Search results for "theoretical physics"

showing 10 items of 751 documents

Implications of nonsymmetric metric theories for particle physics. New interpretation of the Pauli coupling

2014

In this work, we provide a possible geometrical interpretation of the spin of elementary particles. In particular, it is investigated how the wave equations of matter are altered by the addition of an antisymmetric contribution to the metric tensor. In this scenario, the explicit form of the matter wave equations is investigated in a general curved spacetime, and then the equations are particularized to the flat case. Unlike traditional approaches of Nonsymmetric Gravitational Theories (NGT), in which the gravitational field is responsible for breaking the symmetry of the flat Minkowski metric, we find more natural to consider that, in general, the metric of the spacetime could be nonsymme…

PhysicsNuclear and High Energy PhysicsAntisymmetric relationScalar (physics)General Physics and AstronomyAstronomy and AstrophysicsSymmetry (physics)General Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyTheoretical physicssymbols.namesakePauli exclusion principleMetric (mathematics)Minkowski spacesymbolsMetric tensor (general relativity)Spin-½
researchProduct

Charge radius of the neutrino

2000

Using the pinch technique we construct at one-loop order a neutrino charge radius, which is finite, depends neither on the gauge-fixing parameter nor on the gauge-fixing scheme employed, and is process independent. This definition stems solely from an effective proper photon-neutrino one-loop vertex, with no reference to box or self-energy contributions. The role of the $\mathrm{WW}$ box in this construction is critically examined. In particular it is shown that the exclusion of the effective $\mathrm{WW}$ box from the definition of the neutrino charge radius is not a matter of convention but is in fact dynamically realized when the target fermions are right-handedly polarized. In this way …

PhysicsNuclear and High Energy PhysicsCamps de galga (Física)Background field methodElectroweak interactionFermionsymbols.namesakeTheoretical physicsCharge radiusQuantum mechanicssymbolsFeynman diagramGauge theoryCamps Teoria quàntica deNeutrinoGauge fixing
researchProduct

Recent developments in effective field theory

2007

We will give a short introduction to the one-nucleon sector of chiral perturbation theory and will address the issue of a consistent power counting and renormalization. We will discuss the infrared regularization and the extended on-mass-shell scheme. Both allow for the inclusion of further degrees of freedom beyond pions and nucleons and the application to higher-loop calculations. As applications we consider the chiral expansion of the nucleon mass to order O(q^6) and the inclusion of vector and axial-vector mesons in the calculation of nucleon form factors.

PhysicsNuclear and High Energy PhysicsChiral perturbation theoryMesonNuclear TheoryHigh Energy Physics::LatticeNuclear TheoryDegrees of freedom (statistics)FOS: Physical sciencesRenormalizationNuclear Theory (nucl-th)Theoretical physicsPionRegularization (physics)Effective field theoryNucleonNuclear Experiment
researchProduct

String fields as limit of functions and surface terms in string field theory

1989

We consider the String Field Theory proposed by Witten in the discretized approach, where the string is considered as the limit N → ∞ of a collection of N points. In this picture the string functional is the limit of a succession of functions of an increasing number of variables; an object with some resemblances to distributions. Attention is drawn to the fact that the convergence is not of the uniform kind, and that therefore exchanges of limits, sums and integral signs can cause problems, and be ill defined. In this context we discuss some surface terms found by Woodard, which arise in integrations by parts, and argue that they depend crucially on the choice of the successions of functio…

PhysicsNuclear and High Energy PhysicsCompactification (physics)DiscretizationFísicaAstronomy and AstrophysicsString field theoryTopological string theoryRelationship between string theory and quantum field theoryAtomic and Molecular Physics and OpticsNon-critical string theoryTheoretical physicsQuantum mechanicsString cosmologyBoundary value problem
researchProduct

THE SPACE OF STRING CONFIGURATIONS IN STRING FIELD THEORY

1990

In this paper we consider the set of maps from the interval [0, π] which constitute the argument of the functionals of a String Field Theory. We show that in order to correctly reproduce results of the dual model one has to include all square integrable functions in the functional integral, or Ω0 in terms of Sobolev spaces.

PhysicsNuclear and High Energy PhysicsCompactification (physics)FísicaAstronomy and AstrophysicsString field theoryType I string theoryRelationship between string theory and quantum field theoryAtomic and Molecular Physics and OpticsSobolev spaceNon-critical string theoryTheoretical physicsClassical mechanicsSquare-integrable functionString cosmologyInternational Journal of Modern Physics A
researchProduct

Combinatorics of theSU(2)black hole entropy in loop quantum gravity

2009

We use the combinatorial and number-theoretical methods developed in previous works by the authors to study black hole entropy in the new proposal put forth by Engle, Noui, and Perez. Specifically, we give the generating functions relevant for the computation of the entropy and use them to derive its asymptotic behavior, including the value of the Immirzi parameter and the coefficient of the logarithmic correction.

PhysicsNuclear and High Energy PhysicsConfiguration entropyImmirzi parameterTheoryofComputation_GENERALLoop quantum gravityBinary entropy functionGeneral Relativity and Quantum CosmologyTheoretical physicsClassical mechanicsQuantum gravityBlack hole thermodynamicsEntropy (arrow of time)Joint quantum entropyPhysical Review D
researchProduct

Biases on cosmological parameters by general relativity effects

2012

General relativistic corrections to the galaxy power spectrum appearing at the horizon scale, if neglected, may induce biases on the measured values of the cosmological parameters. In this paper, we study the impact of general relativistic effects on non standard cosmologies such as scenarios with a time dependent dark energy equation of state, with a coupling between the dark energy and the dark matter fluids or with non-Gaussianities. We then explore whether general relativistic corrections affect future constraints on cosmological parameters in the case of a constant dark energy equation of state and of non-Gaussianities. We find that relativistic corrections on the power spectrum are no…

PhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsEquation of state (cosmology)Dark matterScalar field dark matterFísicaFOS: Physical sciencesLambda-CDM modelAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesPhysical cosmologyTheoretical physicsThermodynamics of the universeClassical mechanics0103 physical sciencesDark energy010303 astronomy & astrophysicsDark fluidAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Phenomenological approaches of inflation and their equivalence

2014

In this work, we analyze two possible alternative and model-independent approaches to describe the inflationary period. The first one assumes a general equation of state during inflation due to Mukhanov, while the second one is based on the slow-roll hierarchy suggested by Hoffman and Turner. We find that, remarkably, the two approaches are equivalent from the observational viewpoint, as they single out the same areas in the parameter space, and agree with the inflationary attractors where successful inflation occurs. Rephrased in terms of the familiar picture of a slowly rolling, canonically normalized scalar field, the resulting inflaton excursions in these two approaches are almost ident…

PhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsFísicaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsInflatonParameter space01 natural sciencessymbols.namesakeTheoretical physicsGeneral Relativity and Quantum Cosmology0103 physical sciencesAttractorsymbolsInflationary epochPlanck010306 general physicsScalar fieldEquivalence (measure theory)Eternal inflationAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Intrinsic energy of Lema\^itre-Tolman-Bondi models and cosmological implications

2013

Recently, some Lema{\^{\i}}tre-Tolman-Bondi metrics have been considered as models alternative to the dark energy within the Friedmann-Lema{\^{\i}}tre-Robertson-Walker universes. The vanishing of the intrinsic energy of these metrics is examined since such a vanishing, in the present case and in general, could be interpreted as a necessary condition to consider the possibility of the quantum creation of a metric. More specifically, this vanishing is examined in the particular case where the Lema{\^{\i}}tre-Tolman-Bondi metrics behave asymptotically like a Friedmann-Lema{\^{\i}}tre-Robertson-Walker universe. Finally, we deal with a particular model ruled out after being confronted with cosmi…

PhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmologiamedia_common.quotation_subjectFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsUniversePhysics::History of PhysicsGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum CosmologyRelativitat general (Física)Metric (mathematics)Dark energyValue (mathematics)QuantumEnergy (signal processing)media_commonAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Cosmology in a certain vector-tensor theory of gravitation

2014

We study relevant cosmological topics in the framework of a certain vector-tensor theory of gravitation (hereafter VT). This theory is first compared with the so-called extended electromagnetism (EE). These theories have a notable resemblance and both explain the existence of a cosmological constant. It is shown that, in EE, a positive dark energy density requires a Lagrangian leading to quantum ghosts, whereas VT is free from these ghosts. On account of this fact, the remainder of the paper is devoted to study cosmology in the framework of VT. Initial conditions, at high redshift, are used to solve the evolution equations of all the VT scalar modes. In particular, a certain scalar mode cha…

PhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityScalar (mathematics)FOS: Physical sciencesCosmological constantCosmologyStandard ModelGravitationTheoretical physicsCMBFASTDark energyAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct