Search results for " solution"

showing 10 items of 3084 documents

The influence of the solvent's mass on the location of the dividing surface for a model Hamiltonian

2019

The Transition State dividing surface is a key concept, not only for the precise calculation of the rate constant of a reaction, but also for the proper prediction of product ratios. The correct location of this surface is defined by the requirement that reactive trajectories do not recross it. In the case of reactions in solution the solvent plays an important role in the location of the dividing surface. In this paper we show with the aid of a model Hamiltonian that the effective mass of the solvent can dramatically change the location of the dividing surface. Keywords: Dynamical systems, Dividing surface, Reactions in solution, 2019 MSC: 00-01, 99-00

PhysicsDynamical systems theoryMathematical analysisSolvationlcsh:QD450-801General Physics and Astronomylcsh:Physical and theoretical chemistryDividing surfaceSurface reactionSistemes dinàmics diferenciablesChemical reactionlcsh:QC1-999Reactions in solutionSolventsymbols.namesakeReaction rate constantEffective mass (solid-state physics)Dynamical systemssymbolsPhysical and Theoretical ChemistryHamiltonian (quantum mechanics)lcsh:PhysicsFisicoquímica
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Strong etching formulation (time and rate) for PADC with deep depth bulk etch rate study

2021

Abstract Aqueous NaOH with ethanol (strong) etchant is widely used. It shortens etching time effectively compared to normal etching conditions (6.25N NaOH at 70 °C). Two equations have been proposed to calculate the etching time with NaOH molarity and ethanol volume. Another two empirical equations were introduced for estimating the bulk etch rates of PADC etched in strong etchant. Up to now, there were no such equations available in the literature that can predict etching time and V b of PADC with etchant molarity and ethanol volumes. The proposed equations were compared to fundamental V b models stemming from literature. Fast etching enables the follow-up of bulk etch rate variation versu…

PhysicsEmpirical equationsNuclear and High Energy PhysicsAqueous solutionMolar concentration010308 nuclear & particles physicsAnalytical chemistry01 natural sciences030218 nuclear medicine & medical imaging03 medical and health sciences0302 clinical medicineVolume (thermodynamics)Etching (microfabrication)0103 physical sciencesInstrumentationLayer (electronics)Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Beyond the Vegard's law: solid mixing excess volume and thermodynamic potentials prediction, from end-members

2020

Abstract A method has been developed, herein presented, to model binary solid solutions' volume, enthalpy and Gibbs energy using the energy state functions, E ( V , S ) , of the end-members only. The E ( V , S ) s are expanded around an unknown mixing volume, V Mix , and the fundamental equilibrium equation − ( ∂ E / ∂ V ) S = P is used to determine V Mix . V Mix allows us to model enthalpy, straightforwardly. The same argument holds using Helmholtz energy, F ( V , T ) , in place of E ( V , S ) , and the equilibrium equation becomes − ( ∂ F / ∂ V ) T = P . One can readily determine the Gibbs free energy, too. The method presented remarkably simplifies computing of solid mixings' thermodynam…

PhysicsEnthalpyGeneral Physics and AstronomyThermodynamicsComputer simulation01 natural sciences010305 fluids & plasmasThermodynamic potentialGibbs free energysymbols.namesakeVolume (thermodynamics)Vegard's lawNitride materialHelmholtz free energy0103 physical sciencessymbols010306 general physicsMetals and alloyThermodynamic modelingMixing (physics)Solid solution
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Dynamical behaviour of an XX central spin model through Bethe ansatz techniques

2009

Following the Bethe ansazt procedure the exact dynamics of an XX central spin model is revealed. Particular initial conditions are analyzed and the consequent time evolution is compared with the exact solution obtained by solving the time-dependent Schrudinger equation. The interest towards spin systems and in particular central spin systems, is motivated by the recent developments in more applicative contexts.

PhysicsExact solutions in general relativityQuantum mechanicsSpin modelTime evolutionCondensed Matter::Strongly Correlated ElectronsStatistical and Nonlinear PhysicsMathematical PhysicsBethe ansatzMathematical physicsSpin-½Reports on Mathematical Physics
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Pair and triple correlations in theA+B→Bdiffusion-controlled reaction

1994

An exact solution for the one-dimensional kinetics of the diffusion-controlled reaction A+B\ensuremath{\rightarrow}B is obtained by means of the three-particle correlation functions. Because of a lattice discreteness each site could be occupied by a single particle only which leads to the so-called ``bus effect'': Recombination of any particle A is defined by a spatial configuration of two nearest particles B only surrounding A from its left and right. This results in the unusual algebraic decay law, n(t)\ensuremath{\propto}${\mathit{t}}^{\mathrm{\ensuremath{-}}1}$, which asymptotically (as t\ensuremath{\rightarrow}\ensuremath{\infty}) does not depend on the trap B concentration.

PhysicsExact solutions in general relativitySpatial configurationLattice (order)Diffusion-controlled reactionGeneral Physics and AstronomyAlgebraic numberAtomic physicsPhysical Review Letters
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One pendulum to run them all

2013

The analytical solution for the three-dimensional linear pendulum in a rotating frame of reference is obtained, including Coriolis and centrifugal accelerations, and expressed in terms of initial conditions. This result offers the possibility of treating Foucault and Bravais pendula as trajectories of the same system of equations, each of them with particular initial conditions. We compare them with the common two-dimensional approximations in textbooks. A previously unnoticed pattern in the three-dimensional Foucault pendulum attractor is presented.

PhysicsFoucault pendulumPendulumGeneral Physics and AstronomyClassical Physics (physics.class-ph)FOS: Physical sciencesPhysics - Classical PhysicsPopular Physics (physics.pop-ph)Physics - Popular PhysicsSystem of linear equationsRotating reference framePartícules (Física nuclear)Analytical Solutionlaw.inventionPhysics::Popular PhysicsClassical mechanicslawCentrifugal accelerationsAttractor
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An intrinsic characterization of the Schwarzschild metric

1998

An intrinsic algorithm that exclusively involves conditions on the metric tensor and its differential concomitants is presented to identify every type-D static vacuum solution. In particular, the necessary and sufficient explicit and intrinsic conditions are given for a Lorentzian metric to be the Schwarzschild solution.

PhysicsGeneral Relativity and Quantum CosmologyPhysics and Astronomy (miscellaneous)Schwarzschild coordinatesMetric signatureSchwarzschild geodesicsKerr metricSchwarzschild metricDeriving the Schwarzschild solutionMetric tensor (general relativity)Mathematical physicsIntrinsic metricClassical and Quantum Gravity
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Cosmological solutions in theD=5 Einstein-Maxwell theory coupled to matter

1991

We study the Einstein-Maxwell theory in five dimensions coupled to matter in two distinct ways. In the first we reduce the Lagrangian to an effective four-dimension one and then we couple it to matter; in the second, we introduce matter directly in the original five-dimensional theory. In both cases we use a non trivial configuration for the Maxwell potential. We find non singular solutions which present a repulsive gravitational phase. When this phase is absent, the initial singularity is unavoidable.

PhysicsGravitationsymbols.namesakeSingularityPhysics and Astronomy (miscellaneous)Initial singularitySingular solutionGeneral relativitySpace timesymbolsEinsteinCosmologyMathematical physicsGeneral Relativity and Gravitation
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Wormholes supported by hybrid metric-Palatini gravity

2012

Recently, a modified theory of gravity was presented, which consists of the superposition of the metric Einstein-Hilbert Lagrangian with an $f(\cal R)$ term constructed \`{a} la Palatini. The theory possesses extremely interesting features such as predicting the existence of a long-range scalar field, that explains the late-time cosmic acceleration and passes the local tests, even in the presence of a light scalar field. In this brief report, we consider the possibility that wormholes are supported by this hybrid metric-Palatini gravitational theory. We present here the general conditions for wormhole solutions according to the null energy conditions at the throat and find specific examples…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)High Energy Physics - TheoryNuclear and High Energy Physics010308 nuclear & particles physicsScalar theories of gravitationFOS: Physical sciencesVacuum solutionGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationsymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)0103 physical sciencessymbolsf(R) gravityWormhole010306 general physicsAstrophysics - High Energy Astrophysical PhenomenaKlein–Gordon equationScalar fieldAsymptotically flat spacetimeMathematical physics
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Rotating black holes in Eddington-inspired Born-Infeld gravity: an exact solution

2020

We find an exact, rotating charged black hole solution within Eddington-inspired Born-Infeld gravity. To this end we employ a recently developed correspondence or {\it mapping} between modified gravity models built as scalars out of contractions of the metric with the Ricci tensor, and formulated in metric-affine spaces (Ricci-Based Gravity theories) and General Relativity. This way, starting from the Kerr-Newman solution, we show that this mapping bring us the axisymmetric solutions of Eddington-inspired Born-Infeld gravity coupled to a certain model of non-linear electrodynamics. We discuss the most relevant physical features of the solutions obtained this way, both in the spherically sym…

PhysicsHigh Energy Physics - TheoryGravity (chemistry)Modified gravityFísica-Modelos matemáticos010308 nuclear & particles physicsGeneral relativityRotational symmetryFOS: Physical sciencesAstronomy and AstrophysicsGR black holesGeneral Relativity and Quantum Cosmology (gr-qc)Charged black hole01 natural sciencesGravitational-wave astronomyGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum CosmologyExact solutions in general relativityHigh Energy Physics - Theory (hep-th)0103 physical sciencesMetric (mathematics)Física matemáticaWormholesRicci curvature
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