Search results for " Set theory"

showing 10 items of 113 documents

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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Indirect dark matter search with the ANTARES neutrino telescope

2012

Using the data recorded by the ANTARES neutrino telescope during 2007 and 2008, a search for high energy neutrinos coming from the direction of the Sun has been performed. The neutrino selection criteria have been chosen so as to maximize the rejection of the atmospheric background with respect to possible signals produced by the self-annihilation of weakly interactive massive particles accumulated in the centre of the Sun. After data unblinding, the number of neutrinos observed was found to be compatible with background expectations. The results obtained were compared to the fluxes predicted by the Constrained Minimal Supersymmetric Standard Model, and 90% upper limits for this model were …

HistoryParticle physicsHigh energyAstrophysics::High Energy Astrophysical PhenomenaScalar (mathematics)Neutrino telescopeDark matterCompact dimensionFOS: Physical sciencesScale (descriptive set theory)EducationStandard ModelHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Direct searchInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MuonHigh Energy Physics::PhenomenologyGauginoAstrophysics::Instrumentation and Methods for AstrophysicsComputer Science ApplicationsHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsMinimal Supersymmetric Standard Model
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Searches for small-scale anisotropies from neutrino point sources with three years of IceCube data

2015

Recently, IceCube found evidence for a diffuse signal of astrophysical neutrinos in an energy range of $60\,\mathrm{TeV}$ to the $\mathrm{PeV}$-scale. The origin of those events, being a key to understanding the origin of cosmic rays, is still an unsolved question. So far, analyses have not succeeded to resolve the diffuse signal into point-like sources. Searches including a maximum-likelihood-ratio test, based on the reconstructed directions and energies of the detected down- and up-going neutrino candidates, were also performed on IceCube data leading to the exclusion of bright point sources. In this paper, we present two methods to search for faint neutrino point sources in three years o…

J.2Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayScale (descriptive set theory)AstrophysicsIceCubelaw.inventionTelescopelawPoint (geometry)Anisotropyastro-ph.HE2pt-correlationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHigh Energy Physics::Phenomenology2pt-correlation; Astrophysical neutrinos; Extraterrestrial neutrinos; IceCube; Multipole analysis; Point sourcesAstrophysics::Instrumentation and Methods for AstrophysicsPoint sourcesAstronomyAstronomy and AstrophysicsMultipole analysis3. Good health85-05Astrophysical neutrinosddc:540Extraterrestrial neutrinosHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaMultipole expansionGamma-ray burstAstroparticle Physics
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μ-e conversion in nuclei versus μ→e γ: an effective field theory point of view

1998

Using an effective lagrangian description we analyze possible new physics contributions to the most relevant muon number violating processes: $\mu \to e \gamma$ and $\mu$--$e$ conversion in nuclei. We identify a general class of models in which those processes are generated at one loop level and in which $\mu$--$e$ conversion is enhanced with respect to $\mu \to e \gamma$ by a large $\ln(m^2_\mu/\Lambda^2),$ where $\Lambda$ is the scale responsible for the new physics. For this wide class of models bounds on $\mu$--$e$ conversion constrain the scale of new physics more stringently than $\mu \to e \gamma$ already at present and, with the expected improvements in $\mu$--$e$ conversion experim…

Loop (topology)PhysicsNuclear and High Energy PhysicsParticle physicsMuonViolació CP (Física nuclear)Physics beyond the Standard ModelScalar (mathematics)Effective field theoryScale (descriptive set theory)Order of magnitudePartícules (Física nuclear)Lepton
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The Gaia-ESO Survey: matching chemodynamical simulations to observations of the Milky Way

2017

The typical methodology for comparing simulated galaxies with observational surveys is usually to apply a spatial selection to the simulation to mimic the region of interest covered by a comparable observational survey sample. In this work, we compare this approach with a more sophisticated post-processing in which the observational uncertainties and selection effects (photometric, surface gravity and effective temperature) are taken into account. We compare a 'solar neighbourhood analogue' region in a model MilkyWay-like galaxy simulated with RAMSES-CH with fourth release Gaia-ESO survey data. We find that a simple spatial cut alone is insufficient and that the observational uncertainties …

Matching (statistics)Milky Wayastro-ph.GAFOS: Physical sciencesScale (descriptive set theory)AstrophysicsF500Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesmethods: numerical0103 physical sciencesgalaxies: formation010303 astronomy & astrophysicsSelection (genetic algorithm)Astrophysics::Galaxy AstrophysicsPhysics[PHYS]Physics [physics]numerical [Methods]010308 nuclear & particles physicsgalaxies: evolution - galaxies: formationabundances [Galaxy]Astronomy and AstrophysicsEffective temperatureSurface gravityevolution [Galaxies]Astrophysics - Astrophysics of Galaxiesformation [Galaxies]GalaxyGalaxy: abundanceGalaxies: evolution; Galaxies: formation; Galaxy: abundances; Methods: numerical; Astronomy and Astrophysics; Space and Planetary ScienceSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Survey data collectionGalaxy: abundancesmethods: numerical - Galaxy: abundancesgalaxies: evolution[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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A Simple Metaheuristic for the FleetSize and Mix Problem with TimeWindows

2017

This paper presents a powerful new single-parameter metaheuristic to solve the Fleet Size and Mix Vehicle Routing Problem with Time Windows. The key idea of the new metaheuristic is to perform a random number of random-sized jumps in random order through four well-known local search operators. Computational testing on the 600 large-scale benchmarks of Bräysy et al. (Expert Syst Appl 36(4):8460–8475, 2009) show that the new metaheuristic outperforms previous best approaches, finding 533 new best-known solutions. Despite the significant number of random components, it is demonstrated that the variance of the results is rather low. Moreover, the suggested metaheuristic is shown to scale almost…

Mathematical optimizationComputer scienceSimple (abstract algebra)business.industryVehicle routing problemKey (cryptography)Scale (descriptive set theory)Local search (optimization)Variance (accounting)businessMetaheuristicParallel metaheuristic
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Spatial Besov regularity for stochastic partial differential equations on Lipschitz domains

2010

We use the scale of Besov spaces B^\alpha_{\tau,\tau}(O), \alpha>0, 1/\tau=\alpha/d+1/p, p fixed, to study the spatial regularity of the solutions of linear parabolic stochastic partial differential equations on bounded Lipschitz domains O\subset R^d. The Besov smoothness determines the order of convergence that can be achieved by nonlinear approximation schemes. The proofs are based on a combination of weighted Sobolev estimates and characterizations of Besov spaces by wavelet expansions.

Mathematics::Functional AnalysisSmoothness (probability theory)General MathematicsProbability (math.PR)Mathematics::Analysis of PDEsScale (descriptive set theory)Numerical Analysis (math.NA)Lipschitz continuitySobolev spaceStochastic partial differential equation60H15 Secondary: 46E35 65C30WaveletRate of convergenceBounded functionFOS: MathematicsApplied mathematicsMathematics - Numerical AnalysisMathematics - ProbabilityMathematicsStudia Mathematica
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Evolution of worldwide stock markets, correlation structure and correlation based graphs

2011

We investigate the daily correlation present among market indices of stock exchanges located all over the world in the time period Jan 1996 - Jul 2009. We discover that the correlation among market indices presents both a fast and a slow dynamics. The slow dynamics reflects the development and consolidation of globalization. The fast dynamics is associated with critical events that originate in a specific country or region of the world and rapidly affect the global system. We provide evidence that the short term timescale of correlation among market indices is less than 3 trading months (about 60 trading days). The average values of the non diagonal elements of the correlation matrix, corre…

NETWORK STRUCTUREPhysics - Physics and SocietyStatistical Finance (q-fin.ST)CROSS-CORRELATIONSCovariance matrixINDEXESFOS: Physical sciencesQuantitative Finance - Statistical FinanceScale (descriptive set theory)Physics and Society (physics.soc-ph)Mutual informationNOISEFOS: Economics and businessCorrelationMINIMUM SPANNING-TREESDYNAMIC ASSET TREESStock exchangeOrder (exchange)EconometricsEQUITY MARKETSMATRICESStock (geology)Eigenvalues and eigenvectorsMathematics
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Photon events with missing energy at root s=183 to 189 GeV

2000

The production of single photons has been studied in the reaction e+e- -> gamma + invisible particles at centre-of-mass energies of 183 GeV and 189 GeV. A previously published analysis of events with multi-photon final states accompanied by missing energy has been updated with 189 GeV data. The data were collected with the DELPHI detector and correspond to integrated luminosities of about 51 pb^{-1} and 158 pb^{-1} at the two energies. The number of light neutrino families is measured to be 2.84 +/- 0.15(stat) +/- 0.14(syst). The absence of an excess of events beyond that expected from Standard Model processes is used to set limits on new physics as described by supersymmetric and compos…

NEUTRALINOSParticle physicsDIMENSIONSPhotonPhysics and Astronomy (miscellaneous)Physics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaSTANDARD MODELFOS: Physical sciencesScale (descriptive set theory)7. Clean energy01 natural sciencesPartícules (Física nuclear)Standard ModelHigh Energy Physics - ExperimentGravitationHigh Energy Physics - Experiment (hep-ex)E(+)E(-) COLLISIONSSIGNALSSEARCH0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNuclear ExperimentEngineering (miscellaneous)DELPHIPhysicsMissing energy010308 nuclear & particles physicsSUPERLIGHT GRAVITINOLEPLARGE ELECTRON POSITRON COLLIDERSINGLE-PHOTONCOLLIDERSPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIPARTICLE PHYSICSProduction (computer science)Física nuclearHigh Energy Physics::ExperimentNeutrinoE(+)E(-) COLLISIONS; SUPERLIGHT GRAVITINO; STANDARD MODEL; SINGLE-PHOTON; COLLIDERS; SEARCH; LEP; NEUTRALINOS; DIMENSIONS; SIGNALSParticle Physics - Experiment
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A strategy to study the role of the charm quark in explaining the Delta{I}=1/2 rule

2004

We present a strategy designed to separate several possible origins of the well-known enhancement of the Delta{I}=1/2 amplitude in non-leptonic kaon decays. In particular, we seek to disentangle the contribution of physics at the typical QCD scale (soft-gluon exchange) from the effects at the scale of the charm quark mass. This is achieved by considering QCD with an unphysically light charm quark, so that the theory possesses an approximate SU(4)_L x SU(4)_R chiral symmetry. By computing the relevant operator matrix elements and monitoring their values as the charm quark mass departs from the SU(4)-symmetric situation, the role of the charm quark can be assessed. We study the influence of t…

Nuclear and High Energy PhysicsParticle physicsChiral perturbation theoryHigh Energy Physics::LatticeLattice (group)FOS: Physical sciencesScale (descriptive set theory)weak decaysCharm quarkHigh Energy Physics - Phenomenology (hep-ph)lattice QCDHigh Energy Physics - Latticefield theory gauge theory lattice kaon decayskaon physicschiral lagrangiansLimit (mathematics)Quantum chromodynamicsPhysicsHigh Energy Physics - Lattice (hep-lat)High Energy Physics::PhenomenologyFísicaFIS/02 - FISICA TEORICA MODELLI E METODI MATEMATICIHigh Energy Physics - PhenomenologyAmplitudeOperator matrixHigh Energy Physics::Experiment
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