Search results for "Theoretical physics"

showing 10 items of 751 documents

Discrete Abelian gauge symmetries and axions

2015

We combine two popular extensions of beyond the Standard Model physics within the framework of intersecting D6-brane models: discrete Zn symmetries and Peccei-Quinn axions. The underlying natural connection between both extensions is formed by the presence of massive U(1) gauge symmetries in D-brane model building. Global intersecting D6-brane models on toroidal orbifolds of the type T6/Z2N and T6/Z2xZ2M with discrete torsion offer excellent playgrounds for realizing these extensions. A generation-dependent Z2 symmetry is identified in a global Pati-Salam model, while global left-right symmetric models give rise to supersymmetric realizations of the DFSZ axion model. In one class of the lat…

High Energy Physics - TheoryHistoryPhysics beyond the Standard ModelFOS: Physical sciencesD-brane01 natural sciencesEducationTheoretical physicsHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)Non-trivialGauge symmetries0103 physical sciencesAbelian group010306 general physicsAxionPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaCharge (physics)Gauge (firearms)16. Peace & justiceSymmetry (physics)Computer Science ApplicationsStandard Model (mathematical formulation)High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Homogeneous spaceStandard model
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Black Hole Entropy Quantization

2006

Ever since the pioneer works of Bekenstein and Hawking, black hole entropy has been known to have a quantum origin. Furthermore, it has long been argued by Bekenstein that entropy should be quantized in discrete (equidistant) steps given its identification with horizon area in (semi-)classical general relativity and the properties of area as an adiabatic invariant. This lead to the suggestion that black hole area should also be quantized in equidistant steps to account for the discrete black hole entropy. Here we shall show that loop quantum gravity, in which area is {\it not} quantized in equidistant steps can nevertheless be consistent with Bekenstein's equidistant entropy proposal in a s…

High Energy Physics - TheoryHolographic principlePhysicsWhite holeBlack hole information paradoxBekenstein boundFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyTheoretical physicsClassical mechanicsHigh Energy Physics - Theory (hep-th)Extremal black holeBlack hole thermodynamicsBlack hole complementarityHawking radiationPhysical Review Letters
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Intersecting Defects and Supergroup Gauge Theory

2021

Journal of physics / A 54(43), 435401 (2021). doi:10.1088/1751-8121/ac2716

High Energy Physics - TheoryInstantondimension: 5supersymmetry: algebra[PHYS.MPHY]Physics [physics]/Mathematical Physics [math-ph]General Physics and Astronomy01 natural sciencesHigh Energy Physics::Theorytopological [string]Mathematics - Quantum AlgebraGauge theorytopological stringsMathematical PhysicsdefectsPhysics[PHYS]Physics [physics][PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Chern-Simons termsupergroups[PHYS.MPHY] Physics [physics]/Mathematical Physics [math-ph]algebra [supersymmetry]5 [dimension]geometrical [transition]Modeling and SimulationEmbeddingBPSinstanton010307 mathematical physicsSupergroupStatistics and Probabilitysupersymmetry [gauge field theory]defectFOS: Physical sciencesDuality (optimization)Unitary state530Supersymmetric gauge theoryTheoretical physicsIntersectiongauge field theory: supersymmetry0103 physical sciencesFOS: Mathematicsstring: topologicalQuantum Algebra (math.QA)ddc:530Abelian grouptransition: geometrical010308 nuclear & particles physicsStatistical and Nonlinear PhysicsHigh Energy Physics - Theory (hep-th)Chern-Simons theory[PHYS.HTHE] Physics [physics]/High Energy Physics - Theory [hep-th]
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Palatini actions and quantum gravity phenomenology

2011

We show that an invariant an universal length scale can be consistently introduced in a generally covariant theory through the gravitational sector using the Palatini approach. The resulting theory is able to capture different aspects of quantum gravity phenomenology in a single framework. In particular, it is found that in this theory field excitations propagating with different energy-densities perceive different background metrics, which is a fundamental characteristic of the DSR and Rainbow Gravity approaches. We illustrate these properties with a particular gravitational model and explicitly show how the soccer ball problem is avoided in this framework. The isotropic and anisotropic cosmol…

High Energy Physics - TheoryLength scalePhysicsFOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (physics)General Relativity and Quantum CosmologyGravitationTheoretical physicsGeneral Relativity and Quantum CosmologySingularityHigh Energy Physics - Theory (hep-th)Quantum gravityCovariant transformationPhenomenology (particle physics)Big Bounce
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Quantum gravitational decoherence from fluctuating minimal length and deformation parameter at the Planck scale

2020

Schemes of gravitationally induced decoherence are being actively investigated as possible mechanisms for the quantum-to-classical transition. Here, we introduce a decoherence process due to quantum gravity effects. We assume a foamy quantum spacetime with a fluctuating minimal length coinciding on average with the Planck scale. Considering deformed canonical commutation relations with a fluctuating deformation parameter, we derive a Lindblad master equation that yields localization in energy space and decoherence times consistent with the currently available observational evidence. Compared to other schemes of gravitational decoherence, we find that the decoherence rate predicted by our mo…

High Energy Physics - TheoryLength scaleQuantum decoherenceScienceQuantum physicsGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Quantum spacetime01 natural sciencesGeneral Relativity and Quantum CosmologyArticleGeneral Biochemistry Genetics and Molecular BiologyGravitation0103 physical sciencesMaster equation010306 general physicsQuantumCondensed Matter - Statistical MechanicsPhysicsMesoscopic physicsMultidisciplinaryStatistical Mechanics (cond-mat.stat-mech)010308 nuclear & particles physicsQGeneral ChemistryClassical mechanicsHigh Energy Physics - Theory (hep-th)Quantum gravityQuantum Physics (quant-ph)Theoretical physics
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BPS preons in M-theory and supergravity

2007

7 pages.-- PACS nrs.: 11.30.Pb, 11.25.-w, 04.65.+e, 11.10.Kk.-- ISI Article Identifier: 000247103400029.-- ArXiv pre-print available at: http://arxiv.org/abs/hep-th/0702099

High Energy Physics - TheoryM-theoryPhysicsPhysics::General PhysicsSupergravityHigh Energy Physics::PhenomenologyFOS: Physical sciencesGeneral Physics and AstronomySupergravityM-theoryHigh Energy Physics::TheoryTheoretical physicsHigh Energy Physics - Theory (hep-th)Generalized holonomyConstituentsSupersymmetryQuantumBPS preonsFortschritte der Physik
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Infrared lessons for ultraviolet gravity: the case of massive gravity and Born-Infeld

2014

We generalize the ultraviolet sector of gravitation via a Born-Infeld action using lessons from massive gravity. The theory contains all of the elementary symmetric polynomials and is treated in the Palatini formalism. We show how the connection can be solved algebraically to be the Levi-Civita connection of an effective metric. The non-linearity of the algebraic equations yields several branches, one of which always reduces to General Relativity at low curvatures. We explore in detail a {\it minimal} version of the theory, for which we study solutions in the presence of a perfect fluid with special attention to the cosmological evolution. In vacuum we recover Ricci-flat solutions, but also…

High Energy Physics - TheoryModified gravityAlternatives to inflationCosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityGravityFOS: Physical sciencesPerfect fluidddc:500.2General Relativity and Quantum Cosmology (gr-qc)Space (mathematics)01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationsymbols.namesakeTheoretical physicsGeneral Relativity and Quantum Cosmology0103 physical sciencesEinstein010306 general physicsPhysics010308 nuclear & particles physicsEquation of state (cosmology)Astronomy and AstrophysicsMassive gravityHigh Energy Physics - Theory (hep-th)symbolsGravitational singularityAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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New scalar compact objects in Ricci-based gravity theories

2019

Taking advantage of a previously developed method, which allows to map solutions of General Relativity into a broad family of theories of gravity based on the Ricci tensor (Ricci-based gravities), we find new exact analytical scalar field solutions by mapping the free-field static, spherically symmetric solution of General Relativity (GR) into quadratic $f(R)$ gravity and the Eddington-inspired Born-Infeld gravity. The obtained solutions have some distinctive feature below the would-be Schwarzschild radius of a configuration with the same mass, though in this case no horizon is present. The compact objects found include wormholes, compact balls, shells of energy with no interior, and a new …

High Energy Physics - TheoryModified gravityFísica-Modelos matemáticosGeneral relativityGravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum Cosmology0103 physical sciencesFísica matemáticaWormhole010306 general physicsRicci curvaturePhysics010308 nuclear & particles physicsScalar (physics)Astronomy and AstrophysicsGR black holesBlack holeHigh Energy Physics - Theory (hep-th)Horizon (general relativity)WormholesScalar fieldSchwarzschild radius
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Matter dependence of the four-loop QCD cusp anomalous dimension: from small angles to all angles

2019

We compute the fermionic contributions to the cusp anomalous dimension in QCD at four loops as an expansion for small cusp angle. As a byproduct we also obtain the respective terms of the four-loop HQET wave function anomalous dimension. Our new results at small angles provide stringent tests of a recent conjecture for the exact angle dependence of the matter terms in the four-loop cusp anomalous dimension. We find that the conjecture does not hold for two of the seven fermionic color structures, but passes all tests for the remaining terms. This provides strong support for the validity of the corresponding conjectured expressions with full angle dependence. Taking the limit of large Minkow…

High Energy Physics - TheoryNuclear and High Energy PhysicsConformal anomalyFOS: Physical sciencesConformal map01 natural sciencesTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)Dimension (vector space)Perturbative QCD0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityScattering Amplitudes010306 general physicsWave functionQuantum chromodynamicsCusp (singularity)Physics010308 nuclear & particles physicsPerturbative QCDEffective Field TheoriesWilson ’t Hooft and Polyakov loopsScattering amplitudeHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)lcsh:QC770-798Journal of High Energy Physics
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Tensor bounds on the hidden universe

2018

During single clock inflation, hidden fields (i.e. fields coupled to the inflaton only gravitationally) in their adiabatic vacua can ordinarily only affect observables through virtual effects. After renormalizing background quantities (fixed by observations at some pivot scale), all that remains are logarithmic runnings in correlation functions that are both Planck and slow roll suppressed. In this paper we show how a large number of hidden fields can partially compensate this suppression and generate a potentially observable running in the tensor two point function, consistently inferable courtesy of a large $N$ resummation. We detour to address certain subtleties regarding loop correction…

High Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectCosmic microwave backgroundFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)ddc:500.201 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityTensorPlanck010306 general physicsmedia_commonPhysicsInflation (cosmology)Slow roll010308 nuclear & particles physicsScalar (physics)InflatonCosmology of Theories beyond the SMUniverseHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)symbolslcsh:QC770-798Renormalization Regularization and RenormalonsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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