Search results for "Mathematical physics"

showing 10 items of 2687 documents

Cosmological Horizon Modes and Linear Response in de Sitter Spacetime

2009

Linearized fluctuations of quantized matter fields and the spacetime geometry around de Sitter space are considered in the case that the matter fields are conformally invariant. Taking the unperturbed state of the matter to be the de Sitter invariant Bunch-Davies state, the linear variation of the stress tensor about its self-consistent mean value serves as a source for fluctuations in the geometry through the semiclassical Einstein equations. This linear response framework is used to investigate both the importance of quantum backreaction and the validity of the semiclassical approximation in cosmology. The full variation of the stress tensor delta bi contains two kinds of terms: (1) those…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsQuantum field theory in curved spacetimeCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsCauchy stress tensorDe Sitter spaceSemiclassical physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyAuxiliary fieldGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)De Sitter universeQuantum cosmologyQuantum mechanics0103 physical sciencesEinstein field equations010306 general physicsAstrophysics - Cosmology and Nongalactic AstrophysicsMathematical physics
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Electric-magnetic duality and renormalization in curved spacetimes

2014

We point out that the duality symmetry of free electromagnetism does not hold in the quantum theory if an arbitrary classical gravitational background is present. The symmetry breaks in the process of renormalization, as also happens with conformal invariance. We show that a similar duality-anomaly appears for a massless scalar field in $1+1$ dimensions.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsQuantum field theory in curved spacetimeScalar field theoryConformal field theoryFísicaFOS: Physical sciencesDuality (optimization)General Relativity and Quantum Cosmology (gr-qc)Scale invariance16. Peace & justiceGeneral Relativity and Quantum CosmologyRenormalizationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Conformal symmetryQuantum mechanicsScalar fieldMathematical physicsPhysical Review D
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Noncommutative space and the low-energy physics of quasicrystals

2008

We prove that the effective low-energy, nonlinear Schroedinger equation for a particle in the presence of a quasiperiodic potential is the potential-free, nonlinear Schroedinger equation on noncommutative space. Thus quasiperiodicity of the potential can be traded for space noncommutativity when describing the envelope wave of the initial quasiperiodic wave.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsQuasicrystalFOS: Physical sciencesAstronomy and AstrophysicsMathematical Physics (math-ph)Space (mathematics)Noncommutative geometryAtomic and Molecular Physics and OpticsNonlinear Sciences::Chaotic DynamicsQuasiperiodicitysymbols.namesakeLow energyHigh Energy Physics - Theory (hep-th)Quasiperiodic functionsymbolsNonlinear Schrödinger equationMathematical PhysicsMathematical physicsEnvelope (waves)
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THE PARISI–SOURLAS MECHANISM IN YANG–MILLS THEORY?

1999

The Parisi-Sourlas mechanism is exhibited in pure Yang-Mills theory. Using the new scalar degrees of freedom derived from the non-linear gauge condition, we show that the non-perturbative sector of Yang-Mills theory is equivalent to a 4D O(1,3) sigma model in a random field. We then show that the leading term of this equivalent theory is invariant under supersymmetry transformations where (x^{2}+\thetabar\theta) is unchanged. This leads to dimensional reduction proving the equivalence of the non-perturbative sector of Yang-Mills theory to a 2D O(1,3) sigma model.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsRandom fieldSigma modelHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstronomy and AstrophysicsSupersymmetryYang–Mills theoryInvariant (physics)Atomic and Molecular Physics and OpticsHigh Energy Physics::TheoryNonlinear systemHigh Energy Physics - Theory (hep-th)Dimensional reductionEquivalence (measure theory)Mathematical physicsInternational Journal of Modern Physics A
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A comparison of efficient methods for the computation of Born gluon amplitudes

2006

We compare four different methods for the numerical computation of the pure gluonic amplitudes in the Born approximation. We are in particular interested in the efficiency of the various methods as the number n of the external particles increases. In addition we investigate the numerical accuracy in critical phase space regions. The methods considered are based on (i) Berends-Giele recurrence relations, (ii) scalar diagrams, (iii) MHV vertices and (iv) BCF recursion relations.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsRecurrence relationComputationScalar (mathematics)FOS: Physical sciencesRecursion (computer science)Space (mathematics)GluonHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)AmplitudeHigh Energy Physics - Theory (hep-th)Born approximationMathematical physicsJournal of High Energy Physics
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Proper Time Flow Equation for Gravity

2004

We analyze a proper time renormalization group equation for Quantum Einstein Gravity in the Einstein-Hilbert truncation and compare its predictions to those of the conceptually different exact renormalization group equation of the effective average action. We employ a smooth infrared regulator of a special type which is known to give rise to extremely precise critical exponents in scalar theories. We find perfect consistency between the proper time and the average action renormalization group equations. In particular the proper time equation, too, predicts the existence of a non-Gaussian fixed point as it is necessary for the conjectured nonperturbative renormalizability of Quantum Einstein…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsScalar (physics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Fixed pointRenormalization groupGeneral Relativity and Quantum CosmologyAction (physics)High Energy Physics - PhenomenologyGeneral Relativity and Quantum Cosmologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Flow (mathematics)symbolsProper timeEinsteinCritical exponentMathematical physicsJournal of High Energy Physics
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Free field realization of cylindrically symmetric Einstein gravity

1998

Cylindrically reduced Einstein gravity can be regarded as an $SL(2,R)/SO(2)$ sigma model coupled to 2D dilaton gravity. By using the corresponding 2D diffeomorphism algebra of constraints and the asymptotic behaviour of the Ernst equation we show that the theory can be mapped by a canonical transformation into a set of free fields with a Minkowskian target space. We briefly discuss the quantization in terms of these free-field variables, which is considerably simpler than in the other approaches.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsSigma modelFOS: Physical sciencesCanonical transformationGeneral Relativity and Quantum Cosmology (gr-qc)Free fieldGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmologysymbols.namesakeQuantization (physics)High Energy Physics - Theory (hep-th)symbolsFísica nuclearDilatonNernst equationDiffeomorphismEinsteinMathematical physicsPhysics Letters B
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A comment on the relationship between differential and dimensional renormalization

1992

We show that there is a very simple relationship between differential and dimensional renormalization of low-order Feynman graphs in renormalizable massless quantum field theories. The beauty of the differential approach is that it achieves the same finite results as dimensional renormalization without the need to modify the space time dimension.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsSpace timeHigh Energy Physics::LatticeFOS: Physical sciencesFísicaRenormalizationMassless particlesymbols.namesakeHigh Energy Physics - Theory (hep-th)Dimension (vector space)Simple (abstract algebra)symbolsFeynman diagramQuantum field theoryDifferential (mathematics)Mathematical physics
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Twistor transform inddimensions and a unifying role for twistors

2005

Twistors in four dimensions d=4 have provided a convenient description of massless particles with any spin, and this led to remarkable computational techniques in Yang-Mills field theory. Recently it was shown that the same d=4 twistor provides also a unified description of an assortment of other particle dynamical systems, including special examples of massless or massive particles, relativistic or non-relativistic, interacting or non-interacting, in flat space or curved spaces. In this paper, using 2T-physics as the primary theory, we derive the general twistor transform in d-dimensions that applies to all cases, and show that these more general twistor transforms provide d dimensional ho…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsSpacetimeFOS: Physical sciencesYang–Mills theorySpace (mathematics)ModuliTwistor theoryHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)Phase spaceMinkowski spaceTwistor spaceMathematics::Differential GeometryMathematical physicsPhysical Review D
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Renormalization group improved gravitational actions: A Brans-Dicke approach

2003

A new framework for exploiting information about the renormalization group (RG) behavior of gravity in a dynamical context is discussed. The Einstein-Hilbert action is RG-improved by replacing Newton's constant and the cosmological constant by scalar functions in the corresponding Lagrangian density. The position dependence of $G$ and $\Lambda$ is governed by a RG equation together with an appropriate identification of RG scales with points in spacetime. The dynamics of the fields $G$ and $\Lambda$ does not admit a Lagrangian description in general. Within the Lagrangian formalism for the gravitational field they have the status of externally prescribed ``background'' fields. The metric sat…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsSpacetimeScalar (mathematics)FOS: Physical sciencesEnergy–momentum relationGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantRenormalization groupGeneral Relativity and Quantum CosmologyGravitationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Gravitational fieldQuantum mechanicsQuantum gravityMathematical physicsPhysical Review D
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