Search results for "electrodynamics"

showing 10 items of 820 documents

Mapping nonlinear gravity into General Relativity with nonlinear electrodynamics

2018

We show that families of nonlinear gravity theories formulated in a metric-affine approach and coupled to a nonlinear theory of electrodynamics can be mapped into General Relativity (GR) coupled to another nonlinear theory of electrodynamics. This allows to generate solutions of the former from those of the latter using purely algebraic transformations. This correspondence is explicitly illustrated with the Eddington-inspired Born-Infeld theory of gravity, for which we consider a family of nonlinear electrodynamics and show that, under the map, preserve their algebraic structure. For the particular case of Maxwell electrodynamics coupled to Born-Infeld gravity we find, via this corresponden…

Gravity (chemistry)Physics and Astronomy (miscellaneous)Algebraic structureGeneral relativityFOS: Physical scienceslcsh:AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationlcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)Metric-affine approachPhysics010308 nuclear & particles physicsNumerical analysisNonlinear theoryPower (physics)Nonlinear gravity theoriesNonlinear systemQuantum electrodynamicslcsh:QC770-798Regular Article - Theoretical Physics
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Computational general relativistic force-free electrodynamics

2021

Scientific codes are an indispensable link between theory and experiment; in (astro-)plasma physics, such numerical tools are one window into the universe's most extreme flows of energy. The discretization of Maxwell's equations - needed to make highly magnetized (astro)physical plasma amenable to its numerical modeling - introduces numerical diffusion. It acts as a source of dissipation independent of the system's physical constituents. Understanding the numerical diffusion of scientific codes is the key to classify their reliability. It gives specific limits in which the results of numerical experiments are physical. We aim at quantifying and characterizing the numerical diffusion propert…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsDiscretizationWaves in plasmasFOS: Physical sciencesAstronomy and AstrophysicsContext (language use)PlasmaComputational Physics (physics.comp-ph)Numerical diffusionDissipation01 natural sciencesMagnetic fieldCurrent sheetSpace and Planetary ScienceQuantum electrodynamics0103 physical sciencesAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysics010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics - Computational Physics010303 astronomy & astrophysicsAstronomy & Astrophysics
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Computational general relativistic force-free electrodynamics

2020

General relativistic force-free electrodynamics is one possible plasma-limit employed to analyze energetic outflows in which strong magnetic fields are dominant over all inertial phenomena. The amazing images of black hole shadows from the galactic center and the M87 galaxy provide a first direct glimpse into the physics of accretion flows in the most extreme environments of the universe. The efficient extraction of energy in the form of collimated outflows or jets from a rotating BH is directly linked to the topology of the surrounding magnetic field. We aim at providing a tool to numerically model the dynamics of such fields in magnetospheres around compact objects, such as black holes an…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsInertial frame of referenceActive galactic nucleus010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaGalactic CenterFOS: Physical sciencesSpherical coordinate systemAstronomy and AstrophysicsComputational Physics (physics.comp-ph)Magnetar01 natural sciencesGalaxyBlack holeNeutron starSpace and Planetary ScienceQuantum electrodynamics0103 physical sciencesAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics - Computational Physics010303 astronomy & astrophysicsAstronomy & Astrophysics
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Looking at the axionic dark sector with ANITA

2020

The ANITA experiment has recently observed two anomalous events emerging from well below the horizon. Even though they are consistent with tau cascades, a high energy Standard Model or Beyond the Standard Model explanation is challenging and in tension with other experiments. We study under which conditions the reflection of generic radio pulses can reproduce these signals. We propose that these pulses can be resonantly produced in the ionosphere via axion-photon conversion. This naturally explains the direction and polarization of the events and avoids other experimental bounds.

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsPhysics beyond the Standard ModelFOS: Physical scienceslcsh:AstrophysicsPolarization (waves)01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Quantum electrodynamicslcsh:QB460-4660103 physical scienceslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityIonosphereAstrophysics - High Energy Astrophysical Phenomena010306 general physicsEngineering (miscellaneous)Astronomia ObservacionsThe European Physical Journal C
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The force-free twisted magnetosphere of a neutron star – II. Degeneracies of the Grad–Shafranov equation

2017

We extend our previous study of equilibrium solutions of non-rotating force-free magnetospheres of neutron stars. We show that multiple solutions exist for the same sets of parameters, implying that the solutions are degenerate. We are able to obtain configurations with disconnected field lines, however, in nearly all cases these correspond to degenerate higher energy solutions. We carry out a wide parametric search in order to understand the properties of the solutions. We confirm our previous results that the lower energy solutions have up to $\sim 25\%$ more energy than the vacuum case, helicity of the order of $\sim 5$ (in some defined units), maximum twist of $\sim 1.5$ rad, and a dipo…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsWork (thermodynamics)MHDFOS: Physical sciencesMagnetosphereneutron [Stars]Astronomy and Astrophysics01 natural sciencesMagnetic fieldmagnetars [Stars]magnetic field [Stars]Neutron starGrad–Shafranov equationClassical mechanicsSpace and Planetary ScienceMagnetic fieldsQuantum electrodynamics0103 physical sciencesCost actionMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena010306 general physics010303 astronomy & astrophysicsAstronomía y AstrofísicaMonthly Notices of the Royal Astronomical Society
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Analytic Form of the Two-Loop Planar Five-Gluon All-Plus-Helicity Amplitude in QCD

2015

Virtual two-loop corrections to scattering amplitudes are a key ingredient to precision physics at collider experiments. We compute the full set of planar master integrals relevant to five-point functions in massless QCD, and use these to derive an analytical expression for the two-loop five-gluon all-plus-helicity amplitude. After subtracting terms that are related to the universal infrared and ultraviolet pole structure, we obtain a remarkably simple and compact finite remainder function, consisting only of dilogarithms.

High Energy Physics - Theory530 PhysicsFOS: Physical sciencesGeneral Physics and Astronomy10192 Physics Institute01 natural scienceslaw.inventionHigh Energy Physics - Phenomenology (hep-ph)law0103 physical sciences010306 general physicsColliderMathematical physicsPhysicsQuantum chromodynamics010308 nuclear & particles physicsHelicity3100 General Physics and AstronomyGluonScattering amplitudeLoop (topology)Massless particleHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics - Theory (hep-th)Quantum electrodynamicsPhysical Review Letters
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Numerical observation of Hawking radiation from acoustic black holes in atomic Bose–Einstein condensates

2008

We report numerical evidence of Hawking emission of Bogoliubov phonons from a sonic horizon in a flowing one-dimensional atomic Bose-Einstein condensate. The presence of Hawking radiation is revealed from peculiar long-range patterns in the density-density correlation function of the gas. Quantitative agreement between our fully microscopic calculations and the prediction of analog models is obtained in the hydrodynamic limit. New features are predicted and the robustness of the Hawking signal against a finite temperature discussed.

High Energy Physics - TheoryCondensed Matter::Quantum GasesPhysicsPhononHorizonFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum Cosmologylaw.inventionCondensed Matter - Other Condensed MatterGeneral Relativity and Quantum CosmologyCorrelation function (statistical mechanics)HawkingHigh Energy Physics - Theory (hep-th)lawQuantum electrodynamicsBose–Einstein condensateOther Condensed Matter (cond-mat.other)Hawking radiationNew Journal of Physics
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Narrowing the window of inflationary magnetogenesis

2017

We consider inflationary magnetogenesis where the conformal symmetry is broken by the term $f^2(\phi) F_{\alpha\beta} F^{\alpha\beta}$. We assume that the magnetic field power spectrum today between 0.1 and $10^4$ Mpc is a power law, with upper and lower limits from observation. This fixes $f$ to be close to a power law in conformal time in the window during inflation when the modes observed today are generated. In contrast to previous work, we do not make any assumptions about the form of $f$ outside these scales. We cover all possible reheating histories, described by an average equation of state $-1/3 <\bar{w} <1$. Requiring that strong coupling and large backreaction are avoided both at…

High Energy Physics - TheoryCosmology and Nongalactic Astrophysics (astro-ph.CO)gr-qcprimordial magnetic fieldsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesPower law114 Physical sciencesGeneral Relativity and Quantum CosmologyConformal symmetry0103 physical sciencesinflation010303 astronomy & astrophysicsSTFCST/L005573/1ComputingMilieux_MISCELLANEOUSInflation (cosmology)Physics[PHYS]Physics [physics]010308 nuclear & particles physicsEquation of state (cosmology)hep-thRCUKCONSTRAINTSAstronomy and Astrophysics115 Astronomy Space scienceMagnetic fieldOrders of magnitude (time)High Energy Physics - Theory (hep-th)Quantum electrodynamicsCOSMOLOGYSCALE MAGNETIC-FIELDSastro-ph.COBack-reactionST/K00090X/1Order of magnitudeAstrophysics - Cosmology and Nongalactic Astrophysics
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Axionic and nonaxionic electrodynamics in plane and circular geometry

2023

Various aspects of axion electrodynamics in the presence of a homogeneous and isotropic dielectric medium are discussed. 1. We consider first the "antenna-like" property of a planar dielectric surface in axion electrodynamics, elaborating on the treatment given earlier on this topic by Millar {\it et al.} (2017). We calculate the electromagnetic energy transmission coefficient for a dielectric plate, and compare with the conventional expression in ordinary electrodynamics. 2. We consider the situation where the medium exterior to the plate, assumed elastic, is "bent back" and glued together, so that we obtain a circular dielectric string in which the waves can propagate clockwise or counter…

High Energy Physics - TheoryCp conservationSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciHigh Energy Physics - Theory (hep-th)Casimir energyFOS: Physical sciencesAxion Axion Electrodynamics Dark Matter Relativistic aspects of CosmologySettore FIS/04 - Fisica Nucleare E Subnucleare114 Physical sciencesSettore FIS/03 - Fisica Della Materia
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Vacuum energy densities of a field in a cavity with a mobile boundary

2015

We consider the zero-point field fluctuations, and the related field energy densities, inside a one-dimensional and a three-dimensional cavity with a mobile wall. The mechanical degrees of freedom of the mobile wall are described quantum mechanically and they are fully included in the overall system dynamics. In this optomechanical system, the field and the wall can interact with each other through the radiation pressure on the wall, given by the photons inside the cavity or even by vacuum fluctuations. We consider two cases: the one-dimensional electromagnetic field and the three-dimensional scalar field, and use the Green's functions formalism, which allows extension of the results obtain…

High Energy Physics - TheoryElectromagnetic fieldPhysicsQuantum PhysicsNuclear and High Energy PhysicsPhotonQuantum Optomechanics Vacuum Fluctuations Vacuum Energy DensitiesZero-point energyFOS: Physical sciencesRadiation pressureVacuum energyHigh Energy Physics - Theory (hep-th)Quantum electrodynamicsQuantum Physics (quant-ph)Scalar fieldCavity wallQuantum fluctuation
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