Search results for "semiclassical"

showing 10 items of 111 documents

Low-energy corrections to the eikonal description of elastic scattering and breakup of one-neutron halo nuclei in nuclear-dominated reactions

2018

Background: The eikonal approximation is a high-energy reaction model, which is very computationally efficient and provides a simple interpretation of the collision. Unfortunately, it is not valid at energies around 10 MeV/nucleon, the range of energy of HIE-ISOLDE at CERN and the future ReA12 at MSU. Fukui et al. [Phys. Rev. C 90, 034617 (2014)10.1103/PhysRevC.90.034617] have shown that a simple semiclassical correction of the projectile-target deflection could improve the description of breakup of halo nuclei on heavy targets down to 20 MeV/nucleon. Purpose: We study two similar corrections, which aim at improving the projectile-target relative motion within the eikonal approximation, wit…

PhysicsElastic scatteringNuclear Theory010308 nuclear & particles physicsEikonal equationNuclear TheoryFOS: Physical sciencesSemiclassical physics01 natural sciencesPhysique atomique et nucléaireEikonal approximationNuclear Theory (nucl-th)Nuclear physics0103 physical sciencesNeutronHaloImpact parameterNuclear Experiment010306 general physicsNucleonPhysical Review C
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High Order Harmonics from a Molecule: Evidence of the Nuclear Motion

2007

The electromagnetic spectrum emitted by a molecule driven by a laser presents harmonics and satellite lines whose separation is equal to the oscillation frequency of the nuclei. Full quantum and semiclassical calculations are presented.

PhysicsElectromagnetic spectrumlawOscillationHarmonicsSemiclassical physicsAtomic physicsSpectroscopyLaserElectromagnetic radiationQuantumlaw.invention
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Analysis of the viscous quantum hydrodynamic equations for semiconductors

2004

The steady-state viscous quantum hydrodynamic model in one space dimension is studied. The model consists of the continuity equations for the particle and current densities, coupled to the Poisson equation for the electrostatic potential. The equations are derived from a Wigner–Fokker–Planck model and they contain a third-order quantum correction term and second-order viscous terms. The existence of classical solutions is proved for “weakly supersonic” quantum flows. This means that a smallness condition on the particle velocity is still needed but the bound is allowed to be larger than for classical subsonic flows. Furthermore, the uniqueness of solutions and various asymptotic limits (sem…

PhysicsElliptic curveClassical mechanicsInviscid flowQuantum hydrodynamicsApplied MathematicsSemiclassical physicsUniquenessPoisson's equationQuantumExponential functionEuropean Journal of Applied Mathematics
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Pair production due to an electric field in 1+1 dimensions and the validity of the semiclassical approximation

2021

Solutions to the backreaction equation in $1+1$-dimensional semiclassical electrodynamics are obtained and analyzed when considering a time-varying homogeneous electric field initially generated by a classical electric current, coupled to either a quantized scalar field or a quantized spin-$\frac{1}{2}$ field. Particle production by way of the Schwinger effect leads to backreaction effects that modulate the electric field strength. Details of the particle production process are investigated along with the transfer of energy between the electric field and the particles. The validity of the semiclassical approximation is also investigated using a criterion previously implemented for chaotic i…

PhysicsField (physics)010308 nuclear & particles physicsOrder (ring theory)Semiclassical physics01 natural sciencesElectric chargePair production0103 physical sciencesProduction (computer science)Semiclassical gravity010306 general physicsScalar fieldMathematical physicsPhysical Review D
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Is There a C-Function in 4D Quantum Einstein Gravity?

2016

We describe a functional renormalization group-based method to search for ‘C-like’ functions with properties similar to that in 2D conformal field theory. It exploits the mode counting properties of the effective average action and is particularly suited for theories including quantized gravity. The viability of the approach is demonstrated explicitly in a truncation of 4 dimensional Quantum Einstein Gravity, i.e. asymptotically safe metric gravity.

PhysicsGeneral Relativity and Quantum CosmologyClassical mechanicsEntropic gravityHořava–Lifshitz gravityAsymptotic safety in quantum gravityQuantum gravitySpin foamf(R) gravitySemiclassical gravityEuclidean quantum gravityMathematical physics
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The Quantum Scalar Field in Spherically Symmetric Loop Quantum Gravity

2013

We consider the quantization of a spherically symmetric gravitational system coupled to a massless scalar field within the loop quantum gravity framework. Our results rely on the uniform discretizations method developed during the last years. We minimize the associated discrete “master constraint” using a trial state whose gravitational part is peaked around the classical Schwarzschild solution.

PhysicsGeneral Relativity and Quantum CosmologyQuantization (physics)Quantum geometryClassical mechanicsSpin foamQuantum gravitySemiclassical gravityLoop quantum gravityScalar fieldLoop quantum cosmology
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Return to Equilibrium, Non-self-adjointness and Symmetries, Recent Results with M. Hitrik and F. Hérau

2014

In this talk we review some old and new results about the use of supersymmetric structures in semi-classical problems. Necessary and sufficient conditions are obtained for a real semiclassical partial differential operator of order two to possess a supersymmetric structure. For operators coming from a chain of oscillators, coupled to two heat baths, we show the non-existence of a smooth supersymmetric structure. The recent and new results all come from joint works with Michael Hitrik and Frederic Herau.

PhysicsHeat bathHomogeneous spaceStructure (category theory)Semiclassical physicsOrder (group theory)Partial differential operatorMorse theoryMathematical physics
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Adiabatic regularization with a Yukawa interaction

2017

We extend the adiabatic regularization method for an expanding universe to include the Yukawa interaction between quantized Dirac fermions and a homogeneous background scalar field. We give explicit expressions for the renormalized expectation values of the stress-energy tensor $\langle T_{\mu\nu} \rangle$ and the bilinear $\langle \bar\psi\psi\rangle$ in a spatially flat FLRW spacetime. These are basic ingredients in the semiclassical field equations of fermionic matter in curved spacetime interacting with a background scalar field. The ultraviolet subtracting terms of the adiabatic regularization can be naturally interpreted as coming from appropriate counterterms of the background fields…

PhysicsHigh Energy Physics - Theory010308 nuclear & particles physicsConformal anomalyHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologySemiclassical physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Yukawa interaction01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum mechanicsRegularization (physics)Friedmann–Lemaître–Robertson–Walker metric0103 physical sciencessymbols010306 general physicsAdiabatic processScalar fieldEffective actionMathematical physics
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Role of gravity in the pair creation induced by electric fields

2018

We analyze the pair production induced by homogenous, time-dependent electric fields in an expanding space-time background. We point out that, in obtaining the semiclassical Maxwell equations, two distinct notions of adiabatic renormalization are possible. In Minkowski space the two recipes turn out to be equivalent. However, in the presence of gravity only the recipe requiring an adiabatic hierarchy between the gravitational and the gauge field is consistent with the conservation of the energy-momentum tensor.

PhysicsHigh Energy Physics - Theory010308 nuclear & particles physicsSemiclassical physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyRenormalizationGravitationsymbols.namesakeClassical mechanicsMaxwell's equationsHigh Energy Physics - Theory (hep-th)0103 physical sciencesMinkowski spacesymbolsTensorGauge theory010306 general physicsAdiabatic process
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Solvable Models for radiating Black Holes and Area-preserving Diffeomorphisms

1995

Solvable theories of 2D dilaton gravity can be obtained from a Liouville theory by suitable field redefinitions. In this paper we propose a new framework to generate 2D dilaton gravity models which can also be exactly solved in the semiclassical approximation. Our approach is based on the recently introduced scheme to quantize massless scalar fields coupled to 2D gravity maintaining invariance under area-preserving diffeomorphisms and Weyl transformations. Starting from the CGHS model with the new effective action we reestablish the full diffeomorphism invariance by means of an adequate family of field redefinitions. The original theory is therefore mapped into a large family of solvable mo…

PhysicsHigh Energy Physics - TheoryAstrofísicaNuclear and High Energy PhysicsGravitacióField (physics)CGHS modelScalar (physics)Semiclassical physicsFOS: Physical sciencessymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)symbolsDilatonDiffeomorphismEinsteinEffective actionMathematical physics
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