Search results for "UAS"

showing 10 items of 1619 documents

Dynamically screened vertex correction to $GW$

2020

Diagrammatic perturbation theory is a powerful tool for the investigation of interacting many-body systems, the self-energy operator $\mathrm{\ensuremath{\Sigma}}$ encoding all the variety of scattering processes. In the simplest scenario of correlated electrons described by the $GW$ approximation for the electron self-energy, a particle transfers a part of its energy to neutral excitations. Higher-order (in screened Coulomb interaction $W$) self-energy diagrams lead to improved electron spectral functions (SFs) by taking more complicated scattering channels into account and by adding corrections to lower order self-energy terms. However, they also may lead to unphysical negative spectral f…

PhysicsSettore FIS/03Strongly Correlated Electrons (cond-mat.str-el)Operator (physics)Vertex functionFOS: Physical sciences02 engineering and technologyPositive-definite matrix021001 nanoscience & nanotechnology01 natural sciencestiiviin aineen fysiikkaCondensed Matter - Strongly Correlated Electronssymbols.namesakeQuantum mechanics0103 physical sciencesCoulombsymbolsQuasiparticleFermi's golden rulePerturbation theory (quantum mechanics)approksimointikvanttifysiikka010306 general physics0210 nano-technologyFermi gas
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Multi-wavelength VLBI phase-delay astrometry of a complete sample of radio sources

2007

AbstractWe report on the first global high-precision (differential phase-delay) astrometric analyses performed on a complete set of radio sources. We have observed the S5 polar cap sample, consisting of 13 quasars and BL Lac objects, with the VLBA at 8.4, 15, and 43 GHz. We have developed new algorithms to enable the use of the differential phase-delay observable in global astrometric observations. From our global analyses, we determine the relative positions between all pairs of sources with typical precisions ranging from 10 to 200 μas, depending on observing frequency and source separation. In this paper, we discuss the impact of this observable in the enhancement of the astrometric prec…

PhysicsSpace and Planetary ScienceVery-long-baseline interferometrySource separationAstronomyAstronomy and AstrophysicsObservableRangingQuasarAstrophysicsAstrometryStability (probability)Group delay and phase delayProceedings of the International Astronomical Union
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Hyperboloidal slicing approach to quasinormal mode expansions: The Reissner-Nordström case

2018

We study quasi-normal modes of black holes, with a focus on resonant (or quasi-normal mode) expansions, in a geometric frame based on the use of conformal compactifications together with hyperboloidal foliations of spacetime. Specifically, this work extends the previous study of Schwarzschild in this geometric approach to spherically symmetric asymptotically flat black hole spacetimes, in particular Reissner-Nordstr\"om. The discussion involves, first, the non-trivial technical developments needed to address the choice of appropriate hyperboloidal slices in the extended setting as well as the generalization of the algorithm determining the coefficients in the expansion of the solution in te…

PhysicsSpacetime010308 nuclear & particles physicsGeneral relativitynumbers: 0425dgCauchy distributionalternative theories of gravityConformal map04.30.-w16. Peace & justice01 natural sciencesSlicingGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum Cosmology02.30.MvGeneral relativityRegularization (physics)0103 physical sciencesQuasinormal mode[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]010306 general physicsSchwarzschild radiusPhysical Review D
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All good things come in threes: the third image of the lensed quasar PKS1830-211

2020

Strong gravitational lensing distorts our view of sources at cosmological distances but brings invaluable constraints on the mass content of foreground objects and on the geometry and properties of the Universe. We report the detection of a third continuum source toward the strongly lensed quasar PKS1830-211 in ALMA multi-frequency observations of high dynamic range and high angular resolution. This third source is point-like and located slightly to the north of the diagonal joining the two main lensed images, A and B, 0.3 arcsec away from image B. It has a flux density that is ~140 times weaker than images A and B and a similar spectral index, compatible with synchrotron emission. We concl…

PhysicsSpectral indexCosmology and Nongalactic Astrophysics (astro-ph.CO)Einstein ring010308 nuclear & particles physicsContinuum (design consultancy)Strong gravitational lensingFOS: Physical sciencesAstronomy and AstrophysicsQuasarAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - Astrophysics of Galaxies01 natural sciencessymbols.namesakeSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencessymbolsMillimeterAngular resolution010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's law
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Absolute kinematics of radio source components in the complete S5 polar cap sample

2004

We observed the thirteen extragalactic radio sources of the complete S5 polar cap sample at 15.4 GHz with the Very Long Baseline Array, on 27 July 1999 (1999.57) and 15 June 2000 (2000.46). We present the maps from those two epochs, along with maps obtained from observations of the 2 cm VLBA survey for some of the sources of the sample, making a total of 40 maps. We discuss the apparent morphological changes displayed by the radio sources between the observing epochs. Our VLBA observations correspond to the first two epochs at 15.4 GHz of a program to study the absolute kinematics of the radio source components of the members of the sample, by means of phase delay astrometry at 8.4 GHz, 15.…

PhysicsSpectral indexInterferometricAstronomy and AstrophysicsAstrometryKinematicsAstrometryAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAGalaxies:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Sample (graphics)Radio continuumSpace and Planetary ScienceBL Lacertae objectsAstrometry ; Interferometric ; Galaxies ; Quasars ; BL Lacertae objects ; Radio continuumUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaPolar capQuasars:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Very Long Baseline ArrayGroup delay and phase delayAstronomy & Astrophysics
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Discovery of a quasi-periodic oscillation in the X-ray pulsar 1A 1118-615: correlated spectral and aperiodic variability

2010

Aims. Our goal is to investigate the X-ray timing and spectral variability of the high-mass X-ray binary 1A 1118-615 during a type-II outburst. Methods. We performed a detailed color, spectral, and timing analysis of a giant outburst from 1A 1118-615 using RXTE data. Results. We report the discovery of a variable quasi-periodic oscillation (QPO) in the power spectral density of 1A 1118-615, with a centroid frequency of ∼0.08 Hz. The centroid frequency of the QPO correlates with the X-ray flux, as expected according to the most accredited models for QPO production. For energies above ∼4 keV, the QPO rms variability decreases as the energy increases. Pulse profiles display an energy dependenc…

PhysicsSpectral indexQuasi-periodic oscillation010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaX-ray binarySpectral densityFluxAstronomy and AstrophysicsAstrophysics01 natural sciencesNeutron starPulsarSpace and Planetary Science0103 physical sciences010303 astronomy & astrophysicsX-ray pulsarAstronomy & Astrophysics
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X-Ray Spectral Variability of 3C273

1985

3C273 has been monitored by EXOSAT over the period December 1983 to June 1984 in 4 observations. In the December observation the flux was high and the spectrum showed a power law index of 1.5 changing to 0.9 at~8 keV. In subsequent observations the flux dropped to~40% of its original value and the hard tail disappeared. In the last observation the LE flux increased by a factor of 2 with no accompanying ME flux increase.

PhysicsSpectral indexX-ray astronomyX-rayCompton scatteringAstronomyFluxQuasarAstrophysicsPower lawX ray spectra
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Evolution from γ -soft to stable triaxiality in Nd136 as a prerequisite of chirality

2018

The level structure of Nd136 has been investigated using the Mo100(Ar40,4n) reaction and the JUROGAM II+RITU+GREAT setup. The level scheme has been extended significantly. Many new bands have been identified both at low and high spin, among which are five nearly degenerate bands interpreted as chiral partners. Excitation energies, spins, and parities of the previously known bands are revised and firmly established, and some previously known bands have been revised. Configurations are assigned to the observed bands based on cranked Nilsson-Strutinsky calculations. The band structure of Nd136 is now clarified and the various types of single-particle and collective excitations are well underst…

PhysicsSpins010308 nuclear & particles physicsDegenerate energy levelsNuclear structure01 natural sciencesMolecular physics0103 physical sciencesQuasiparticleLevel structure010306 general physicsElectronic band structureExcitationSpin-½Physical Review C
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Thermal localizable entanglement in a simple multipartite system

2009

The quantum correlations present in a system of three coupled spins 12 in a thermal state are investigated. Localizable entanglement, as well as concurrence function, is exactly evaluated. The results obtained show the existence of a temperature range corresponding to which it is impossible to localize entanglement.

PhysicsSpinsConcurrenceQuantum PhysicsQuantum entanglementCondensed Matter PhysicsSquashed entanglementMultipartite entanglementAtomic and Molecular Physics and OpticsMultipartiteQuantum mechanicsW stateQuantumMathematical Physicsentanglement spin systems
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AN OPTICAL PLAQUETTE: MINIMUM EXPRESSIONS OF TOPOLOGICAL MATTER

2009

Topological matter is an unconventional form of matter: it exhibits a global hidden order which is not associated with the spontaneous breaking of any symmetry. The defects of this exotic type of order are anyons, quasiparticles with fractional statistics. Moreover, when living on a surface with non-trivial topology, like a plane with a hole or a torus, this type of matter develops a number of degenerate states which are locally indistinguishable and could be used to build a quantum memory naturally resistant to errors. Except for the fractional quantum Hall effect there is no experimental evidence as to the existence of topologically ordered phases, and it remains a huge challenge to devel…

PhysicsSpinsQuantum mechanicsDegenerate energy levelsFractional quantum Hall effectQuasiparticleTopological orderQuantum Hall effectTopologyTopological quantum computerQuantum dimer modelsPushing the Frontiers of Atomic Physics
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