Search results for "semiclassical"

showing 10 items of 111 documents

Static quantum corrections to the Schwarzschild spacetime

2005

We study static quantum corrections of the Schwarzschild metric in the Boulware vacuum state. Due to the absence of a complete analytic expression for the full semiclassical Einstein equations we approach the problem by considering the s-wave approximation and solve numerically the associated backreaction equations. The solution, including quantum effects due to pure vacuum polarization, is similar to the classical Schwarzschild solution up to the vicinity of the classical horizon. However, the radial function has a minimum at a time-like surface close to the location of the classical event horizon. There the g_{00} component of the metric reaches a very small but non-zero value. The analys…

PhysicsHigh Energy Physics - TheoryHistorySpacetimeEvent horizonVacuum stateSemiclassical physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyComputer Science ApplicationsEducationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Horizon (general relativity)Schwarzschild metricVacuum polarizationSchwarzschild radiusMathematical physics
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Quantum Gravity Effects in the Kerr Spacetime

2010

We analyze the impact of the leading quantum gravity effects on the properties of black holes with nonzero angular momentum by performing a suitable renormalization group improvement of the classical Kerr metric within Quantum Einstein Gravity (QEG). In particular we explore the structure of the horizons, the ergosphere, and the static limit surfaces as well as the phase space avilable for the Penrose process. The positivity properties of the effective vacuum energy momentum tensor are also discussed and the "dressing" of the black hole's mass and angular momentum are investigated by computing the corresponding Komar integrals. The pertinent Smarr formula turns out to retain its classical f…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsGeneral relativityAstrophysics::High Energy Astrophysical PhenomenaKerr metricFOS: Physical sciencesPenrose processBlack holeGeneral Relativity and Quantum CosmologyClassical mechanicsRotating black holeHigh Energy Physics - Theory (hep-th)Total angular momentum quantum numberSemiclassical gravityBlack hole thermodynamics
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Short-distance contribution to the spectrum of Hawking radiation

2006

The Hawking effect can be rederived in terms of two-point functions and in such a way that it makes it possible to estimate, within the conventional semiclassical theory, the contribution of ultrashort distances to the Planckian spectrum. For Schwarzschild black holes of three solar masses the analysis shows that Hawking radiation is very robust up to frequencies of 96 T_H or 270 T_H for bosons and fermions, respectively. For primordial black holes (with masses around 10^{15} g) these frequencies turn out to be of order 52T_H and 142 T_H. Only at these frequencies and above do we find that the contribution of Planck distances is of order of the total spectrum itself. Below this scale, the c…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsQuantum field theory in curved spacetime010308 nuclear & particles physicsSemiclassical physicsFOS: Physical sciencesFermion01 natural sciencesHigh Energy Physics::TheoryMicro black holeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum electrodynamicsQuantum mechanics0103 physical sciencesQuantum gravityFísica nuclear010306 general physicsSchwarzschild radiusHawking radiationBoson
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Conformal and non-conformal symmetries in 2D dilaton gravity

1996

We introduce new extra symmetry transformations for generic 2D dilaton-gravity models. These symmetries are non-conformal but special linear combinations of them turn out to be the extra (conformal) symmetries of the CGHS model and the model with an exponential potential. We show that one of the non-conformal extra symmetries can be converted into a conformal one by means of adequate field redefinitions involving the metric and the derivatives of the dilaton. Finally, by expressing the Polyakov-Liouville effective action in terms of an auxiliary invariant metric, we construct one-loop models which maintain the extra symmetry of the classical action. © 1997 Elsevier Science B.V.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsSigma modelCGHS modelSemiclassical physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Symmetry (physics)General Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)Solvable modelsHomogeneous spaceAstronomiaDilatonInvariant (mathematics)Simetria (Física)Effective actionNon-conformal symmetriesMathematical physics
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RG flows of Quantum Einstein Gravity in the linear-geometric approximation

2014

We construct a novel Wetterich-type functional renormalization group equation for gravity which encodes the gravitational degrees of freedom in terms of gauge-invariant fluctuation fields. Applying a linear-geometric approximation the structure of the new flow equation is considerably simpler than the standard Quantum Einstein Gravity construction since only transverse-traceless and trace part of the metric fluctuations propagate in loops. The geometric flow reproduces the phase-diagram of the Einstein-Hilbert truncation including the non-Gaussian fixed point essential for Asymptotic Safety. Extending the analysis to the polynomial $f(R)$-approximation establishes that this fixed point come…

PhysicsHigh Energy Physics - Theory; High Energy Physics - Theory; General Relativity and Quantum CosmologyHigh Energy Physics - TheoryEntropic gravityGeneral relativityAsymptotic safety in quantum gravityGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Euclidean quantum gravityGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Linearized gravityTheoretical High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGQuantum gravitySemiclassical gravityf(R) gravityAnnals of Physics
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Photodetachment o F- by a few-cycle circularly polarized laser field

2009

We report on calculations of the above threshold detachment of F(-) by a few-cycle circularly polarized laser field, discussing the effects of both the carrier-envelope relative phase and the number of the cycle contained in a pulse on the angular distribution of ejected photoelectron. The results are analyzed in terms of a two-step semiclassical model: after the electrons are detached through tunnelling their motion is determined by the electric field pulse according to the classical dynamics laws. Anisotropies in the angular distributions of the electrons ejected on the plane perpendicular to the laser propagation direction are found that depend on the number of cycle of the laser pulse.

PhysicsIonizationField (physics)business.industrySemiclassical physicsElectronLaserAtomic and Molecular Physics and OpticsSettore FIS/03 - Fisica Della Materialaw.inventionPulse (physics)Opticslawnonsequential doubleElectric fieldPerpendicularAtomic physicsbusinessQuantum tunnellinglasers
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Calculated Line Broadening Coefficients in the nu2 Band of CH3D Perturbed by Helium

2003

International audience; Line broadening coefficients have been calculated, at room temperature, for lines in the P and R branches of the nu2 band of monodeuterated methane. A properly symmetrized semiclassical model with parabolic relative trajectories has been used. Two interaction potential models have been considered. The first is a Lennard-Jones type atom-atom potential, while the second one was derived from ab initio calculations. The calculated line widths were compared to the available experimental data and a satisfactory agreement was found, although the model contains no other adjustable parameters than the four atomic Lennard-Jones ones. Nonetheless, failures of calculations have …

PhysicsLine broadening coefficients010304 chemical physicsCondensed matter physics[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Semiclassical physicschemistry.chemical_elementQuantum numberSemiclassical calculations01 natural sciences7. Clean energyAtomic and Molecular Physics and OpticsCH3DInteraction potentialchemistry[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]Ab initio quantum chemistry methods0103 physical sciencesPhysics::Atomic and Molecular ClustersPhysical and Theoretical ChemistryAtomic physics010303 astronomy & astrophysicsSpectroscopyHeliumLine (formation)
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Shears Mechanism in theA∼110Region

1999

Lifetimes of states in a rotational-like $M1$ band in ${}^{110}\mathrm{Cd}$ have been determined through a Doppler-shift attenuation method measurement performed with the Gammasphere array. The deduced $B(M1)$ values, which agree well with the predictions of the tilted axis cranking model, clearly confirm that it has the character of a shears band. Using a semiclassical scheme of the coupling of two long $j$ vectors we deduce information on the strength and form of the effective interaction between the constituent nucleons. These results are the first definitive evidence of the shears mechanism and ``magnetic rotation'' in this mass region.

PhysicsMagnetic momentAttenuationNuclear structureGeneral Physics and AstronomySemiclassical physicsGammasphereAtomic physicsRotationCoupling (probability)NucleonPhysical Review Letters
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Lifetime measurements in 166Re : Collective versus magnetic rotation

2016

WOS: 000371740600004

PhysicsManchester Cancer Research Centreta114010308 nuclear & particles physicsResearchInstitutes_Networks_Beacons/mcrcMagnetic rotationRouthianNuclear TheoryOrder (ring theory)Semiclassical physicsState (functional analysis)rhenium01 natural sciencesNuclear shapeRecoilExcited state0103 physical scienceslifetimesAtomic physics010306 general physicsexcited statesPhysical Review C
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Semiquantum molecular dynamics simulation of thermal properties and heat transport in low-dimensional nanostructures

2012

We present a detailed description of the semi-quantum approach to the molecular dynamics simulation of stochastic dynamics of a system of interacting particles. Within this approach, the dynamics of the system is described with the use of classical Newtonian equations of motion in which the quantum effects are introduced through random Langevin-like forces with a specific power spectral density (the color noise). The color noise describes the interaction of the molecular system with the thermostat. We apply this technique to the simulation of the thermal properties of different low-dimensional nanostructures. Within this approach, we simulate the specific heat and heat transport in carbon n…

PhysicsMolecular dynamicsClassical mechanicsThermal conductivityQuantum dynamicsAnharmonicityEquations of motionSemiclassical physicsInteratomic potentialCondensed Matter PhysicsQuantum statistical mechanicsElectronic Optical and Magnetic MaterialsPhysical Review B
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