Search results for "relativitat"

showing 10 items of 20 documents

Search for neutral Higgs bosons decaying into four taus at LEP2

2010

A search for the production and non-standard decay of a Higgs boson, h, into four taus through intermediate pseudoscalars, a, is conducted on 683 pb-1 of data collected by the ALEPH experiment at centre-of-mass energies from 183 to 209 GeV. No excess of events above background is observed, and exclusion limits are placed on the combined production cross section times branching ratio, β2 = σ(e+e -→Zh)/σSM(e+e-→Zh) ×B(h→aa)×B(a→τ+τ-) 2. For mh 1 is excluded at the 95% confidence level.

Nuclear and High Energy PhysicsParticle physicsTeoria quàntica de campsFOS: Physical sciences01 natural scienceshiggs bosonHigh Energy Physics - ExperimentALEPH Experimente+-e-ExperimentsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Collisions (Nuclear physics)Violació CP (Física nuclear)0103 physical sciencesCERN[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Teoria quàntica010306 general physicsALEPH experimentBosonPhysicse+-e- ExperimentsHiggs bosonsALEPH Experiment; CERN; higgs boson010308 nuclear & particles physicsBranching fractionSettore FIS/01 - Fisica SperimentaleSigmaRelativity (Physics)Relativitat (Física)e plus -e- ExperimentsQuantum field theoryHigh Energy Physics - PhenomenologyBosons de HiggsCol·lisions (Física nuclear)Quantum theoryHiggs bosonPhysique des particules élémentairesProduction (computer science)Particle Physics - ExperimentE+-e- ExperimentsCP violation (Nuclear physics)
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Creatable universes

2007

We consider the question of properly defining energy and momenta for non asymptotic Minkowskian spaces in general relativity. Only spaces of this type, whose energy, linear 3-momentum, and intrinsic angular momentum vanish, would be candidates for creatable universes, that is, for universes which could have arisen from a vacuum quantum fluctuation. Given a universe, we completely characterize the family of coordinate systems for which one could sensibly say that this universe is a creatable universe.

PhysicsNuclear and High Energy PhysicsAngular momentumCosmologiaGeneral relativitymedia_common.quotation_subjectCoordinate systemAstrophysics (astro-ph)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Type (model theory)AstrophysicsUniverseGeneral Relativity and Quantum CosmologyTheoretical physicsRelativitat general (Física)Quantum fluctuationmedia_common
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Precision measurement of D meson mass differences

2013

Using three- and four-body decays of D mesons produced in semileptonic b-hadron decays, precision measurements of D meson mass differences are made together with a measurement of the D-0 mass. The measurements are based on a dataset corresponding to an integrated luminosity of 1.0 fb(-1) collected in pp collisions at 7 TeV. Using the decay D-0 -> K+K-K-pi(+), the D-0 mass is measured to be M(D-0) = 1864.75 +/- 0.15 (stat) +/- 0.11 (syst) MeV/c(2). The mass differences M(D+) - M(D-0) = 4.76 +/- 0.12 (stat) +/- 0.07 (syst) MeV/c(2), M(D-s(+)) - M(D+) = 98.68 +/- 0.03 (stat) +/- 0.04 (syst) MeV/c(2) are measured using the D-0 -> K+K-pi(+)pi(-) and D-(s)(+) -> K+K-pi(+) modes.

Hadronic decays of charmed mesonsParticle physicsTeoria quàntica de campsGravitacióNuclear and High Energy PhysicsMesonHigh Energy Physics::LatticeNuclear TheoryFOS: Physical sciencesHadrons01 natural sciencesHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadrons; Leptonic semileptonic and radiative decays of bottom mesons; Charmed mesons (|C|>0 B=0); Hadronic decays of charmed mesonsPartícules (Física nuclear)Settore FIS/04 - Fisica Nucleare e SubnucleareLuminosityHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesD mesonLeptonic semileptonic and radiative decays of bottom meson[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]TOOLTeoria quàntica010306 general physicsHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadronsNuclear ExperimentQCHadron-Hadron Scattering; Nuclear and High Energy PhysicsPhysicsHadron-Hadron Scattering010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadronRelativity (Physics)DecayRelativitat (Física)Quantum field theoryFIS/01 - FISICA SPERIMENTALEQuantum theoryLeptonic semileptonic and radiative decays of bottom mesonsDECAY; TOOLFísica nuclearHigh Energy Physics::ExperimentCharmed mesons (|C|>0 B=0)DECAYParticle Physics - ExperimentGravitationJournal of High Energy Physics
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Implicaciones de la evolución histórica de algunos conceptos en la enseñanza de la Relatividad

2006

La relatividad es una parte importante de la fisica moderna. En este articulo se analiza el debate en torno a la utilizacion de la historia de la ciencia para orientar la didactica de la relatividad en la ensenanza secundaria. Se repasa la evolucion historica de algunos conceptos clave de la relatividad especial y se muestra su implicacion en la ensenanza-aprendizaje.Palabras clave: ensenanza-aprendizaje; relatividad; historia de la ciencia.Implications of the historical evolution of some concepts in the teaching of relativityThe relativity is an important part the modern physics. In this article we analyze the discussion around the use of the history of science to guide the didactics of th…

Històriahistoria de la cienciaSecondary educationPhilosophyrelatividadaprendizajeSocial SciencesModern physicsRelativitat (Física)enseñanzaSpecial relativity (alternative formulations)Educationlcsh:Social Scienceslcsh:HHTheory of relativityenseñanza-aprendizajeAprenentatgeHumanitiesHistory of scienceEnsenyament
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Two-Perfect Fluid Interpretation of an Energy Tensor

1990

The paper contains the necessary and sufficient conditions for a given energy tensor to be interpreted as a sum of two perfect fluids. Given a tensor of this class, the decomposition in two perfect fluids (which is determined up to a couple of real functions) is obtained.

Weyl tensorPhysicsTensor contractionFluidsPhysics and Astronomy (miscellaneous)Geometria diferencialMathematical analysisTensor fieldPhysics::Fluid Dynamicssymbols.namesakeExact solutions in general relativityRelativitat general (Física)symbolsSymmetric tensorStress–energy tensorTensorTensor density
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On the uniqueness of the space-time energy in General Relativity. The illuminating case of the Schwarzschild metric

2013

The case of asymptotic Minkowskian space-times is considered. A special class of asymptotic rectilinear coordinates at the spatial infinity, related to a specific system of free falling observers, is chosen. This choice is applied in particular to the Schwarzschild metric, obtaining a vanishing energy for this space-time. This result is compared with the result of some known theorems on the uniqueness of the energy of any asymptotic Minkowskian space, showing that there is no contradiction between both results, the differences becoming from the use of coordinates with different operational meanings. The suitability of Gauss coordinates when defining an {\em intrinsic} energy is considered a…

PhysicsGravitacióPhysics and Astronomy (miscellaneous)General relativitySpace timemedia_common.quotation_subjectGaussFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)InfinitySpace (mathematics)General Relativity and Quantum CosmologyRelativitat general (Física)Schwarzschild metricUniquenessEnergy (signal processing)media_commonMathematical physics
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Method to obtain shear-free two-fluid solutions of Einstein's equations.

1989

We use the Einstein equations, stated as an initial-value problem (3+1 formalism), to present a method for obtaining a class of solutions which may be interpreted as the gravitational field produced by a mixture of two perfect fluids. The four-velocity of one of the components is assumed to be a shear-free, irrotational, and geodesic vector field. The solutions are given up to a set of a hyperbolic quasilinear system.

PhysicsGravitacióGeodesicPerfect fluidConservative vector fieldRelativitat (Física)symbols.namesakeGravitational fieldEinstein field equationssymbolsVector fieldEinsteinRicci curvatureMathematical physicsPhysical review. D, Particles and fields
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Cosmic censorship conjecture in some matching spherical collapsing metrics

2017

A physically plausible Lema{\^{\i}}tre-Tolman-Bondi collapse in the marginally bound case is considered. By "physically plausible" we mean that the corresponding metric is ${\cal C}^1$ matched at the collapsing star surface and further that its {\em intrinsic} energy is, as due, stationary and finite. It is proved for this Lema{\^{\i}}tre-Tolman-Bondi collapse, for some parameter values, that its intrinsic central singularity is globally naked, thus violating the cosmic censorship conjecture with, for each direction, one photon, or perhaps a pencil of photons, leaving the singularity and reaching the null infinity. Our result is discussed in relation to some other cases in the current liter…

PhysicsGravitacióConjecture010308 nuclear & particles physicsStar (game theory)media_common.quotation_subjectCosmic censorship hypothesisNull (mathematics)Collapse (topology)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsInfinity01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologySingularityRelativitat general (Física)0103 physical sciencesGravitational singularity010306 general physicsMathematical physicsmedia_common
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Solutions of the Einstein field equations for a bounded and finite discontinuous source, and its generalization: Metric matching conditions and jumpi…

2019

We consider the metrics of the General Relativity, whose energy-momentum tensor has a bounded support where it is continuous except for a finite step across the corresponding boundary surface. As a consequence, the first derivative of the metric across this boundary could perhaps present a finite step too. However, we can assume that the metric is ${\cal C}^1$ class everywhere. In such a case, although the partial second derivatives of the metric exhibit finite (no Dirac $\delta$ functions) discontinuities, the Dirac $\delta$ functions will still appear in the conservation equation of the energy-momentum tensor. As a consequence, strictly speaking, the corresponding metric solutions of the …

AstrofísicaSolutions of the Einstein field equationsPhysicsGravitacióConservation lawPure mathematics010308 nuclear & particles physicsGeneral relativityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationRelativitat general (Física)Bounded function0103 physical sciencesEinstein field equationsPartial derivative010306 general physicsSecond derivativePhysical Review D
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Students' Understanding of the Special Theory of Relativity and Design for a Guided Visit to a Science Museum

2009

International audience; This paper describes the design of teaching materials that are used as learning tools in school visits to a science museum. An exhibition on the A century of the Special Theory of Relativity, in the Kutxaespacio Science Museum, in San Sebastian (Spain), was used to design a visit for first year engineering students at the university and assess the learning which was achieved. The first part of the paper presents the teaching sequence which was designed to build a bridge between formal teaching and the exhibition visit. The second part analyses the potential of the exhibition and the aforementioned teaching sequence to influence the students' knowledge of three aspect…

Science instructionMuseus de ciències4. EducationTeaching method05 social sciencesStudents understanding050301 educationRelativitat (Física)01 natural sciencesCiència EnsenyamentEducationExhibitionddc:370Engineering education0103 physical sciencesPedagogyMathematics educationComputingMilieux_COMPUTERSANDEDUCATIONCurriculum Teaching DidacticsSociologySocial Sciences & HumanitiesUnterricht Didaktik010306 general physicsBildung und Erziehung0503 education
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