Search results for "SCALAR"

showing 10 items of 1002 documents

N-quantum approach to quantum field theory at finite T and mu: the NJL model

1999

We extend the N-quantum approach to quantum field theory to finite temperature ($T$) and chemical potential ($\mu$) and apply it to the NJL model. In this approach the Heisenberg fields are expressed using the Haag expansion while temperature and chemical potential are introduced simultaneously through a generalized Bogoliubov transformation. Known mean field results are recovered using only the first term in the Haag expansion. In addition, we find that at finite T and in the broken symmetry phase of the model the mean field approximation can not diagonalize the Hamiltonian. Inclusion of scalar and axial vector diquark channels in the SU(2)$_{rm f}$ $otimes$ SU(3)$_{\rm c}$ version of the …

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsParticle physicsNuclear TheoryScalar (mathematics)Order (ring theory)FísicaHigh Energy Physics - Phenomenologysymbols.namesakeBogoliubov transformationVacuum energyMean field theorysymbolsQuantum field theoryHamiltonian (quantum mechanics)PseudovectorMathematical physics
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PRIME NUMBERS, QUANTUM FIELD THEORY AND THE GOLDBACH CONJECTURE

2012

Motivated by the Goldbach conjecture in Number Theory and the abelian bosonization mechanism on a cylindrical two-dimensional spacetime we study the reconstruction of a real scalar field as a product of two real fermion (so-called \textit{prime}) fields whose Fourier expansion exclusively contains prime modes. We undertake the canonical quantization of such prime fields and construct the corresponding Fock space by introducing creation operators $b_{p}^{\dag}$ --labeled by prime numbers $p$-- acting on the vacuum. The analysis of our model, based on the standard rules of quantum field theory and the assumption of the Riemann hypothesis, allow us to prove that the theory is not renormalizabl…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsPure mathematicsMathematics - Number TheoryCanonical quantizationPrime numberFOS: Physical sciencesFísicaAstronomy and AstrophysicsMathematical Physics (math-ph)Atomic and Molecular Physics and OpticsPrime (order theory)Riemann hypothesissymbols.namesakeNumber theoryHigh Energy Physics - Theory (hep-th)Goldbach's conjectureFOS: MathematicssymbolsNumber Theory (math.NT)Quantum field theoryScalar fieldMathematical PhysicsInternational Journal of Modern Physics A
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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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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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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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Comment on `Critical scalar field collapse in AdS$_3$: an analytical approach'

2014

We comment on the derivation of an analytical solution presented in arXiv:1309.1629, show that it belongs to a family of separable solutions previously constructed in arXiv:gr-qc/0109002, and question its relevance to critical collapse.

High Energy Physics - TheoryPhysicsPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsCollapse (topology)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologySeparable spaceTheoretical physicsHigh Energy Physics - Theory (hep-th)0103 physical sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]010306 general physicsScalar field
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General invertible transformation and physical degrees of freedom

2017

An invertible field transformation is such that the old field variables correspond one-to-one to the new variables. As such, one may think that two systems that are related by an invertible transformation are physically equivalent. However, if the transformation depends on field derivatives, the equivalence between the two systems is nontrivial due to the appearance of higher derivative terms in the equations of motion. To address this problem, we prove the following theorem on the relation between an invertible transformation and Euler-Lagrange equations: If the field transformation is invertible, then any solution of the original set of Euler-Lagrange equations is mapped to a solution of …

High Energy Physics - TheoryPhysicsPure mathematicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsEquations of motionMaterial derivativeClassical Physics (physics.class-ph)FOS: Physical sciencesPhysics - Classical PhysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyTensor fieldlaw.inventionField transformationInvertible matrixHigh Energy Physics - Theory (hep-th)law0103 physical sciencesEquivalence (formal languages)010306 general physicsField equationScalar fieldAstrophysics - Cosmology and Nongalactic Astrophysics
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Continuous-variable entanglement sharing in noninertial frames

2007

We study the distribution of entanglement between modes of a free scalar field from the perspective of observers in uniform acceleration. We consider a two-mode squeezed state of the field from an inertial perspective, and analytically study the degradation of entanglement due to the Unruh effect, in the cases of either one or both observers undergoing uniform acceleration. We find that for two observers undergoing finite acceleration, the entanglement vanishes between the lowest frequency modes. The loss of entanglement is precisely explained as a redistribution of the inertial entanglement into multipartite quantum correlations among accessible and unaccessible modes from a non-inertial p…

High Energy Physics - TheoryPhysicsQuantum PhysicsInertial frame of referenceStatistical Mechanics (cond-mat.stat-mech)FOS: Physical sciencesAcceleration (differential geometry)General Relativity and Quantum Cosmology (gr-qc)Quantum PhysicsQuantum entanglementSquashed entanglementGeneral Relativity and Quantum CosmologyAtomic and Molecular Physics and OpticsMultipartiteUnruh effectClassical mechanicsHigh Energy Physics - Theory (hep-th)Quantum mechanicsQuantum Physics (quant-ph)Scalar fieldCondensed Matter - Statistical MechanicsSqueezed coherent state
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Sum rules for light-by-light scattering

2010

We derive a set of sum rules for the light-by-light scattering and fusion: $\gamma\gamma \to all$, and verify them in lowest order QED calculations. A prominent implication of these sum rules is the superconvergence of the helicity-difference total cross-section for photon fusion, which in the hadron sector reveals an intricate cancellation between the pseudoscalar and tensor mesons. An experimental verification of superconvergence of the polarized photon fusion into hadrons is called for, but will only be possible at $e^+ e^-$ and $\gamma\gamma$ colliders with both beams polarized. We also show how the sum rules can be used to measure various contributions to the low-energy light-by-light …

High Energy Physics - TheoryPhysicsQuantum PhysicsParticle physicsPhotonNuclear TheoryMesonScatteringHadronHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyOrder (ring theory)FOS: Physical sciencesElementary particleLight scatteringNuclear physicsPseudoscalarNuclear Theory (nucl-th)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Quantum Physics (quant-ph)
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