Search results for "symmetry"

showing 10 items of 3576 documents

Widespread Nanoflare Variability Detected with Hinode/X-Ray Telescope in a Solar Active Region

2011

It is generally agreed that small impulsive energy bursts called nanoflares are responsible for at least some of the Sun's hot corona, but whether they are the explanation for most of the multimillion-degree plasma has been a matter of ongoing debate. We present here evidence that nanoflares are widespread in an active region observed by the X-Ray Telescope on board the Hinode mission. The distributions of intensity fluctuations have small but important asymmetries, whether taken from individual pixels, multipixel subregions, or the entire active region. Negative fluctuations (corresponding to reduced intensity) are greater in number but weaker in amplitude, so that the median fluctuation i…

Physicsmedia_common.quotation_subjectAstronomy and AstrophysicsAstrophysicsPlasmaactivity Sun: corona Sun: X-rays gamma rays [Sun]Poisson distributionCoronaAsymmetryIntensity (physics)Nanoflareslaw.inventionTelescopesymbols.namesakeAmplitudeSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary SciencelawPhysics::Space PhysicssymbolsSun: activity Sun: corona Sun: X-rays gamma raysAstrophysics::Solar and Stellar Astrophysicsmedia_common
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Very peculiar wind from BD+53°2790, the optical counterpart to 4U 2206+54

2008

BD+53 2790, an O9.5Vp star, is the optical counterpart to the HMXRB 4U 2206+54. This system was classified initially as a BeX, but observational evidence soon stressed the need to revise this classification. The permanent asymmetry in the H-alpha line profiles (in contrast with the cyclic variations shown by Be stars), the variations in the profile of this line in time scales of hours (while time scales from weeks to months are expected in Be stars), and the lack of correlation between IR observables and H-alpha line parameters, strongly suggest that, while BD+53 2790 contains a circunstellar disc, it is not like the one present in Be stars. Furthermore, there is evidence of overabundance o…

Physicsmedia_common.quotation_subjectAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsObservableAstrophysicsStar (graph theory)AstrophysicsAsymmetryUnexpected findingStarsObservational evidenceSpace and Planetary Sciencemedia_commonLine (formation)Astrophysics and Space Science
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Charge Form Factor of the Neutron at Low Momentum Transfer from theH→2(e→,e′n)H1Reaction

2008

We report new measurements of the neutron charge form factor at low momentum transfer using quasielastic electrodisintegration of the deuteron. Longitudinally polarized electrons at an energy of 850 MeV were scattered from an isotopically pure, highly polarized deuterium gas target. The scattered electrons and coincident neutrons were measured by the Bates Large Acceptance Spectrometer Toroid (BLAST) detector. The neutron form factor ratio ${G}_{E}^{n}/{G}_{M}^{n}$ was extracted from the beam-target vector asymmetry ${A}_{\mathrm{ed}}^{V}$ at four-momentum transfers ${Q}^{2}=0.14$, 0.20, 0.29, and $0.42\text{ }\text{ }(\mathrm{GeV}/c{)}^{2}$.

Physicsmedia_common.quotation_subjectNuclear TheoryMomentum transferForm factor (quantum field theory)General Physics and AstronomyCharge (physics)ElectronAsymmetryDeuteriumHigh Energy Physics::ExperimentNeutronAtomic physicsNuclear ExperimentEnergy (signal processing)media_commonPhysical Review Letters
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Optical pumping and unstable nuclei

1985

The paper reviews the application of optical pumping to short-lived nuclei, where either the nuclear polarisation is detected by the β-decay asymmetry or the atomic polarisation by Stern-Gerlach-analyzer. Moreover the paper deals with collinear laser spectroscopy on beams of short-lived, mass-separated isotopes. The aim of the experiments is the systematic investigation of nuclear structure through the determination of spin, moments and charge radii from the hyperfine structure and isotopic shift of the atomic spectra. The impact of these experiments on the theory of nuclear forces and structure is discussed by means of a few examples.

Physicsmedia_common.quotation_subjectNuclear structureGeneral Physics and AstronomyAsymmetryOptical pumpingIsotopic shiftNuclear forcePhysics::Atomic PhysicsAtomic physicsNuclear ExperimentSpin (physics)SpectroscopyHyperfine structuremedia_commonAnnales de Physique
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Asymmetric balance in symmetry breaking

2020

Spontaneous symmetry breaking is central to our understanding of physics and explains many natural phenomena, from cosmic scales to subatomic particles. Its use for applications requires devices with a high level of symmetry, but engineered systems are always imperfect. Surprisingly, the impact of such imperfections has barely been studied, and restricted to a single asymmetry. Here, we experimentally study spontaneous symmetry breaking with two controllable asymmetries. We remarkably find that features typical of spontaneous symmetry breaking, while destroyed by one asymmetry, can be restored by introducing a second asymmetry. In essence, asymmetries are found to balance each other. Our st…

Physicsmedia_common.quotation_subjectSpontaneous symmetry breakingFOS: Physical sciencesPattern Formation and Solitons (nlin.PS)Polarization (waves)Nonlinear Sciences - Pattern Formation and SolitonsAsymmetryNonlinear Sciences - Adaptation and Self-Organizing SystemsNonlinear systemTheoretical physicsPitchfork bifurcationSymmetry breakingSubatomic particleAdaptation and Self-Organizing Systems (nlin.AO)QCBifurcationPhysics - OpticsOptics (physics.optics)media_commonPhysical Review Research
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Use of site symmetry in supercell models of defective crystals: Polarons in CeO2

2017

The authors thank R. Merkle and G. W. Watson for stimulating discussions. E. K. also acknowledges partial financial support from the Russian Science Foundation for the study of charged defects under the project 14-43-00052. A. C. also acknowledges financial support from the University of Latvia Foundation (Arnis Riekstins's "MikroTik" donation). E. K. and D. G. express their gratitude to the High Performance Computer Centre in Stuttgart (HLRS, project DEFTD 12939) for the provided computer facilities whereas R. A. E. thanks the St. Petersburg State University Computer Center for assistance in high-performance calculations.

PhysicspolaronCondensed matter physicssite symmetryGeneral Physics and Astronomy02 engineering and technologyoxygen vacancy021001 nanoscience & nanotechnologyPolaron01 natural sciencesCrystallographic defectSymmetry (physics)Condensed Matter::Materials SciencePerfect crystalLinear combination of atomic orbitalsPosition (vector)Vacancy defect0103 physical sciences:NATURAL SCIENCES:Physics [Research Subject Categories]Wyckoff positionsPhysical and Theoretical Chemistry010306 general physics0210 nano-technologyfirst principles calculationsCeO2
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ASY-EOS experiment at GSI

2012

The elliptic-flow ratio of neutrons with respect to protons in reactions of neutron rich Heavy-Ion at intermediate energies has been recently proposed as an observable sensitive to the strength of the symmetry term in the nuclear equation of state (EOS) at supra-saturation densities. The recent results obtained from the existing FOPI/LAND data for 197Au+197Au collisions at 400 MeV/nucleon in comparison with the UrQMD model allowed a first estimate of the symmetry term of the EOS but suffer from a considerable statistical uncertainty. In order to obtain an improved data set for Au+Au collisions and to extend the study to other systems, a new experiment was carried out at the GSI laboratory b…

PhysicssezelePhysicsQC1-999Nuclear Theorysymmetry energyObservableNuclear equation of state[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]nuclear equation of stateSymmetry (physics)Term (time)Nuclear physicsPhysics and Astronomy (all)nucleus-nucleus collisionsNeutronNucleonNuclear ExperimentEPJ Web of Conferences
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Effects of non-uniform interstellar magnetic field on synchrotron X-ray and inverse-Compton γ-ray morphology of supernova remnants

2011

Context. Observations of SuperNova Remnants (SNRs) in X-ray and γ-ray bands promise to contribute important information to our understanding of the kinematics of charged particles and magnetic fields in the vicinity of strong non-relativistic shocks and, therefore, the nature of Galactic cosmic rays. The accurate analysis of SNR images collected in different energy bands requires theoretical modeling of synchrotron and inverse Compton emission from SNRs. Aims. We develop a numerical code (remlight) to synthesize, from MHD simulations, the synchrotron radio, X-ray, and inverse Compton γ-ray emission originating in SNRs expanding in a non-uniform interstellar medium (ISM) and/or non-uniform i…

Physicsshock waveAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectGamma rayAstronomy and AstrophysicsCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsElectronradiation mechanisms: non-thermalAsymmetrymagnetohydrodynamics (MHD)SynchrotronX-rays: ISMComputational physicsMagnetic fieldlaw.inventionInterstellar mediumgamma rays: ISMSpace and Planetary SciencelawMagnetohydrodynamicsAstrophysics::Galaxy AstrophysicsISM: supernova remnantmedia_common
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Asymptotic structure factor for the two-component Ginzburg-Landau equation

1992

We derive an analytic form for the asymptotic time-dependent structure factor for the two-component Ginzburg-Landau equation in arbitrary dimensions. This form is in reasonable agreement with results from numerical simulations in two dimensions. A striking feature of our analytic form is the absence of Porod's law in the tail. This is a consequence of the continuous symmetry of the Hamiltonian, which inhibits the formation of sharp domain walls.

Physicssymbols.namesakeContinuous symmetryDynamic structure factorsymbolsGinzburg landau equationGeneral Physics and AstronomyStructure factorHamiltonian (quantum mechanics)Mathematical physicsPhysics Letters A
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The Pauli Principle and Systems Consisting of Composite Particles

1993

In nature we often deal with many-body systems that are described in terms of particles that are not elementary but themselves composite. Examples of such composite particles are hadrons, atoms, phonons, and Cooper pairs. For the description of systems consisting of such composite particles in terms of the underlying degrees of freedom group theory plays an important role, in particular the symmetric group to describe the permutational symmetry of the wave function of the system, and unitary groups to describe the symmetry forced on the system by the interaction between the particles.

Physicssymbols.namesakeTheoretical physicsPauli exclusion principleSymmetric groupsymbolsDegrees of freedom (physics and chemistry)Cooper pairPermutation groupWave functionGroup theorySymmetry (physics)
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