Search results for "SCALAR"

showing 10 items of 1002 documents

An alternative scenario for critical scalar field collapse in $AdS_3$

2016

In the context of gravitational collapse and black hole formation, we reconsider the problem to describe analytically the critical collapse of a massless and minimally coupled scalar field in $2+1$ gravity.

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)Particle physicsBlack HolesCritical phenomenaAstrophysics::High Energy Astrophysical PhenomenaCollapse (topology)FOS: Physical sciencesContext (language use)Critical collapseGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics::TheoryGeneral Relativity and Quantum Cosmology0103 physical sciencesGravitational collapse010306 general physicsComputingMilieux_MISCELLANEOUSPhysics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]010308 nuclear & particles physicsMassless particle2+1 gravityHigh Energy Physics - Theory (hep-th)Anti-de Sitter spaceScalar field
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Derivation of spontaneously broken gauge symmetry from the consistency of effective field theory II: Scalar field self-interactions and the electroma…

2019

We extend our study of deriving the local gauge invariance with spontaneous symmetry breaking in the context of an effective field theory by considering self-interactions of the scalar field and inclusion of the electromagnetic interaction. By analyzing renormalizability and the scale separation conditions of three-, four- and five-point vertex functions of the scalar field, we fix the two couplings of the scalar field self-interactions of the leading order Lagrangian. Next we add the electromagnetic interaction and derive conditions relating the magnetic moment of the charged vector boson to its charge and the masses of the charged and neutral massive vector bosons to each other and the tw…

High Energy Physics - TheoryNuclear and High Energy PhysicsNuclear TheorySpontaneous symmetry breakingFOS: Physical sciences01 natural sciencesStandard ModelVector bosonNuclear Theory (nucl-th)Theoretical physicsHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesEffective field theoryddc:530Gauge theory010306 general physicsGauge symmetryPhysics010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics - Lattice (hep-lat)lcsh:QC1-999High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Scalar fieldlcsh:Physics
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Derivation of spontaneously broken gauge symmetry from the consistency of effective field theory I: Massive vector bosons coupled to a scalar field

2018

We revisit the problem of deriving local gauge invariance with spontaneous symmetry breaking in the context of an effective field theory. Previous derivations were based on the condition of tree-order unitarity. However, the modern point of view considers the Standard Model as the leading order approximation to an effective field theory. As tree-order unitarity is in any case violated by higher-order terms in an effective field theory, it is instructive to investigate a formalism which can be also applied to analyze higher-order interactions. In the current work we consider an effective field theory of massive vector bosons interacting with a massive scalar field. We impose the conditions o…

High Energy Physics - TheoryNuclear and High Energy PhysicsNuclear TheorySpontaneous symmetry breakingFOS: Physical sciences53001 natural sciencesRenormalizationNuclear Theory (nucl-th)Theoretical physicsHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesEffective field theoryddc:530Gauge theory010306 general physicsGauge symmetryPhysicsCoupling constantUnitarity010308 nuclear & particles physicsHigh Energy Physics - Lattice (hep-lat)lcsh:QC1-999High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Scalar fieldlcsh:Physics
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Elementary Goldstone Higgs boson and dark matter

2015

We investigate a perturbative extension of the Standard Model featuring elementary pseudo-Goldstone Higgs and dark matter particles. These are two of the five Goldstone bosons parametrising the SU(4)/Sp(4) coset space. They acquire masses, and therefore become pseudo-Goldstone bosons, due to the embedding of the Yukawa and the electroweak gauge interactions that do not preserve the full SU(4) symmetry. At the one-loop order the top corrections dominate and align the vacuum in the direction where the Higgs is mostly a pseudo-Goldstone boson. Because of the perturbative and elementary nature of the theory, the quantum corrections are precisely calculable. The remaining pseudo-Goldstone boson …

High Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsHiggs bosonHigh Energy Physics::LatticeFOS: Physical sciencesElementary particleTechnicolor01 natural sciencesdark matterStandard Modelsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Goldstone bosons0103 physical sciences010306 general physicsCondensed Matter::Quantum GasesPhysicsGauge bosonta114relic densityelectroweak interaction010308 nuclear & particles physicshep-thHigh Energy Physics::Phenomenologyhep-phHigh Energy Physics - PhenomenologyHiggs fieldscalar particleHigh Energy Physics - Theory (hep-th)symbolsHiggs bosonLHCHiggs mechanismMinimal Supersymmetric Standard ModelPhysical Review D
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Subleading Regge limit from a soft anomalous dimension

2018

Wilson lines capture important features of scattering amplitudes, for example soft effects relevant for infrared divergences, and the Regge limit. Beyond the leading power approximation, corrections to the eikonal picture have to be taken into account. In this paper, we study such corrections in a model of massive scattering amplitudes in N = 4 super Yang-Mills, in the planar limit, where the mass is generated through a Higgs mechanism. Using known three-loop analytic expressions for the scattering amplitude, we find that the first power suppressed term has a very simple form, equal to a single power law. We propose that its exponent is governed by the anomalous dimension of a Wilson loop w…

High Energy Physics - TheoryNuclear and High Energy PhysicsWilson loopScalar (mathematics)FOS: Physical sciencesComputer Science::Digital Libraries01 natural sciencesPower lawSupersymmetric Gauge Theorysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityScattering Amplitudes010306 general physicsMathematical physicsPhysics010308 nuclear & particles physicsEikonal equation16. Peace & justiceWilson ’t Hooft and Polyakov loopsScattering amplitudeHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics - Theory (hep-th)Computer Science::Mathematical SoftwareExponentsymbolslcsh:QC770-798Higgs mechanismJournal of High Energy Physics
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Revising the Predictions of Inflation for the Cosmic Microwave Background Anisotropies

2009

4 pages, 1 figure.-- PACS nrs.: 98.70.Vc; 11.10.Gh; 98.80.Cq.-- ArXiv pre-print available at: http://arxiv.org/abs/0901.0439

High Energy Physics - TheoryParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Scalar (mathematics)Cosmic microwave backgroundFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)[PACS] Cosmic background radiations01 natural sciencesGeneral Relativity and Quantum CosmologySpectral lineRenormalizationHigh Energy Physics - Phenomenology (hep-ph)[PACS] Particle-theory and field-theory models of the early UniverseQuantum mechanics0103 physical sciencesQuantum field theory010306 general physicsPhysicsInflation (cosmology)010308 nuclear & particles physicsSpectral densityCMB cold spot3. Good healthHigh Energy Physics - Phenomenology[PACS] Renormalization in quantum field theoryHigh Energy Physics - Theory (hep-th)Astrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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Planck-scale effects on WIMP dark matter

2014

There exists a widely known conjecture that gravitational effects violate global symmetries. We study the effect of global-symmetry violating higher-dimension operators induced by Planck-scale physics on the properties of WIMP dark matter. Using an effective description, we show that the lifetime of the WIMP dark matter candidate can satisfy cosmological bounds under reasonable assumptions regarding the strength of the dimension-five operators. On the other hand, the indirect WIMP dark matter detection signal is significantly enhanced due to new decay channels.

High Energy Physics - TheoryParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)WIMPMaterials Science (miscellaneous)Scalar field dark matterBiophysicsFOS: Physical sciencesGeneral Physics and AstronomyAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesdark matterHigh Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciencesWarm dark matterindirect detectionparticle physicsPhysical and Theoretical Chemistry010306 general physicsLight dark matterMathematical PhysicsDark Matter PhenomenologyPhysics010308 nuclear & particles physicsHot dark matterPhysicsWIMP dark matterFísicalcsh:QC1-999decaying dark matterHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)astroparticle physicsWeakly interacting massive particlesPlanck scale effectsMixed dark matterdirect detectionHigh Energy Physics::Experimentlcsh:PhysicsDark fluidAstrophysics - Cosmology and Nongalactic AstrophysicsFrontiers in Physics
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Adiabatic regularization for Dirac fields in time-varying electric backgrounds

2020

The adiabatic regularization method was originally proposed by Parker and Fulling to renormalize the energy-momentum tensor of scalar fields in expanding universes. It can be extended to renormalize the electric current induced by quantized scalar fields in a time-varying electric background. This can be done in a way consistent with gravity if the vector potential is considered as a variable of adiabatic order one. Assuming this, we further extend the method to deal with Dirac fields in four spacetime dimensions. This requires a self-consistent ansatz for the adiabatic expansion, in presence of a prescribed time-dependent electric field, which is different from the conventional expansion u…

High Energy Physics - TheoryPhysics010308 nuclear & particles physicsConformal anomalyScalar (mathematics)FOS: Physical sciencesField strengthGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum electrodynamicsElectric fieldRegularization (physics)0103 physical sciences010306 general physicsAdiabatic processAnsatzVector potentialPhysical Review
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Operator product expansion coefficients in the exact renormalization group formalism

2020

We study how to compute the operator product expansion coefficients in the exact renormalization group formalism. After discussing possible strategies, we consider some examples explicitly, within the $\epsilon$-expansions, for the Wilson-Fisher fixed points of the real scalar theory in $d=4-\epsilon$ dimensions and the Lee-Yang model in $d=6-\epsilon$ dimensions. Finally we discuss how our formalism may be extended beyond perturbation theory.

High Energy Physics - TheoryPhysics010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Scalar (mathematics)FOS: Physical sciencesFixed pointRenormalization group16. Peace & justiceComputer Science::Digital Libraries01 natural sciencesoperator product expansionfield theory in curved spaceFormalism (philosophy of mathematics)Formal aspects of field theoryHigh Energy Physics - Theory (hep-th)fixed point0103 physical sciencesLee-Yang modelOperator product expansionrenormalization group010306 general physicsMathematical physicsperturbation theory
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Investigating the Ultraviolet Properties of Gravity with a Wilsonian Renormalization Group Equation

2008

We review and extend in several directions recent results on the asymptotic safety approach to quantum gravity. The central issue in this approach is the search of a Fixed Point having suitable properties, and the tool that is used is a type of Wilsonian renormalization group equation. We begin by discussing various cutoff schemes, i.e. ways of implementing the Wilsonian cutoff procedure. We compare the beta functions of the gravitational couplings obtained with different schemes, studying first the contribution of matter fields and then the so-called Einstein-Hilbert truncation, where only the cosmological constant and Newton's constant are retained. In this context we make connection with…

High Energy Physics - TheoryPhysicsAsymptotic safety in quantum gravityGeneral Physics and AstronomyFOS: Physical sciencesCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)Renormalization groupFixed pointGeneral Relativity and Quantum CosmologyGravitationHigh Energy Physics - Theory (hep-th)Quantum gravityConstant (mathematics)Scalar curvatureMathematical physics
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