Search results for "Names"

showing 10 items of 6843 documents

Numerical evolution of matter in dynamical axisymmetric black hole spacetimes

2000

We have developed a numerical code to study the evolution of self-gravitating matter in dynamic black hole axisymmetric spacetimes in general relativity. The matter fields are evolved with a high-resolution shock-capturing scheme that uses the characteristic information of the general relativistic hydrodynamic equations to build up a linearized Riemann solver. The spacetime is evolved with an axisymmetric ADM code designed to evolve a wormhole in full general relativity. We discuss the numerical and algorithmic issues related to the effective coupling of the hydrodynamical and spacetime pieces of the code, as well as the numerical methods and gauge conditions we use to evolve such spacetime…

PhysicsSpacetimeGeneral relativityGravitational waveAstrophysics::High Energy Astrophysical PhenomenaNumerical analysisRotational symmetryGeneral Physics and AstronomyRiemann solverBlack holeGeneral Relativity and Quantum Cosmologysymbols.namesakeClassical mechanicsHardware and ArchitecturesymbolsWormholeComputer Physics Communications
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Variation of physical constants and electron–positron oscillations: Zitterbewegung in a plane wave

2021

The space and time dependence of physical constants is currently a debated issue for experimental findings, and theoretical reasons seem to indicate that this is not a mere speculative possibility. The paper provides a relativistic description of a free fermion evolving under the assumption of temporal variation of the physical constants. The assumed generalisation of the Dirac equation is particularly simple and permits a grouping of the constants in one single parameter and a consequent agile treatment of the problem. The form of the equations suggests a rescaling of the temporal coordinate $$x^0=ct$$ which allows a plane wave solution. Two are the main results of the treatment. First, th…

PhysicsSpacetimePhysical constantOscillationPhysical constantPlane waveGeneral Physics and AstronomyElectronFermionsymbols.namesakeParticle PhysicQuantum electrodynamicsDirac equationsymbolsZitterbewegungDirac equation
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Spatial correlation of laser-generated electrons and holes in quantum wells

1995

The spatial correlation of hot electrons and holes generated by light in a semiconductor quantum well (QW) is studied. For hot electron-hole pairs in a polar material, this correlation is determined by the interaction with LO-phonons. We analyze the distribution F N (r, K) of electrons and holes which are created in a given light absorption process, with respect to their relative separation r and total quasimomentum ħK, after the emission of a number N of LO-phonons. The relationship between the spatial distribution of electrons and holes in these intermediate states and the cross-section of multi-phonon resonant Raman scattering (MPRRS) is established. Spatial correlation effects are stron…

PhysicsSpatial correlationbusiness.industryQuantum-confined Stark effectElectronCondensed Matter PhysicsLaserSpatial distributionElectronic Optical and Magnetic Materialslaw.inventionsymbols.namesakeSemiconductorlawsymbolsAtomic physicsbusinessRaman scatteringQuantum wellphysica status solidi (b)
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The Wigner Distribution of Sum-of-Cissoids and Sum-of-Chirps Processes for the Modelling of Stationary and Non-Stationary Mobile Channels

2016

This paper concerns the time-frequency analysis of stationary and non-stationary multipath flat fading channels. For the modelling of stationary multipath fading channels, we use a sum-of-cisoids (SOCi) process, while the non-stationary channel is modelled by a sum-of-chirps (SOCh) process that captures the time-variant Doppler effect caused by speed variations of the mobile station. For the time-frequency analysis, we apply the concept of the Wigner distribution. Closed-form solutions are provided for the Wigner distribution of SOCi and SOCh processes. It is shown that the obtained Wigner distributions can be expressed by the sum of an auto-term representing the true Doppler power spectral…

PhysicsSpectral density020206 networking & telecommunications020302 automobile design & engineering02 engineering and technologyTime–frequency analysissymbols.namesake0203 mechanical engineeringMobile stationComputer Science::Networking and Internet Architecture0202 electrical engineering electronic engineering information engineeringsymbolsElectronic engineeringWigner distribution functionFadingStatistical physicsDoppler effectRandom variableMultipath propagationComputer Science::Information Theory2016 IEEE 83rd Vehicular Technology Conference (VTC Spring)
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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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The rotational gas-phase spectrum of trans- and cis-HSSOH at 100GHz

2009

Abstract We present the first pure rotational spectra of the two most stable conformers of oxatrisulfane, trans- and cis-HSSOH, in their vibrational ground state. For both conformers a-, b-, and c-type transitions have been recorded in the range from 75 to 120 GHz using an all solid-state spectrometer. More than 200 lines have been assigned for each conformer, most of them belonging to the r Q 2 - and the r Q 3 -branch of the perpendicular spectra. The least-squares fit analysis using a semirigid rotor Hamiltonian in S-reduction yields precise values for the ground-state rotational constants A 0 = 21 145.93422 ( 66 ) , B 0 = 4479.92301 ( 21 ) , C 0 = 3828.34269 ( 21 ) for cis-HSSOH, and A 0…

PhysicsSpectrometerAtomic and Molecular Physics and OpticsSpectral lineDipolesymbols.namesakeNuclear magnetic resonanceQuartic functionsymbolsRotational spectroscopyPhysical and Theoretical ChemistryAtomic physicsGround stateHamiltonian (quantum mechanics)Conformational isomerismSpectroscopyJournal of Molecular Spectroscopy
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Shape coexistence in neutron-deficient Hg188 investigated via lifetime measurements

2020

Background: Shape coexistence in the Z≈82 region has been established in mercury, lead, and polonium isotopes. For even-even mercury isotopes with 100≤N≤106 multiple fingerprints of this phenomenon are observed, which seems to be no longer present for N≥110. According to a number of theoretical calculations, shape coexistence is predicted in the Hg188 isotope. Purpose: The aim of this work was to measure lifetimes of excited states in Hg188 to infer their collective properties, such as the deformation. Extending the investigation to higher-spin states, which are expected to be less affected by band-mixing effects, can provide additional information on the coexisting structures. Methods: The…

PhysicsSpectrometerIsotope010308 nuclear & particles physicsNuclear structurechemistry.chemical_element01 natural sciences7. Clean energyMolecular physicssymbols.namesakemedicine.anatomical_structurechemistryExcited state0103 physical sciencesmedicinesymbolsNeutron010306 general physicsHamiltonian (quantum mechanics)NucleusPolonium
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Hyperfine structure study of atomic niobium with enhanced sensitivity of Fourier transform spectroscopy

2011

In an experimental setup with a high-resolution Fourier transform (FT) spectrometer and a hollow-cathode discharge, bandpass interference filters are used to enhance the sensitivity. This extension leads to an improvement of the signal-to-noise ratio in the spectrum of atomic niobium by a factor of up to 10 compared to FT spectra measured previously without filters (see Kroger et al 2010 Astron. Astrophys. 516 A70). Several additional spectral lines with low intensity have been observed. Additionally, in some intense lines, blends become visible due to the better signal-to-noise ratio. The hyperfine structure of 51 lines recorded in the wavelength range from 415 to 670 nm is analysed or re-…

PhysicsSpectrometerNiobiumchemistry.chemical_elementCondensed Matter PhysicsAtomic and Molecular Physics and OpticsFourier transform spectroscopySpectral linesymbols.namesakeFourier transformchemistrysymbolsAtomic physicsSpectroscopyHyperfine structureVisible spectrumJournal of Physics B: Atomic, Molecular and Optical Physics
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Generalized Langevin dynamics: construction and numerical integration of non-Markovian particle-based models.

2018

We propose a generalized Langevin dynamics (GLD) technique to construct non-Markovian particle-based coarse-grained models from fine-grained reference simulations and to efficiently integrate them. The proposed GLD model has the form of a discretized generalized Langevin equation with distance-dependent two-particle contributions to the self- and pair-memory kernels. The memory kernels are iteratively reconstructed from the dynamical correlation functions of an underlying fine-grained system. We develop a simulation algorithm for this class of non-Markovian models that scales linearly with the number of coarse-grained particles. Our GLD method is suitable for coarse-grained studies of syste…

PhysicsSpeedup010304 chemical physicsDiscretizationFOS: Physical sciencesMarkov processGeneral ChemistryCondensed Matter - Soft Condensed MatterComputational Physics (physics.comp-ph)Condensed Matter Physics01 natural sciencesNumerical integrationsymbols.namesake0103 physical sciencessymbolsSoft Condensed Matter (cond-mat.soft)ParticleSoft matterStatistical physics010306 general physicsLangevin dynamicsPhysics - Computational PhysicsOrder of magnitudeSoft matter
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Ising Spin-Glass on a Lattice with Small Loops

1991

We consider the Ising spin-glass on a special lattice containing small loops with finite coordination number c. We derive the equation for the effective field distribution. With zero external field, we calculate the spin-glass transition temperature and obtain the lower critical dimension of the system. We investigate the system near and below the spin-glass transition and find that the replica symmetric solution is unstable in the low-temperature phase. Our results indicate that the replica symmetry breaking (RSB) effects are stronger than that of the Bethe lattice and furthermore, RSB is enhanced as the dimension (c/2) is decreased. Comparison with recent results of the 1/d expansion is a…

PhysicsSpin glassBethe latticeCondensed matter physicsTransition temperatureGeneral Physics and AstronomyCondensed Matter::Disordered Systems and Neural Networkssymbols.namesakeLattice (order)symbolsIsing modelSymmetry breakingHamiltonian (quantum mechanics)Critical dimensionEurophysics Letters (EPL)
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