Search results for "EXPANSION"

showing 10 items of 630 documents

Renormalisation group improvement in the stochastic formalism

2019

We investigate compatibility between the stochastic infrared (IR) resummation of light test fields on inflationary spacetimes and renormalisation group running of the ultra-violet (UV) physics. Using the Wilsonian approach, we derive improved stochastic Langevin and Fokker-Planck equations which consistently include the renormalisation group effects. With the exception of stationary solutions, these differ from the naive approach of simply replacing the classical potential in the standard stochastic equations with the renormalisation group improved potential. Using this new formalism, we exemplify the IR dynamics with the Yukawa theory during inflation, illustrating the differences between …

High Energy Physics - TheoryGAUGED NJL-MODELgr-qcHigh Energy Physics::LatticeFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsHigh Energy Physics - Phenomenology (hep-ph)PROPAGATORFLATNESSHORIZON0201 Astronomical and Space Sciences0103 physical sciencesphysics of the early universeinflationINFLATIONARY UNIVERSE SCENARIOResummationMathematical physicsPhysicsScience & Technology010308 nuclear & particles physicsPhysicshep-thYukawa potentialhep-phAstronomy and AstrophysicsEXPANSIONNuclear & Particles Physicsquantum field theory on curved spaceFormalism (philosophy of mathematics)High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)particle physics - cosmology connectionINTERACTING SCALAR FIELDVACUUMPhysical Sciences0202 Atomic Molecular Nuclear Particle and Plasma PhysicsPHASE-TRANSITIONGENERATION
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Einstein, Planck and Vera Rubin: Relevant Encounters Between the Cosmological and the Quantum Worlds

2021

In Cosmology and in Fundamental Physics there is a crucial question like: where the elusive substance that we call Dark Matter is hidden in the Universe and what is it made of? that, even after 40 years from the Vera Rubin seminal discovery [1] does not have a proper answer. Actually, the more we have investigated, the more this issue has become strongly entangled with aspects that go beyond the established Quantum Physics, the Standard Model of Elementary particles and the General Relativity and related to processes like the Inflation, the accelerated expansion of the Universe and High Energy Phenomena around compact objects. Even Quantum Gravity and very exotic Dark Matter particle candid…

High Energy Physics - TheoryGeneral Physics and AstronomyNature of dark matter01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologyClassical vs quantum cosmologyHigh Energy Physics - Phenomenology (hep-ph)010303 astronomy & astrophysicsQuantumMathematical PhysicsQuantum gravity and cosmologyPhysicsModification of general relativityChaplygin Gaslcsh:QC1-999CosmologyHigh Energy Physics - PhenomenologyExpansion of the UniversesymbolsGeneral RelativityGeneral relativityMaterials Science (miscellaneous)BiophysicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Metric expansion of spacesymbols.namesakeTheory of relativitySettore FIS/05 - Astronomia e Astrofisica0103 physical sciencesDark matterddc:530Cosmological ModelsPhysical and Theoretical ChemistryPlanckEinsteindark matter; galaxies; nature of dark matter; beyond standard model; modification of general relativity; quantum gravity and cosmology; expansion of the Universe010308 nuclear & particles physicsFísicaGalaxiesAstrophysics - Astrophysics of GalaxiesCosmosEpistemologyHigh Energy Physics - Theory (hep-th)quantum gravityAstrophysics of Galaxies (astro-ph.GA)Quantum gravityBeyond standard modellcsh:Physics
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Numerical evaluation of iterated integrals related to elliptic Feynman integrals

2021

We report on an implementation within GiNaC to evaluate iterated integrals related to elliptic Feynman integrals numerically to arbitrary precision within the region of convergence of the series expansion of the integrand. The implementation includes iterated integrals of modular forms as well as iterated integrals involving the Kronecker coefficient functions $g^{(k)}(z,\tau)$. For the Kronecker coefficient functions iterated integrals in $d\tau$ and $dz$ are implemented. This includes elliptic multiple polylogarithms.

High Energy Physics - TheoryKronecker coefficientFeynman integralModular formFOS: Physical sciencesGeneral Physics and AstronomyMathematical Physics (math-ph)01 natural sciences010305 fluids & plasmasAlgebraHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Hardware and ArchitectureIterated integrals0103 physical sciencesArbitrary-precision arithmeticTrailing zero010306 general physicsSeries expansionLink (knot theory)Mathematical PhysicsMathematicsComputer Physics Communications
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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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Dark energy cosmologies for codimension-two branes

2005

A six-dimensional universe with two branes in the "football-shaped" geometry leads to an almost realistic cosmology. We describe a family of exact solutions with time dependent characteristic size of internal space. After a short inflationary period the late cosmology is either of quintessence type or turns to a radiation dominated Friedmann universe where the cosmological constant appears as a free integration constant of the solution. The radiation dominated universe with relativistic fermions is analyzed in detail, including its dimensional reduction.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsBig RipFOS: Physical sciencesNon-standard cosmologyLambda-CDM modelCosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsMetric expansion of spaceTheoretical physicsGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)De Sitter universeQuantum cosmologyScale factor (cosmology)
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The cosmological constant problem in codimension-two brane models

2005

We discuss the possibility of a dynamical solution to the cosmological constant problem in the contaxt of six-dimensional Einstein-Maxwell theory. A definite answer requires an understanding of the full bulk cosmology in the early universe, in which the bulk has time-dependent size and shape. We comment on the special properties of codimension two as compared to higher codimensions.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsFOS: Physical sciencesNon-standard cosmologyCosmological constantMetric expansion of spaceGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physicsClassical mechanicsHigh Energy Physics - Theory (hep-th)De Sitter universeFriedmann–Lemaître–Robertson–Walker metricBrane cosmologysymbolsBraneCosmological constant problemPhysics Letters B
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A note on Einstein gravity on AdS(3) and boundary conformal field theory

1998

We find a simple relation between the first subleading terms in the asymptotic expansion of the metric field in AdS$_3$, obeying the Brown-Henneaux boundary conditions, and the stress tensor of the underlying Liouville theory on the boundary. We can also provide an more explicit relation between the bulk metric and the boundary conformal field theory when it is described in terms of a free field with a background charge.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsField (physics)Cauchy stress tensorBoundary (topology)Boundary conformal field theoryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Free fieldGeneral Relativity and Quantum Cosmologysymbols.namesakeHigh Energy Physics - Theory (hep-th)symbolsAstronomiaBoundary value problemCamps Teoria quàntica deEinsteinAsymptotic expansionMathematical physics
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Constraining inverse-curvature gravity with supernovae

2005

We show that the current accelerated expansion of the Universe can be explained without resorting to dark energy. Models of generalized modified gravity, with inverse powers of the curvature can have late time accelerating attractors without conflicting with solar system experiments. We have solved the Friedman equations for the full dynamical range of the evolution of the Universe. This allows us to perform a detailed analysis of Supernovae data in the context of such models that results in an excellent fit. Hence, inverse curvature gravity models represent an example of phenomenologically viable models in which the current acceleration of the Universe is driven by curvature instead of dar…

High Energy Physics - TheoryPhysicsPhantom energyAstrophysics (astro-ph)FOS: Physical sciencesGeneral Physics and AstronomyBig RipGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGeneral Relativity and Quantum CosmologyParticle horizonMetric expansion of spaceTheoretical physicsHigh Energy Physics - Theory (hep-th)De Sitter universeZero-energy universeFlatness problemScale factor (cosmology)
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The kite integral to all orders in terms of elliptic polylogarithms

2016

We show that the Laurent series of the two-loop kite integral in $D=4-2\varepsilon$ space-time dimensions can be expressed in each order of the series expansion in terms of elliptic generalisations of (multiple) polylogarithms. Using differential equations we present an iterative method to compute any desired order. As an example, we give the first three orders explicitly.

High Energy Physics - TheoryPure mathematics010308 nuclear & particles physicsIterative methodDifferential equationNumerical analysisLaurent seriesOrder (ring theory)FOS: Physical sciencesStatistical and Nonlinear PhysicsMathematical Physics (math-ph)01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Kite0103 physical sciencesBoundary value problem010306 general physicsSeries expansionMathematical PhysicsMathematics
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Renormalization group analysis of the gluon mass equation

2014

In the present work we carry out a systematic study of the renormalization properties of the integral equation that determines the momentum evolution of the effective gluon mass. A detailed, all-order analysis of the complete kernel appearing in this particular equation reveals that the renormalization procedure may be accomplished through the sole use of ingredients known from the standard perturbative treatment of the theory, with no additional assumptions. However, the subtle interplay of terms operating at the level of the exact equation gets distorted by the approximations usually employed when evaluating the aforementioned kernel. This fact is reflected in the form of the obtained sol…

High Energy Physics - TheoryQuarkQuantum chromodynamicsPhysicsNuclear and High Energy PhysicsHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciencesRenormalization groupInvariant (physics)Integral equationPartícules (Física nuclear)Mass formulaRenormalizationHigh Energy Physics - PhenomenologyTheoretical physicsHigh Energy Physics - LatticeClassical mechanicsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Operator product expansion
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