Search results for "Particles"

showing 10 items of 8085 documents

Small and hollow magnetic monopoles

2018

We deal with the presence of magnetic monopoles in a non Abelian model that generalizes the standard 't~Hooft-Polyakov model in three spatial dimensions. We investigate the energy density of the static and spherically symmetric solutions to find first order differential equations that solve the equations of motion. The system is further studied and two distinct classes of solutions are obtained, one that can also be described by analytical solutions which is called small monopole, since it is significantly smaller than the standard 't~Hooft-Polyakov monopole. The other type of structure is the hollow monopole, since the energy density is endowed with a hole at its core. The hollow monopole …

High Energy Physics - TheoryPhysics010308 nuclear & particles physicsDifferential equationHigh Energy Physics::LatticeMathematical analysisMagnetic monopoleStructure (category theory)FOS: Physical sciencesEquations of motionPattern Formation and Solitons (nlin.PS)Type (model theory)Nonlinear Sciences - Pattern Formation and Solitons01 natural sciencesCondensed Matter - Other Condensed MatterCore (optical fiber)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Ordinary differential equation0103 physical sciencesEnergy density010306 general physicsOther Condensed Matter (cond-mat.other)Physical Review D
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Coupled dynamics in gluon mass generation and the impact of the three-gluon vertex

2018

We present a detailed study of the subtle interplay transpiring at the level of two integral equations that are instrumental for the dynamical generation of a gluon mass in pure Yang-Mills theories. The main novelty is the joint treatment of the Schwinger-Dyson equation governing the infrared behaviour of the gluon propagator and of the integral equation that controls the formation of massless bound-state excitations, whose inclusion is instrumental for obtaining massive solutions from the former equation. The self-consistency of the entire approach imposes the requirement of using a single value for the gauge coupling entering in the two key equations; its fulfillment depends crucially on …

High Energy Physics - TheoryPhysics010308 nuclear & particles physicsHigh Energy Physics::LatticeHigh Energy Physics - Lattice (hep-lat)Mass generationFOS: Physical sciencesPropagator01 natural sciencesIntegral equationGluonVertex (geometry)Massless particleHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - LatticeHigh Energy Physics - Theory (hep-th)Lattice (order)Quantum electrodynamics0103 physical sciences010306 general physicsMathematical physicsPhysical Review D
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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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Black hole radiance, short distances and TeV gravity.

2006

Using a derivation of black hole radiance in terms of two-point functions one can provide a quantitative estimate of the contribution of short distances to the spectrum. Thermality is preserved for black holes with $��l_P <<1$. However, deviations from the Planckian spectrum can be found for mini black holes in TeV gravity scenarios, even before reaching the Planck phase.

High Energy Physics - TheoryPhysicsAstrofísicaGravity (chemistry)Gravitació010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyQuàntums Teoria delsAstrophysics01 natural sciencesGravitationBlack holeMicro black holeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)0103 physical sciencesExtremal black holeRadiance010306 general physicsVirtual black holeHawking radiation
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Acceleration radiation, transition probabilities, and trans-Planckian physics

2010

An important question in the derivation of the acceleration radiation, which also arises in Hawking's derivation of black hole radiance, is the need to invoke trans-Planckian physics in describing the creation of quanta. We point out that this issue can be further clarified by reconsidering the analysis in terms of particle detectors, transition probabilities and local two-point functions. By writing down separate expressions for the spontaneous-and induced-transition probabilities of a uniformly accelerated detector, we show that the bulk of the effect comes from the natural (non-trans-Planckian) scale of the problem, which largely diminishes the importance of the trans-Planckian sector. T…

High Energy Physics - TheoryPhysicsAstrofísicaPhysics::General Physics010308 nuclear & particles physicsGeneral Physics and AstronomyFOS: Physical sciencesAcceleration (differential geometry)Scale (descriptive set theory)General Relativity and Quantum Cosmology (gr-qc)RadiationLorentz covariance01 natural sciencesGeneral Relativity and Quantum CosmologyPartícules (Física nuclear)Black holeTheoretical physicsHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHawkingHigh Energy Physics - Theory (hep-th)0103 physical sciencesRadianceQuantum field theory010306 general physics
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Mapping Ricci-based theories of gravity into general relativity

2018

We show that the space of solutions of a wide family of Ricci-based metric-affine theories of gravity can be put into correspondence with the space of solutions of general relativity (GR). This allows us to use well-established methods and results from GR to explore new gravitational physics beyond it.

High Energy Physics - TheoryPhysicsClass (set theory)Gravity (chemistry)010308 nuclear & particles physicsGeneral relativityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Space (mathematics)01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationTheoretical physicsHigh Energy Physics - Theory (hep-th)0103 physical sciences010306 general physics
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Exact spherically-symmetric inhomogeneous model withnperfect fluids

2011

We present the exact equations governing the dynamics of a spherically-symmetric inhomogeneous model with n decoupled and non-comoving perfect fluids. Thanks to the use of physically meaningful quantities we write the set of 3+2n equations in a concise and transparent way. The n perfect fluids can have general equations of state, thus making the model extremely flexible to study a large variety of cosmological and astrophysical problems. As applications we consider a model sourced by two non-comoving dust components and a cosmological constant, and a model featuring dust and a dark energy component with negligible speed of sound.

High Energy Physics - TheoryPhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsDark matterFOS: Physical sciencesExact differential equationAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsCosmological constant01 natural sciencesGeneral Relativity and Quantum CosmologySymmetry (physics)CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Speed of sound0103 physical sciencesDark energyCosmological perturbation theory010303 astronomy & astrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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No chiral light bending by clumps of axion-like particles

2019

We study the propagation of light in the presence of a parity-violating coupling between photons and axion-like particles (ALPs). Naively, this interaction could lead to a split of light rays into two separate beams of different polarization chirality and with different refraction angles. However, by using the eikonal method we explicitly show that this is not the case and that ALP clumps do not produce any spatial birefringence. This happens due to non-trivial variations of the photon's frequency and wavevector, which absorb time-derivatives and gradients of the ALP field. We argue that these variations represent a new way to probe the ALP-photon couping with precision frequency measuremen…

High Energy Physics - TheoryPhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)BirefringencePhoton010308 nuclear & particles physicsEikonal equationFOS: Physical sciencesPhysics::OpticsAstronomy and AstrophysicsPolarization (waves)01 natural sciencesMolecular physicsRayPhysics::GeophysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Space and Planetary Science0103 physical sciencesWave vectorChirality (chemistry)010303 astronomy & astrophysicsAxionAstrophysics - Cosmology and Nongalactic Astrophysics
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Differential equations for loop integrals in Baikov representation

2018

We present a proof that differential equations for Feynman loop integrals can always be derived in Baikov representation without involving dimension-shift identities. We moreover show that in a large class of two- and three-loop diagrams it is possible to avoid squared propagators in the intermediate steps of setting up the differential equations.

High Energy Physics - TheoryPhysicsFor loopLarge class010308 nuclear & particles physicsDifferential equationPropagatorFOS: Physical sciences01 natural sciencesLoop integralLoop (topology)High Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)0103 physical sciencessymbolsFeynman diagramApplied mathematics010306 general physicsRepresentation (mathematics)Physical Review D
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Composite operators in asymptotic safety

2017

We study the role of composite operators in the Asymptotic Safety program for quantum gravity. By including in the effective average action an explicit dependence on new sources we are able to keep track of operators which do not belong to the exact theory space and/or are normally discarded in a truncation. Typical examples are geometric operators such as volumes, lengths, or geodesic distances. We show that this set-up allows to investigate the scaling properties of various interesting operators via a suitable exact renormalization group equation. We test our framework in several settings, including Quantum Einstein Gravity, the conformally reduced Einstein-Hilbert truncation, and two dim…

High Energy Physics - TheoryPhysicsGeodesic010308 nuclear & particles physicsTruncationAsymptotic safety in quantum gravityFOS: Physical sciencesObservableGeneral Relativity and Quantum Cosmology (gr-qc)Operator theoryRenormalization group01 natural sciencesGeneral Relativity and Quantum CosmologyAction (physics)Theoretical physicsHigh Energy Physics - Theory (hep-th)Quantum mechanics0103 physical sciencesQuantum gravity010306 general physicsPhysical Review D
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