Search results for "PLASMA"

showing 10 items of 4043 documents

Spectral Evolution of the X-Ray Remnant of SN 1987A: A High-Resolution $Chandra$ HETG Study

2021

Based on observations with the $Chandra$ X-ray Observatory, we present the latest spectral evolution of the X-ray remnant of SN 1987A (SNR 1987A). We present a high-resolution spectroscopic analysis using our new deep ($\sim$312 ks) $Chandra$ HETG observation taken in March 2018, as well as archival $Chandra$ gratings spectroscopic data taken in 2004, 2007, and 2011 with similarly deep exposures ($\sim$170 - 350 ks). We perform detailed spectral model fits to quantify changing plasma conditions over the last 14 years. Recent changes in electron temperatures and volume emission measures suggest that the shocks moving through the inner ring have started interacting with less dense circumstell…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Supernovae (1668)Astrophysics::High Energy Astrophysical PhenomenaSupernova remnants (1667)Resolution (electron density)FluxFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsElectronPlasmaIonSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceObservatoryAstrophysics - High Energy Astrophysical PhenomenaEjectaCircumstellar matter (241)Interstellar medium (847)Line (formation)
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Excitation spectra of solitary waves in scalar field models with polynomial self-interaction

2016

We study excitations of solitary waves -- the kinks -- in scalar models with degree eight polynomial self-interaction in (1+1) dimensions. We perform numerical studies of scattering of two kinks with an exponential asymptotic off each other and analyse the occurring resonance phenomena. We connect these phenomena to the energy exchange between the translational and the vibrational modes of the colliding kinks. We also point out that the interaction of two kinks with power-law asymptotic can lead to a long-range interaction between the two kinks.

PhysicsHigh Energy Physics - TheoryHistoryPolynomialDegree (graph theory)ScatteringScalar (mathematics)FOS: Physical sciencesMathematical Physics (math-ph)Pattern Formation and Solitons (nlin.PS)01 natural sciencesResonance (particle physics)Nonlinear Sciences - Pattern Formation and Solitons010305 fluids & plasmasComputer Science ApplicationsEducationExponential functionClassical mechanicsHigh Energy Physics - Theory (hep-th)Molecular vibration0103 physical sciences010306 general physicsScalar fieldNonlinear Sciences::Pattern Formation and SolitonsMathematical Physics
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On Central Charges and Hamiltonians for 0-brane dynamics

1999

We consider general properties of central charges of zero branes and associated duality invariants, in view of their double role, on the bulk and on the world volume (quantum-mechanical) theory. A detailed study of the BPS condition for the mass spectrum arising from toroidal compactifications is given for 1/2, 1/4 and 1/8 BPS states in any dimensions. As a byproduct, we retreive the U-duality invariant conditions on the charge (zero mode) spectrum and the orbit classification of BPS states preserving different fractions of supersymmetry. The BPS condition for 0-branes in theories with 16 supersymmetries in any dimension is also discussed.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsZero modeSupergravityFOS: Physical sciencesDuality (optimization)FísicaCharge (physics)SupersymmetryTheoretical physicsHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)Physics::Plasma PhysicsQuantum mechanicsBraneOrbit (control theory)Invariant (mathematics)Mathematics::Symplectic GeometryParticle Physics - Theory
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Derivation of transient relativistic fluid dynamics from the Boltzmann equation

2012

In this work we present a general derivation of relativistic fluid dynamics from the Boltzmann equation using the method of moments. The main difference between our approach and the traditional 14-moment approximation is that we will not close the fluid-dynamical equations of motion by truncating the expansion of the distribution function. Instead, we keep all terms in the moment expansion. The reduction of the degrees of freedom is done by identifying the microscopic time scales of the Boltzmann equation and considering only the slowest ones. In addition, the equations of motion for the dissipative quantities are truncated according to a systematic power-counting scheme in Knudsen and inve…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy Physicsta114Nuclear TheoryDegrees of freedom (physics and chemistry)Lattice Boltzmann methodsEquations of motionFOS: Physical sciencesMethod of moments (statistics)Plasma modelingBoltzmann equationNuclear Theory (nucl-th)Physics::Fluid DynamicsHigh Energy Physics - PhenomenologyClassical mechanicsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Direct simulation Monte CarloKnudsen number
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Flavor vacuum entanglement in boson mixing

2021

Mixing transformations in quantum field theory are non-trivial, since they are intimately related to the unitary inequivalence between Fock spaces for fields with definite mass and fields with definite flavor. Considering the superposition of two neutral scalar (spin-0) bosonic fields, we investigate some features of the emerging condensate structure of the flavor vacuum. In particular, we quantify the flavor vacuum entanglement in terms of the von Neumann entanglement entropy of the reduced state. Furthermore, in a suitable limit, we show that the flavor vacuum has a structure akin to the thermal vacuum of Thermo Field Dynamics, with a temperature dependent on both the mixing angle and the…

PhysicsHigh Energy Physics - TheoryQuantum PhysicsField (physics)Scalar (physics)FOS: Physical sciencesQuantum entanglement01 natural sciences010305 fluids & plasmasFock spaceEntropy (classical thermodynamics)High Energy Physics - Theory (hep-th)Quantum mechanics0103 physical sciencesQuantum field theoryQuantum Physics (quant-ph)010306 general physicsMixing (physics)Boson
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First-order flows and stabilisation equations for non-BPS extremal black holes

2011

28 páginas.-- This article is distributed under the terms of the Creative Commons Attribution Noncommercial License.

PhysicsHigh Energy Physics - TheorySupergravity modelsNuclear and High Energy Physics010308 nuclear & particles physicsSupergravityFOS: Physical sciencesCharge (physics)Black holes in string theoryFirst order01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)Flow (mathematics)Harmonic functionPhysics::Plasma Physics0103 physical sciences010306 general physicsMathematical physicsAnsatzJournal of High Energy Physics
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Production of thermal dileptons in high energy nucleus-nucleus collisions

1989

A method for including realistic nuclear geometry and impact parameter effects in computations of production rates of thermal dileptons of mass in the 1.5 to 3 GeV range andy≈0 in nucleus nucleus collisions at $$\sqrt s = 20 - 200$$ GeV is given. A comparison with the Drell-Yan rate indicates that for large nuclei and energies thermal production gives a sizable contribution even atM=M Jψ and thus may contribute significantly toJ/ψ suppression as background enchancement.

PhysicsHigh energyRange (particle radiation)Particle physicsPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsPlasma01 natural sciencesNuclear physicsmedicine.anatomical_structure0103 physical sciencesThermalmedicineImpact parameter010306 general physicsEngineering (miscellaneous)NucleusZeitschrift f�r Physik C Particles and Fields
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Anomalous properties of hot dense nonequilibrium plasmas

2005

A concise overview of a number of anomalous properties of hot dense nonequilibrium plasmas is given. The possibility of quasistationary megagauss magnetic field generation due to Weibel instability is discussed for plasmas created in atom tunnel ionization. The collisionless absorption and reflection of a test electromagnetic wave normally impinging on the plasma with two-temperature bi-maxwellian electron velocity distribution function are studied. Due to the wave magnetic field influence on the electron kinetics in the skin layer the wave absorption and reflection significantly depend on the degree of the electron temperature anisotropy. The linearly polarized impinging wave during reflec…

PhysicsHistoryElectronPlasmaElliptical polarizationElectromagnetic radiationComputer Science ApplicationsEducationWeibel instabilityTunnel ionizationPhysics::Plasma PhysicsIonizationElectromagnetic electron waveAtomic physics
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The dynamics of bunched laser-cooled ion beams at relativistic energies

2007

We discuss the axial dynamics of laser-cooled relativistic C3+ ion beams at moderate bunching voltages. Schottky noise spectra measured at a beam energy of 122 MeV/u are compared to simulations of the axial beam dynamics. Ions confined in the bucket are addressed by the narrow-band force of a laser beam counter-propagating to the ion beam, while the laser frequency is detuned relatively to the cooling transition frequency in the rest frame of the bucket. At large detuning comparable to the momentum acceptance of the bucket, the axial dynamics can be well explained by the secular motion of individual non-interacting ions. At small detuning, corresponding to a small axial momentum spread Δpax…

PhysicsHistoryIon beamRest frameIon gunKinetic energyComputer Science ApplicationsEducationIonMomentumPhysics::Plasma PhysicsPhysics::Accelerator PhysicsAtomic physicsBeam (structure)Noise (radio)Journal of Physics: Conference Series
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Numerical test of finite-size scaling predictions for the droplet condensation-evaporation transition

2016

We numerically study the finite-size droplet condensation-evaporation transition in two dimensions. We consider and compare two orthogonal approaches, namely at fixed temperature and at fixed density, making use of parallel multicanonical simulations. The equivalence between Ising model and lattice gas allows us to compare to analytical predictions. We recover the known background density (at fixed temperature) and transition temperature (at fixed density) in the thermodynamic limit and compare our finite-size deviations to the predicted leading-order finite-size corrections.

PhysicsHistoryStatistical Mechanics (cond-mat.stat-mech)010308 nuclear & particles physicsTransition temperatureFOS: Physical sciencesCondensed Matter - Soft Condensed Matter01 natural sciences010305 fluids & plasmasComputer Science ApplicationsEducationLattice (order)0103 physical sciencesThermodynamic limitSoft Condensed Matter (cond-mat.soft)Ising modelNumerical testsStatistical physicsScalingCondensed Matter - Statistical Mechanics
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