Search results for "Names"

showing 10 items of 6843 documents

Gravito-magnetic vacuum spacetimes: kinematic restrictions

2003

We show that there are no vacuum solutions with a purely magnetic Weyl tensor with respect to an observer submitted to kinematic restrictions involving first order differential scalars. This result generalizes previous ones for the vorticity-free and shear-free cases. We use a covariant approach which makes evident that only the Bianchi identities are used and, consequently, the results are also valid for non vacuum solutions with vanishing Cotton tensor.

PhysicsWeyl tensorPhysics and Astronomy (miscellaneous)Cotton tensorFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)KinematicsFirst orderObserver (physics)General Relativity and Quantum Cosmologysymbols.namesakeGeneral Relativity and Quantum CosmologysymbolsCovariant transformationDifferential (mathematics)Mathematical physics
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Obtaining the Weyl tensor from the Bel-Robinson tensor

2010

The algebraic study of the Bel-Robinson tensor proposed and initiated in a previous work (Gen. Relativ. Gravit. {\bf 41}, see ref [11]) is achieved. The canonical form of the different algebraic types is obtained in terms of Bel-Robinson eigen-tensors. An algorithmic determination of the Weyl tensor from the Bel-Robinson tensor is presented.

PhysicsWeyl tensorPhysics and Astronomy (miscellaneous)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum Cosmologysymbols.namesakeGeneral Relativity and Quantum CosmologyTensor (intrinsic definition)symbolsAlgebraic data typeCanonical formAlgebraic numberMathematics::Representation TheoryMathematical physics
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Connection between the pinch technique and the background field method

1995

The connection between the pinch technique and the background field method is further explored. We show by explicit calculations that the application of the pinch technique in the framework of the background field method gives rise to exactly the same results as in the linear renormalizable gauges. The general method for extending the pinch technique to the case of Green's functions with off-shell fermions as incoming particles is presented. As an example, the one-loop gauge independent quark self-energy is constructed. We briefly discuss the possibility that the gluonic Green's functions, obtained by either method, correspond to physical quantities.

PhysicsWilson loop010308 nuclear & particles physicsBackground field methodHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaPropagator01 natural sciencesHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Self-energyQuantum electrodynamics0103 physical sciencesPinchsymbolsFeynman diagram010306 general physicsS-matrixPhysical quantityPhysical Review D
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Three-body correlations and conditional forces in suspensions of active hard disks

2017

Self-propelled Brownian particles show rich out-of-equilibrium physics, for instance, the motility-induced phase separation (MIPS). While decades of studying the structure of liquids have established a deep understanding of passive systems, not much is known about correlations in active suspensions. In this work we derive an approximate analytic theory for three-body correlations and forces in systems of active Brownian disks starting from the many-body Smoluchowski equation. We use our theory to predict the conditional forces that act on a tagged particle and their dependence on the propulsion speed of self-propelled disks. We identify preferred directions of these forces in relation to th…

PhysicsWork (thermodynamics)Collective behaviorSmoluchowski coagulation equationNon-equilibrium thermodynamicsFOS: Physical sciencesContext (language use)02 engineering and technologyFunction (mathematics)Condensed Matter - Soft Condensed Matter021001 nanoscience & nanotechnology01 natural sciencessymbols.namesakeRange (mathematics)0103 physical sciencessymbolsSoft Condensed Matter (cond-mat.soft)Statistical physics010306 general physics0210 nano-technologyBrownian motion
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Analytical Expressions for Radiative Losses in Solar Cells

2019

Analytical expressions for the fundamental losses in single junction solar cells are revised and improved. The losses are, as far as possible, described using parameters with clear physical interpretations. One important improvement compared to earlier work is the use of Lambert’s W function, which allows for analytical expressions for the voltage and current at the maximum power point. Other improvements include the use of Stefan Boltzmann’s law to describe the incoming energy flux as well as taking into account the fermionic nature of the electrons when calculating the thermalization loss. A new expression, which combines emission, Boltzmann and Carnot losses, is presented. Finally, an ex…

PhysicsWork (thermodynamics)Stefan–Boltzmann lawMaximum power principleEnergy flux02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesExpression (mathematics)Computational physicssymbols.namesake0103 physical sciencesBoltzmann constantsymbolsRadiative transfer010306 general physics0210 nano-technologyCarnot cycle2019 IEEE 46th Photovoltaic Specialists Conference (PVSC)
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A Preliminary Analysis of a New Chandra Observation (ObsID 6148) of Cir X-1

2008

We present the preliminary spectral analysis of a 25 ks long Chandra observation of the peculiar source Cir X–1 near the periastron passage. We estimate more precise coordinates of the source compatible with the optical and radio counterpart coordinates. We detect emission lines associated to Mg XII, Si XIII, Si XIV, S XV, S XVI Ar XVII, Ar XVIII, Ca XIX, Ca XX, Fe XXV, Fe XXVI showing a redshift of 470 km s−1. The more intense emission features at 6.6 keV show a double‐peaked shape that can be modelled with two or three Gaussian lines.

PhysicsX-ray binaries Accretion and accretion disks Neutron stars Distances redshifts radial velocities; spatial distribution of galaxies Black holesX-ray binaries Accretion and accretion disks Neutron stars Distances redshifts radial velocitieGaussianX-ray binaryAstronomyAstrophysicsRedshiftPreliminary analysisRed shiftNeutron starsymbols.namesakeSettore FIS/05 - Astronomia E AstrofisicasymbolsSpectral analysisEmission spectrumspatial distribution of galaxies Black holes
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The BeppoSAX 0.1–18 keV spectrum of the bright atoll source GX 9+1: an indication of the source distance

2005

We report the results of a long, 350 ks, BeppoSAX observation of the bright atoll source GX 9+1 in the 0.12-18 keV energy range. During this observation GX 9+1 showed a large count rate variability in its lightcurve. From its color-color diagram we selected six zones and extracted the source energy spectrum from each zone. We find that the model, composed of a blackbody plus a Comptonized component absorbed by an equivalent hydrogen column of ~1.4 ¿ 1022 cm-2, fits the spectra in the energy range 1-18 keV well; however, below 1 keV a soft excess is present. We find that the spectrum of GX 9+1, in the 0.12-18 keV energy range, is well fitted by the model above, if we use an equivalent hydrog…

PhysicsX-ray binaryAstronomyAstronomy and AstrophysicsAstrophysicsLight curveSpectral lineLuminosityInterstellar mediumNeutron starStarssymbols.namesakeSpace and Planetary ScienceEddington luminositysymbolsAstronomy & Astrophysics
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Atomic transitions of Rb, D2 line in strong magnetic fields: Hyperfine Paschen–Back regime

2014

An efficient $\lambda/2$-method ($\lambda$ is the resonant wavelength of laser radiation) based on nanometric-thickness cell filled with rubidium is implemented to study the splitting of hyperfine transitions of $^{85}$Rb and $^{87}$Rb $D_2$ lines in an external magnetic field in the range of $B =3$~kG -- 7~kG. It is experimentally demonstrated that at $B > 3$~kG from 38 (22) Zeeman transitions allowed at low $B$-field in $^{85}$Rb ($^{87}$Rb) spectra in the case of $\sigma^+$ polarized laser radiation there remain only 12 (8) which is caused by decoupling of the total electronic momentum $\textbf{J}$ and the nuclear spin momentum $\textbf{I}$ (hyperfine Paschen-Back regime). Note that at $…

PhysicsZeeman effectAtomic Physics (physics.atom-ph)FOS: Physical scienceschemistry.chemical_elementAtomic and Molecular Physics and OpticsSpectral linePhysics - Atomic Physics3. Good healthElectronic Optical and Magnetic MaterialsRubidiumMagnetic fieldMomentumsymbols.namesakeWavelengthchemistrysymbolsPhysics::Atomic PhysicsElectrical and Electronic EngineeringPhysical and Theoretical ChemistryAtomic physicsHyperfine structureLine (formation)Optics Communications
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Hyperfine Paschen-Back regime in alkali metal atoms: consistency of two theoretical considerations and experiment

2013

Simple and efficient "\lambda-method" and "\lambda/2-method" (\lambda is the resonant wavelength of laser radiation) based on nanometric-thickness cell filled with rubidium are implemented to study the splitting of hyperfine transitions of 85Rb and 87Rb D_1 line in an external magnetic field in the range of B = 0.5 - 0.7 T. It is experimentally demonstrated from 20 (12) Zeeman transitions allowed at low B-field in 85Rb (87Rb) spectra in the case of \sigma+ polarized laser radiation, only 6 (4) remain at B > 0.5 T, caused by decoupling of the total electronic momentum J and the nuclear spin momentum I (hyperfine Paschen-Back regime). The expressions derived in the frame of completely uncoupl…

PhysicsZeeman effectAtomic Physics (physics.atom-ph)chemistry.chemical_elementFOS: Physical sciencesStatistical and Nonlinear Physics01 natural sciencesAtomic and Molecular Physics and OpticsSpectral line3. Good healthRubidiumMagnetic fieldPhysics - Atomic Physics010309 opticsMomentumWavelengthsymbols.namesakechemistry0103 physical sciencessymbolsPhysics::Atomic PhysicsAtomic physics010306 general physicsHyperfine structureCircular polarization
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Validity of rate equations for Zeeman coherences for analysis of nonlinear interaction of atoms with broadband laser radiation

2004

In this paper we, to our knowledge, for the first time obtain the rate equations for Zeeman coherences in the broad line approximation and steady-state balance equations directly from optical Bloch equations without the use of the perturbation theory. The broad line approximation allows us to use the adiabatic elimination procedure in order to eliminate the optical coherences from the optical Bloch equations, but the steady-state condition allows us to derive the balance equations straightforward. We compare our approach with the perturbation theory approach as given previously and show that our approach is more flexible in analyzing various experiments. Meanwhile we also show the validity …

PhysicsZeeman effectBasis (linear algebra)Atomic Physics (physics.atom-ph)FOS: Physical sciencesRate equationAtomic and Molecular Physics and OpticsPhysics - Atomic PhysicsNonlinear systemsymbols.namesakeBloch equationsQuantum electrodynamicsQuantum mechanicssymbolsPerturbation theoryAdiabatic processExcitationPhysical Review A
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