Search results for "Mathematical physics"

showing 10 items of 2687 documents

Frame covariant nonminimal multifield inflation

2017

We introduce a frame-covariant formalism for inflation of scalar-curvature theories by adopting a differential geometric approach which treats the scalar fields as coordinates living on a field-space manifold. This ensures that our description of inflation is both conformally and reparameterization covariant. Our formulation gives rise to extensions of the usual Hubble and potential slow-roll parameters to generalized fully frame-covariant forms, which allow us to provide manifestly frame-invariant predictions for cosmological observables, such as the tensor-to-scalar ratio $r$, the spectral indices $n_{\cal R}$ and $n_T$, their runnings $\alpha_{\cal R}$ and $\alpha_T$, the non-Gaussianity…

High Energy Physics - TheoryPhysicsNuclear and High Energy Physics010308 nuclear & particles physicsScalar (mathematics)FOS: Physical sciencesObservableGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsParameter spaceCurvature01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)0103 physical sciencesHiggs bosonlcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityCovariant transformationBoundary value problem010306 general physicsEffective actionMathematical physicsNuclear Physics B
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Explicit results for all orders of the epsilon-expansion of certain massive and massless diagrams

2000

An arbitrary term of the epsilon-expansion of dimensionally regulated off-shell massless one-loop three-point Feynman diagram is expressed in terms of log-sine integrals related to the polylogarithms. Using magic connection between these diagrams and two-loop massive vacuum diagrams, the epsilon-expansion of the latter is also obtained, for arbitrary values of the masses. The problem of analytic continuation is also discussed.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsAnalytic continuationFOS: Physical sciencesMassless particleHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Quantum electrodynamicssymbolsFeynman diagramMathematical physics
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Superconformal mechanics, black holes, and non-linear realizations

1998

The OSp(2|2)-invariant planar dynamics of a D=4 superparticle near the horizon of a large mass extreme black hole is described by an N=2 superconformal mechanics, with the SO(2) charge being the superparticle's angular momentum. The {\it non-manifest} superconformal invariance of the superpotential term is shown to lead to a shift in the SO(2) charge by the value of its coefficient, which we identify as the orbital angular momentum. The full SU(1,1|2)-invariant dynamics is found from an extension to N=4 superconformal mechanics.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsAngular momentumSuperpotentialFOS: Physical sciencesMechanicsGeneral Relativity and Quantum Cosmology (gr-qc)Mathematical Physics (math-ph)General Relativity and Quantum CosmologyBlack holeHigh Energy Physics::TheoryRotating black holeHigh Energy Physics - Theory (hep-th)Total angular momentum quantum numberExtremal black holeAngular momentum couplingAngular momentum operatorMathematical Physics
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Conformal sector of quantum Einstein gravity in the local potential approximation: Non-Gaussian fixed point and a phase of unbroken diffeomorphism in…

2008

We explore the nonperturbative renormalization group flow of quantum Einstein gravity (QEG) on an infinite dimensional theory space. We consider ``conformally reduced'' gravity where only fluctuations of the conformal factor are quantized and employ the local potential approximation for its effective average action. The requirement of ``background independence'' in quantum gravity entails a partial differential equation governing the scale dependence of the potential for the conformal factor which differs significantly from that of a scalar matter field. In the infinite dimensional space of potential functions we find a Gaussian as well as a non-Gaussian fixed point which provides further e…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsAsymptotic safety in quantum gravityFOS: Physical sciencesGaussian fixed pointGeneral Relativity and Quantum Cosmology (gr-qc)Expectation valueRenormalization groupFixed pointGeneral Relativity and Quantum CosmologyRenormalizationClassical mechanicsHigh Energy Physics - Theory (hep-th)Quantum gravityUltraviolet fixed pointMathematical physicsPhysical Review D
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Quantum stress tensor for extreme 2D Reissner-Nordström black holes

2004

Contrary to previous claims, it is shown that the expectation values of the quantum stress tensor for a massless scalar field propagating on a two-dimensional extreme Reissner-Nordstrom black hole are indeed regular on the horizon.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsBLACK HOLEWhite holeFOS: Physical sciencesREISSNER-NORDSTROEMGeneral Relativity and Quantum Cosmology (gr-qc)FuzzballGeneral Relativity and Quantum CosmologyBlack holeHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyMicro black hole2D ENERGY-MOMENTUM TENSORHigh Energy Physics - Theory (hep-th)HORIZONQuantum mechanicsExtremal black holeFísica nuclearVirtual black holeBlack hole thermodynamicsMathematical physicsHawking radiationPhysical Review D
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Pinch technique and the Batalin-Vilkovisky formalism

2002

In this paper we take the first step towards a non-diagrammatic formulation of the Pinch Technique. In particular we proceed into a systematic identification of the parts of the one-loop and two-loop Feynman diagrams that are exchanged during the pinching process in terms of unphysical ghost Green's functions; the latter appear in the standard Slavnov-Taylor identity satisfied by the tree-level and one-loop three-gluon vertex. This identification allows for the consistent generalization of the intrinsic pinch technique to two loops, through the collective treatment of entire sets of diagrams, instead of the laborious algebraic manipulation of individual graphs, and sets up the stage for the…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsBatalin–Vilkovisky formalismBackground field methodFOS: Physical sciencesFísicaYang–Mills theoryHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)PinchsymbolsFeynman diagramQuantum field theoryQuantumS-matrixMathematical physics
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Transcendental numbers and the topology of three-loop bubbles

1999

We present a proof that all transcendental numbers that are needed for the calculation of the master integrals for three-loop vacuum Feynman diagrams can be obtained by calculating diagrams with an even simpler topology, the topology of spectacles.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsComputationBare massFOS: Physical sciencesMathematical Physics (math-ph)TopologyHigh Energy Physics - PhenomenologyDimensional regularizationsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Number theoryHigh Energy Physics - Theory (hep-th)Special functionsRegularization (physics)symbolsFeynman diagramAlgebraic numberMathematical PhysicsPhysical Review D
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Domain wall junctions in a generalized Wess-Zumino model

1999

We investigate domain wall junctions in a generalized Wess-Zumino model with a Z(N) symmetry. We present a method to identify the junctions which are potentially BPS saturated. We then use a numerical simulation to show that those junctions indeed saturate the BPS bound for N=4. In addition, we study the decay of unstable non-BPS junctions.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsComputer simulationFOS: Physical sciencesCondensed Matter::Mesoscopic Systems and Quantum Hall EffectSymmetry (physics)Wess–Zumino modelHigh Energy Physics::TheoryDomain wall (string theory)High Energy Physics - Theory (hep-th)Physics::Plasma PhysicsCondensed Matter::SuperconductivityAstrophysics::Solar and Stellar AstrophysicsMathematical physicsPhysics Letters B
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Adiabatic regularization and particle creation for spin one-half fields

2013

The extension of the adiabatic regularization method to spin-$1/2$ fields requires a self-consistent adiabatic expansion of the field modes. We provide here the details of such expansion, which differs from the WKB ansatz that works well for scalars, to firmly establish the generalization of the adiabatic renormalization scheme to spin-$1/2$ fields. We focus on the computation of particle production in de Sitter spacetime and obtain an analytic expression of the renormalized stress-energy tensor for Dirac fermions.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Quantum field theory in curved spacetimeFOS: Physical sciencesFísicaGeneral Relativity and Quantum Cosmology (gr-qc)Mathematical Physics (math-ph)Adiabatic quantum computationGeneral Relativity and Quantum CosmologyWKB approximationRenormalizationsymbols.namesakeGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Dirac fermionRegularization (physics)symbolsAdiabatic processMathematical PhysicsAstrophysics - Cosmology and Nongalactic AstrophysicsMathematical physicsAnsatz
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Cosmology with self-adjusting vacuum energy density from a renormalization group fixed point

2001

Cosmologies with a time dependent Newton constant and cosmological constant are investigated. The scale dependence of $G$ and $\Lambda$ is governed by a set of renormalization group equations which is coupled to Einstein's equation in a consistent way. The existence of an infrared attractive renormalization group fixed point is postulated, and the cosmological implications of this assumption are explored. It turns out that in the late Universe the vacuum energy density is automatically adjusted so as to equal precisely the matter energy density, and that the deceleration parameter approaches $q = -1/4$. This scenario might explain the data from recent observations of high redshift type Ia S…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsDeceleration parametermedia_common.quotation_subjectCosmic microwave backgroundAstrophysics (astro-ph)FOS: Physical sciencesAstrophysicsCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsRenormalization groupAstrophysicsGeneral Relativity and Quantum CosmologyCosmologyUniverseHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Vacuum energyHigh Energy Physics - Theory (hep-th)Mathematical physicsmedia_commonQuintessencePhysics Letters B
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