Search results for "Derivative"

showing 10 items of 1074 documents

Quantized Fields and Their Interpretation

2013

This chapter deals with the quantum theory of systems with an infinite number of degrees of freedom and provides elements of quantum field theory.

PhysicsInfinite numberClassical mechanicsPath integral formulationDegrees of freedomFunctional derivativeQuantum field theoryInterpretation (model theory)
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Nonlinear Evolution Equations, Quasi-Solitons and their Experimental Manifestation

1990

We review the typical experimental facts which characterize quasisolitons in one-dimensional real systems, in connection with their modeling by nonlinear partial differential equations.We consider these nonlinear waves or excitations in two different domains of the real world : the macroworld and the microworld. In the macroworld we examine typical one-dimensional devices : the electrical networks, the Josephson transmission lines and the optical fibers, where the localized waves or pulses can be simply and coherently created, easily observed and manipulated on a macroscopic scale. In the microworld, we consider the magnetic chains and polymers, where the indirect experimental signatures of…

PhysicsNonlinear systemElectric power transmissionClassical mechanicsField (physics)Transmission lineMacroscopic scaleConnection (vector bundle)Partial derivativeToda lattice
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Renormalization of the 1S0 One-Pion-Exchange NN Interaction in Presence of Derivative Contact Interactions

2003

We use standard distorted wave theory techniques and dimensional regularization to find out solutions of the nucleon-nucleon Lippman--Schwinger equation with a kernel determined by the Weinberg's next-to-leading potential, which consists of one--pion exchange and additional contact terms with derivatives. Though for simplicity, we restrict the discussion to the $^1S_0$ channel and to contact terms containing up to two derivatives, the generalization to higher waves and/or number of derivatives is straightforward. The undetermined low energy constants emerging out of the renormalization procedure are fitted to data.

PhysicsNuclear and High Energy PhysicsNuclear TheoryGeneralizationPartial wave analysisFísicaFOS: Physical sciencesRenormalizationNuclear Theory (nucl-th)Dimensional regularizationHigh Energy Physics - PhenomenologyLow energyPionHigh Energy Physics - Phenomenology (hep-ph)Derivative (finance)Quantum electrodynamicsNuclear theoryMathematical physics
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QUANTIZATION CONDITION FOR HIGHLY EXCITED STATES

1999

We develop a quantization condition for the excited states of simple quantum-mechanical models. The approach combines perturbation theory for the oscillatory part of the eigenfunction with a rational approximation to the logarithmic derivative of the nodeless part of it. We choose one-dimensional anharmonic oscillators as illustrative examples.

PhysicsNuclear and High Energy PhysicsQuantization (physics)Excited stateQuantum mechanicsAnharmonicityGeneral Physics and AstronomyAstronomy and AstrophysicsLogarithmic derivativeEigenfunctionModern Physics Letters A
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Zu notwendigen Resonanzkriterien im station�ren Einkanal-Fall

1975

First will be exhibited, for the stationary case, a connection between the probability, to find a particle in the region of interaction, and the derivative of the scattering phase shift for the momentum. From the idea, that in stationary scattering a resonance is linked with an appreciable increase of this probability, one obtains new and quantitative criteria for the behavior ofδl(k). For instance, the nonresonant behavior can be characterised by the condition 2kdδl(k)/dk<1. The maximum of probability for the particle to be in the region of interaction, is considered in accordance with the criterium of maximal change of the phase shift, as a function ofk. This characterises the location of…

PhysicsNuclear and High Energy PhysicsScatteringbusiness.industryDerivativeFunction (mathematics)CollisionResonance (particle physics)Connection (mathematics)MomentumCross section (physics)OpticsQuantum mechanicsbusinessZeitschrift f�r Physik A Atoms and Nuclei
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Fractional-order theory of heat transport in rigid bodies

2014

Abstract The non-local model of heat transfer, used to describe the deviations of the temperature field from the well-known prediction of Fourier/Cattaneo models experienced in complex media, is framed in the context of fractional-order calculus. It has been assumed (Borino et al., 2011 [53] , Mongiovi and Zingales, 2013 [54] ) that thermal energy transport is due to two phenomena: ( i ) A short-range heat flux ruled by a local transport equation; ( ii ) A long-range thermal energy transfer proportional to a distance-decaying function, to the relative temperature and to the product of the interacting masses. The distance-decaying function is assumed in the functional class of the power-law …

PhysicsNumerical AnalysisField (physics)business.industryApplied MathematicsFractional derivatives; Fractional-order calculus; Fractional-order derivatives; Generalized entropies; Molecular dynamics simulations; Nonlocal; Relative temperatures; Thermal energy transportThermodynamicsContext (language use)Fractional derivativeFractional-order calculuFractional calculusRelative temperatureHeat fluxModeling and SimulationHeat transferGeneralized entropieMolecular dynamics simulationFractional-order derivativeBoundary value problembusinessConvection–diffusion equationNonlocalSettore ICAR/08 - Scienza Delle CostruzioniThermal energyThermal energy transport
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Timing of the 2008 outburst of SAX J1808.4–3658 with XMM-Newton: a stable orbital-period derivative over ten years

2009

We report on a timing analysis performed on a 62-ks long XMM-Newton observation of the accreting millisecond pulsar SAX J1808.4-3658 during the latest X-ray outburst that started on September 21, 2008. By connecting the time of arrivals of the pulses observed during the XMM observation, we derived the best-fit orbital solution and a best-fit value of the spin period for the 2008 outburst. Comparing this new set of orbital parameters and, in particular, the value of the time of ascending-node passage with the orbital parameters derived for the previous four X-ray outbursts of SAX J1808.4-3658 observed by the PCA on board RXTE, we find an updated value of the orbital period derivative, which …

PhysicsOrbital elementsAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesSecular evolutionAstronomy and AstrophysicsAstrophysicsDerivativeOrbital periodstars: neutron stars: magnetic fields X-rays: binaries X-rays: individuals: SAX J1808.4-3658Astrophysics - Astrophysics of GalaxiesLuminosityNeutron starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceMillisecond pulsarAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstronomy &amp; Astrophysics
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Revised orbital parameters of the accreting millisecond pulsar SAX J1808.4-3658

2005

We present temporal analysis of the three outbursts of the X-ray millisecond pulsar SAX J1808.4-3658 that occurred in 1998, 2000 and 2002. With a technique that uses the chi^2 obtained with an epoch folding search to discriminate between different possible orbital solutions, we find an unique solution valid over the whole five years period for which high temporal resolution data are available. We revise the estimate of the orbital period, P_orb =7249.1569(1) s and reduce the corresponding error by one order of magnitude with respect to that previously reported. Moreover we report the first constraint on the orbital period derivative, -6.6 x 10^-12 &lt; Pdot &lt; +0.8 x 10^-12 s/s. These val…

PhysicsOrbital elementsEpoch (astronomy)Astrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsDerivativeOrbital periodAstrophysicsPulse (physics)Orb (astrology)Space and Planetary ScienceMillisecond pulsarOrder of magnitude
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On the convexity of Relativistic Hydrodynamics

2013

The relativistic hydrodynamic system of equations for a perfect fluid obeying a causal equation of state is hyperbolic (Anile 1989 {\it Relativistic Fluids and Magneto-Fluids} (Cambridge: Cambridge University Press)). In this report, we derive the conditions for this system to be convex in terms of the fundamental derivative of the equation of state (Menikoff and Plohr 1989 {\it Rev. Mod. Phys.} {\bf 61} 75). The classical limit is recovered.

PhysicsPhysics and Astronomy (miscellaneous)Equation of state (cosmology)Regular polygonFOS: Physical sciencesPerfect fluidDerivativeGeneral Relativity and Quantum Cosmology (gr-qc)System of linear equationsGeneral Relativity and Quantum CosmologyRelativistic hydrodynamic systemConvexityClassical limitConvexityAstronomía y AstrofísicaMathematical physics
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L-Rigidity in Newtonian approximation

2008

Newtonian limit of L-Rigidity is obtained. In this formalism, L-Rigidity is reduced to steady Newtonian rigid motions in a Newtonian frame of reference in which the observer is at rest.

PhysicsPhysics::General PhysicsInertial frame of referenceNewtonian potentialNewtonian limitRotating reference frameFrame of referenceCovariant derivativePhysics::Fluid DynamicsGeneral Relativity and Quantum CosmologyClassical mechanicsPhysics::Space PhysicsNewtonian fluidVector field
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