Search results for "Mathematical physics"

showing 10 items of 2687 documents

Extraction of K --> pi pi matrix elements with Wilson fermions

2001

We present the status of a lattice calculation for the K-->pipi matrix elements of the (delta S=1) effective weak Hamiltonian, directly with two pion in the final state. We study the energy shift of two pion in a finite volume both in the I=0 and I=2 channels. We explain a method to avoid the Goldstone pole contamination in the computation of renormalization constants for (delta I=3/2) operators. Finally we show some preliminary results for the matrix elements of (delta I=1/2) operators. Our quenched simulation is done at beta=6.0, with Wilson fermions, on a (24^3 X 64) lattice.

PhysicsNuclear and High Energy PhysicsFinite volume methodComputationHigh Energy Physics::LatticeFermionAtomic and Molecular Physics and OpticsRenormalizationFIS/02 - FISICA TEORICA MODELLI E METODI MATEMATICIsymbols.namesakePionHigh Energy Physics - Latticelattice qcdLattice (order)visual_artvisual_art.visual_art_mediumsymbolsFísica nuclearHamiltonian (quantum mechanics)GoldstoneMathematical physics
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Current status of modified gravity

2014

We revisit the cosmological viability of the Hu-Sawicki modified gravity scenario. The impact of such a modification on the different cosmological observables, including gravitational waves, is carefully described. The most recent cosmological data, as well as constraints on the relationship between the clustering parameter ${\ensuremath{\sigma}}_{8}$ and the current matter mass-energy density ${\mathrm{\ensuremath{\Omega}}}_{m}$ from cluster number counts and weak lensing tomography, are considered in our numerical calculations. The strongest bound we find is $|{f}_{R0}|l3.7\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}6}$ at 95% C.L. Forthcoming cluster surveys covering $10\text{ …

PhysicsNuclear and High Energy PhysicsFísicaAstrophysics::Cosmology and Extragalactic AstrophysicsCosmological modelOmegaGalaxyCosmologyQuantum mechanicsAstronomiaGalaxy clusterWeak gravitational lensingMathematical physicsPhysical Review D
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Asymptotic properties of Born-improved amplitudes with gauge bosons in the final state

1999

For processes with gauge bosons in the final state we show how to continuously connect with a single Born-improved amplitude the resonant region, where resummation effects are important, with the asymptotic region far away from the resonance, where the amplitude must reduce to its tree-level form. While doing so all known field-theoretical constraints are respected, most notably gauge-invariance, unitarity and the equivalence theorem. The calculations presented are based on the process $f\bar{f}\to ZZ$, mediated by a possibly resonant Higgs boson; this process captures all the essential features, and can serve as a prototype for a variety of similar calculations. By virtue of massive cancel…

PhysicsNuclear and High Energy PhysicsGauge bosonParticle physicsUnitarityHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaState (functional analysis)Resonance (particle physics)RenormalizationHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics - Phenomenology (hep-ph)Higgs bosonResummationMathematical physicsParticle Physics - Phenomenology
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Interior spacetimes of stars in Palatinif(R)gravity

2006

We study the interior spacetimes of stars in the Palatini formalism of f(R) gravity and derive a generalized Tolman-Oppenheimer-Volkoff and mass equation for a static, spherically symmetric star. We show that matching the interior solution with the exterior Schwarzschild-De Sitter solution in general gives a relation between the gravitational mass and the density profile of a star, which is different from the one in General Relativity. These modifications become neglible in models for which $\delta F(R) \equiv \partial f/\partial R - 1$ is a decreasing function of R however. As a result, both Solar System constraints and stellar dynamics are perfectly consistent with $f(R) = R - \mu^4/R$.

PhysicsNuclear and High Energy PhysicsGeneral relativityAstrophysics (astro-ph)Dark matterFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsGeneral Relativity and Quantum CosmologyCosmologyMass formulaGravitationGeneral Relativity and Quantum CosmologyStarsClassical mechanicsStellar dynamicsf(R) gravityMathematical physicsPhysical Review D
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Reissner-Nordstr\"om black holes in extended Palatini theories

2012

We study static, spherically symmetric solutions with an electric field in an extension of general relativity (GR) containing a Ricci-squared term and formulated in the Palatini formalism. We find that all the solutions present a central core whose area is proportional to the Planck area times the number of charges. Far from the core, curvature invariants quickly tend to those of the usual Reissner-Nordstr\"om solution, though the structure of horizons may be different. In fact, besides the structures found in the Reissner-Nordstr\"om solution of GR, we find black hole solutions with just one nondegenerate horizon (Schwarzschild-like), and nonsingular black holes and naked cores. The charge…

PhysicsNuclear and High Energy PhysicsGeneral relativityCharged black holeCurvatureGeneral Relativity and Quantum Cosmologysymbols.namesakeFormalism (philosophy of mathematics)General Relativity and Quantum CosmologyClassical mechanicsElectric fieldsymbolsPlanckMathematical physics
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Collective subspaces for large amplitude motion and the generator coordinate method

1979

The collection path $|\ensuremath{\varphi}(q)〉$ to be used in a microscopic description of large amplitude collective motion is determined by means of the generator coordinate method. By varying the total energy with respect to $|\ensuremath{\varphi}(q)〉$ and performing an adiabatic expansion a hierarchy of equations is obtained which determines uniquely a hierarchy of collective paths with increasing complexity. To zeroth order the $|\ensuremath{\varphi}(q)〉$ are Slater determinants, to first order they include 2p-2h correlations. In both cases simple noninterative prescriptions for an explicit construction of the path are derived. For a correlated path their solutions agree at the Hartree…

PhysicsNuclear and High Energy PhysicsGenerator (category theory)Quantum mechanicsPath (graph theory)Slater determinantSemiclassical physicsPerturbation theory (quantum mechanics)Adiabatic processRandom phase approximationLinear subspaceMathematical physicsPhysical Review C
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Matrix elements of (delta S=2) operators with Wilson fermions

2002

We test the recent proposal of using the Ward identities to compute the K0-K0bar mixing amplitude with Wilson fermions, without the problem of spurious lattice subtractions. From our simulations, we observe no difference between the results obtained with and without subtractions. In addition, from the standard study of the complete set of (delta S=2) operators, we quote the following (preliminary) results (in the MS(NDR) scheme): Bk(2 GeV)=0.70(10), < O7^{3/2}>_{K->pi pi} = 0.10(2)(1) GeV^3, < O8^{3/2}>_{K->pi pi} = 0.49(6)(0) GeV^3.

PhysicsNuclear and High Energy PhysicsHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciencesFísicaFermionAtomic and Molecular Physics and OpticsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)AmplitudeHigh Energy Physics - LatticeLattice (order)PiMathematical physics
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Measure dependence of 2D simplicial quantum gravity

1995

We study pure 2D Euclidean quantum gravity with $R^2$ interaction on spherical lattices, employing Regge's formulation. We attempt to measure the string susceptibility exponent $\gamma_{\rm str}$ by using a finite-size scaling Ansatz in the expectation value of $R^2$. To check on effects of the path integral measure we investigate two scale invariant measures, the "computer" measure $dl/l$ and the Misner measure $dl/\sqrt A$.

PhysicsNuclear and High Energy PhysicsHigh Energy Physics - Lattice (hep-lat)Measure (physics)FOS: Physical sciencesExpectation valueScale invarianceEuclidean quantum gravityString (physics)Atomic and Molecular Physics and OpticsGeneral Relativity and Quantum CosmologyHigh Energy Physics - LatticePath integral formulationQuantum gravityAnsatzMathematical physics
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Displacement Operator Formalism for Renormalization and Gauge Dependence to All Orders

2005

We present a new method for determining the renormalization of Green functions to all orders in perturbation theory, which we call the displacement operator formalism, or the D-formalism, in short. This formalism exploits the fact that the renormalized Green functions may be calculated by displacing by an infinite amount the renormalized fields and parameters of the theory with respect to the unrenormalized ones. With the help of this formalism, we are able to obtain the precise form of the deformations induced to the Nielsen identities after renormalization, and thus derive the exact dependence of the renormalized Green functions on the renormalized gauge-fixing parameter to all orders. As…

PhysicsNuclear and High Energy PhysicsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaDisplacement operatorRenormalizationFormalism (philosophy of mathematics)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Quantum mechanicsMathematical physics
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Non-perturbative renormalisation of four fermion operators and B0 −B0 bar mixing with Wilson fermions

2003

We present new results for the renormalisation and subtraction constants for the four fermion DeltaF = 2 operators, computed non-perturbatively in the RI-MOM scheme (in the Landau gauge). From our preliminary analysis of the lattice data at beta = 6.45, for the B-0 - B-0,mixing bag-parameter we obtain B-B(RGI) = 1.46(7)(1).

PhysicsNuclear and High Energy PhysicsHigh Energy Physics::LatticeLattice (order)FísicaFermionNon-perturbativeAtomic and Molecular Physics and OpticsMathematical physicsPreliminary analysis
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