmic rays; Energy spectrum; IceCube; IceTop; Knee regionddc:540IceTopPARTICLE IDENTIFICATIONAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsIceCube detectorCompositionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayddc:500.2IceCube Neutrino ObservatorySEARCHESAccelerationcosmic raysdE/dx0103 physical sciences010306 general physicsDETECTORInstrumentation and Methods for Astrophysics (astro-ph.IM)Cherenkov radiationTruncated meanMuon energy010308 nuclear & particles physicsAstronomyAstronomy and Astrophysics540Physics and AstronomycompositionEnergy SpectrumTEVEnergy spectrum
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Architecture-Driven Level Set Optimization: From Clustering to Sub-pixel Image Segmentation

2016

Thanks to their effectiveness, active contour models (ACMs) are of great interest for computer vision scientists. The level set methods (LSMs) refer to the class of geometric active contours. Comparing with the other ACMs, in addition to subpixel accuracy, it has the intrinsic ability to automatically handle topological changes. Nevertheless, the LSMs are computationally expensive. A solution for their time consumption problem can be hardware acceleration using some massively parallel devices such as graphics processing units (GPUs). But the question is: which accuracy can we reach while still maintaining an adequate algorithm to massively parallel architecture? In this paper, we attempt to…

Level set methodComputer science0211 other engineering and technologiesInitialization02 engineering and technology[ SPI.SIGNAL ] Engineering Sciences [physics]/Signal and Image processingLevel setgraphics processing units0202 electrical engineering electronic engineering information engineeringLevel set methodComputer visionElectrical and Electronic EngineeringCluster analysisMassively parallelimage segmentation021101 geological & geomatics engineeringActive contour modelhybrid CPU-GPU architecturebusiness.industryImage segmentationSubpixel renderingComputer Science ApplicationsHuman-Computer InteractionControl and Systems EngineeringHardware acceleration020201 artificial intelligence & image processingArtificial intelligencebusiness[SPI.SIGNAL]Engineering Sciences [physics]/Signal and Image processingSoftwareInformation Systems
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Signs and transitions: Do they differ phonetically and does it matter?

2013

The point of departure of this article is the cluster of three pre-theoretical presuppositions (P) governing modern research on sign languages: (1) that a stream of signing consists of signs (S) and transitions (T), (2) that only Ss are linguistically relevant units, and (3) that there is a qualitative (e.g., phonetic) difference between Ss and Ts. Of these, the article focuses on the relatively untested P3, which is used to back up P1 and P2, and investigates the velocity and acceleration properties of Ss and Ts on the basis of continuous motion-capture data from Finnish Sign Language. The main finding of the study is that the speed of Ss is slower (and varies less) than that of Ts but tha…

Linguistics and LanguageAccelerationInterpretation (logic)PhonologyPhoneticsta6121Sign languagePsychologyLanguage and LinguisticsLinguisticsMotion (physics)PresuppositionSign (mathematics)Sign Language Studies
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