Search results for "Theoretical Physics"

showing 10 items of 751 documents

Revised periodic boundary conditions: Fundamentals, electrostatics, and the tight-binding approximation

2011

Many nanostructures today are low-dimensional and flimsy, and therefore get easily distorted. Distortion-induced symmetry-breaking makes conventional, translation-periodic simulations invalid, which has triggered developments for new methods. Revised periodic boundary conditions (RPBC) is a simple method that enables simulations of complex material distortions, either classically or quantum-mechanically. The mathematical details of this easy-to-implement approach, however, have not been discussed before. Therefore, in this paper we summarize the underlying theory, present the practical details of RPBC, especially related to a non-orthogonal tight-binding formulation, discuss selected featur…

PhysicsCondensed Matter - Materials Scienceta114Materials Science (cond-mat.mtrl-sci)FOS: Physical sciences02 engineering and technologyComputational Physics (physics.comp-ph)021001 nanoscience & nanotechnologyCondensed Matter PhysicsElectrostatics01 natural sciencesSoftware implementation3. Good healthElectronic Optical and Magnetic MaterialsTheoretical physicsTight bindingSimple (abstract algebra)0103 physical sciencesPeriodic boundary conditions010306 general physics0210 nano-technologyPhysics - Computational PhysicsPhysical Review B
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Preparing single ultra-cold antihydrogen atoms for free-fall in GBAR

2014

We discuss an experimental approach allowing to prepare antihydrogen atoms for the GBAR experiment. We study the feasibility of all necessary experimental steps: The capture of incoming $\bar{\rm H}^{+}$ ions at keV energies in a deep linear RF trap, sympathetic cooling by laser cooled Be+ ions, transfer to a miniaturized trap and Raman sideband cooling of an ion pair to the motional ground state, and further reducing the momentum of the wavepacket by adiabatic opening of the trap. For each step, we point out the experimental challenges and discuss the efficiency and characteristic times, showing that capture and cooling are possible within a few seconds. We discuss an experimental approach…

PhysicsCondensed Matter::Quantum GasesSympathetic coolingOther Fields of Physics7. Clean energyphysics.atom-phIonMomentumquant-ph13. Climate actionAntimatterPhysics::Atomic PhysicsAtomic physicsAdiabatic processGround stateAntihydrogenGeneral Theoretical PhysicsBar (unit)
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Poincaré's role in the Crémieu-Pender controversy over electric convection

1989

Summary In the course of 1901, V. Cremieu published the results of some experiments carried out to test the magnetic effects of electric convection currents. According to Cremieu, his experiments had proved that convection currents had no magnetic effects and consequently they were not equivalent to conduction currents, that is they were not ‘real’ electric currents. These negative results conflicted with those of well-known experiments carried out by other researchers, in particular with Rowland's experiments, and with Maxwell's, Hertz's and Lorentz's theories, which was more shocking. The publication of Cremieu's experiments raised a controversy which involved directly or indirectly some …

PhysicsConvectionsymbols.namesakeTheoretical physicsHistory and Philosophy of ScienceLorentz transformationHertzQuantum electrodynamicsPoincaré conjecturesymbolsElectric currentThermal conductionAnnals of Science
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Correlation dimension and affinity of AE data and bicolored noise

1993

This paper is concerned with the general question of the dynamics of the magnetosphere. In general, to solve the dynamics of the magnetosphere one has to solve magnetohydrodynamic equations with some appropriate set of boundary conditions. This results in a very complex solution, which gives indications of being chaotic. The question of the chaotic nature of the magnetospheric dynamics has been addressed by various authors by looking at the correlation dimension of the auroral electrojet index. There has been disagreement on the outcome of such experiments, so the authors report on a detailed analysis of the auroral electrojet index time series. They find a correlation dimension of 3.4. For…

PhysicsCorrelation dimensionSeries (mathematics)ChaoticElectrojetMagnetosphereTheoretical physicsGeophysicsFractalColors of noisePhysics::Space PhysicsSubstormGeneral Earth and Planetary SciencesStatistical physicsGeophysical Research Letters
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On the sources of the late integrated Sachs-Wolfe effect

2000

In some scenarios, the peculiar gravitational potential of linear and mildly nonlinear structures depends on time and, as a result of this dependence, a late integrated Sachs-Wolfe effect appears. Here, an appropriate formalism is used which allows us to improve on the analysis of the spatial scales and locations of the main cosmological inhomogeneities producing this effect. The study is performed in the framework of the currently preferred flat model with cosmological constant, and it is also developed in an open model for comparisons. Results from this analysis are used to discuss the contribution of Great Attractor-like objects, voids, and other structures to the CMB anisotropy.

PhysicsCosmic microwave backgroundAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsCosmological constantAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSachs–Wolfe effectAstrophysicsNonlinear systemGravitational potentialTheoretical physicsFormalism (philosophy of mathematics)Space and Planetary ScienceOpen modelAnisotropyInstrumentation
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Dark sectors with dynamical coupling

2019

Coupled dark matter-dark energy scenarios are modeled via a dimensionless parameter $��$, which controls the strength of their interaction. While this coupling is commonly assumed to be constant, there is no underlying physical law or symmetry that forbids a time-dependent $��$ parameter. The most general and complete interacting scenarios between the two dark sectors should therefore allow for such a possibility, and it is the main purpose of this study to constrain two possible and well-motivated coupled cosmologies by means of the most recent and accurate early and late-time universe observations. We find that CMB data alone prefers $��(z) >0$ and therefore a smaller amount of dark ma…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsmedia_common.quotation_subjectDark matterCosmic microwave backgroundFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsCoupling (probability)01 natural sciencesSymmetry (physics)UniverseGeneral Relativity and Quantum CosmologyTheoretical physics0103 physical sciences010306 general physicsConstant (mathematics)Energy (signal processing)media_commonDimensionless quantityAstrophysics - Cosmology and Nongalactic Astrophysics
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More about a successful vector-tensor theory of gravitation

2016

The vector-tensor (VT) theory of gravitation revisited in this article was studied in previous papers, where it was proved that VT works and deserves attention. New observational data and numerical codes have motivated further development which is presented here. New research has been planed with the essential aim of proving that current cosmological observations, including Planck data, baryon acoustic oscillations (BAO), and so on, may be explained with VT, a theory which accounts for a kind of dark energy which has the same equation of state as vacuum. New versions of the codes CAMB and COSMOMC have been designed for applications to VT, and the resulting versions have been used to get the…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Current (mathematics)010308 nuclear & particles physicsGeneral relativityEquation of state (cosmology)FOS: Physical sciencesValue (computer science)Astronomy and Astrophysics01 natural sciencesGravitationsymbols.namesakeTheoretical physics0103 physical sciencesDark energysymbolsBaryon acoustic oscillationsPlanck010303 astronomy & astrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Exponents of non-linear clustering in scale-free one-dimensional cosmological simulations

2012

One dimensional versions of cosmological N-body simulations have been shown to share many qualitative behaviours of the three dimensional problem. They can resolve a large range of time and length scales, and admit exact numerical integration. We use such models to study how non-linear clustering depends on initial conditions and cosmology. More specifically, we consider a family of models which, like the 3D EdS model, lead for power-law initial conditions to self-similar clustering characterized in the strongly non-linear regime by power-law behaviour of the two point correlation function. We study how the corresponding exponent \gamma depends on the initial conditions, characterized by th…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesSpectral densityAstronomy and AstrophysicsCosmologyNumerical integrationMetric expansion of spaceUniversality (dynamical systems)Nonlinear systemTheoretical physicsSpace and Planetary ScienceExponentStatistical physicsCluster analysisAstrophysics - Cosmology and Nongalactic AstrophysicsMonthly Notices of the Royal Astronomical Society
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On the viability of a certain vector-tensor theory of gravitation

2010

A certain vector-tensor theory is revisited. Our attention is focused on cosmology. Against previous suggestions based on preliminary studies, it is shown that, if the energy density of the vector field is large enough to play the role of the dark energy and its fluctuations are negligible, the theory is not simultaneously compatible with current observations on: supernovae, the cosmic microwave background (CMB) anisotropy, and the power spectrum of the energy density fluctuations. However, for small enough energy densities of the vector field, the theory becomes compatible with all the above observations and, moreover, it leads to an interesting evolution of the so-called vector cosmologic…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityCosmic microwave backgroundFOS: Physical sciencesSpectral densityAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsCosmologyGravitationTheoretical physicsSpace and Planetary ScienceDark energyVector fieldAnisotropyAstrophysics - Cosmology and Nongalactic AstrophysicsAstrophysics and Space Science
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Induced gravity and the attractor dynamics of dark energy/dark matter

2010

Attractor solutions that give dynamical reasons for dark energy to act like the cosmological constant, or behavior close to it, are interesting possibilities to explain cosmic acceleration. Coupling the scalar field to matter or to gravity enlarges the dynamical behavior; we consider both couplings together, which can ameliorate some problems for each individually. Such theories have also been proposed in a Higgs-like fashion to induce gravity and unify dark energy and dark matter origins. We explore restrictions on such theories due to their dynamical behavior compared to observations of the cosmic expansion. Quartic potentials in particular have viable stability properties and asymptotica…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityDark matterFOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsCosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum CosmologyMetric expansion of spaceTheoretical physicsAttractorDark energyScalar fieldInduced gravityAstrophysics - Cosmology and Nongalactic Astrophysics
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