Search results for "astronomía"

showing 10 items of 247 documents

Search for decays of stopped, long-lived particles from 7 TeV pp collisions with the ATLAS detector

2012

New metastable massive particles with electric and colour charge are features of many theories beyond the Standard Model. A search is performed for long-lived gluino-based R-hadrons with the ATLAS detector at the LHC using a data sample corresponding to an integrated luminosity of 31 pb[superscript −1]. We search for evidence of particles that have come to rest in the ATLAS detector and decay at some later time during the periods in the LHC bunch structure without proton–proton collisions. No significant deviations from the expected backgrounds are observed, and a cross-section limit is set. It can be interpreted as excluding gluino-based R-hadrons with masses less than 341 GeV at the 95 % …

Physics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsPhysics beyond the Standard ModelCiencias Físicas01 natural sciencesLong lived particlesLuminosityHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)R-hadronspp collisions; ATLAS detector[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentDetectors de radiacióPhysicsGluinoLarge Hadron ColliderSplit supersymmetrySettore FIS/01 - Fisica SperimentaleATLASmedicine.anatomical_structurePhysical SciencesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearLHCParticle Physics - ExperimentCIENCIAS NATURALES Y EXACTASParticle physicsFOS: Physical sciencesddc:500.2530Partícules (Física nuclear)Nuclear physicsAtlas (anatomy)0103 physical sciencesCollidersmedicineFysikddc:530High Energy Physics010306 general physicsEngineering (miscellaneous)Split Supersymmetry010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyNEW PHYSICS//purl.org/becyt/ford/1.3 [https]AstronomíaR-hadronHADRON-HADRON COLLISIONSCol·lisions (Física nuclear)Experimental High Energy PhysicsNeutralinoHigh Energy Physics::Experiment
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Ab initio quantum-chemical computations of the electronic states in HgBr2 and IBr: Molecules of interest on the Earth’s atmosphere

2016

The electronic states of atmospheric relevant molecules IBr and HgBr are reported, within the UV-Vis spectrum range (170nm≤λphoton≤600 nm) by means of the complete-active-space self-consistent field/multi-state complete-active-space second-order perturbation theory/spin-orbit restricted-active-space state-interaction (CASSCF/MS-CASPT2/SO-RASSI) quantum-chemical approach and atomic-natural-orbital relativistic-correlation-consistent (ANO-RCC) basis sets. Several analyses of the methodology were carried out in order to reach converged results and therefore to establish a highly accurate level of theory. Good agreement is found with the experimental data with errors not higher than around 0.1 …

Physics010504 meteorology & atmospheric sciencesField (physics)Ciencias FísicasAb initioGeneral Physics and Astronomy//purl.org/becyt/ford/1.3 [https]-010402 general chemistry01 natural sciences0104 chemical sciences//purl.org/becyt/ford/1 [https]AstronomíaAb initio quantum chemistry methodsQuantum mechanicsAtmospheric chemistryMoleculePhysical and Theoretical ChemistryPerturbation theoryAtomic physicsSpin (physics)CIENCIAS NATURALES Y EXACTAS0105 earth and related environmental sciencesInterhalogen
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Does GRS 1915+105 exhibit "canonical" black-hole states?

2003

We have analysed RXTE data of the superluminal source GRS 1915+105 in order to investigate if, despite its extreme variability, it also exhibits the canonical source states that characterise other black-hole candidates. The phenomenology of GRS 1915+105 has been described in terms of three states (named A, B and C) based on their hardness ratios and position in the colour-colour diagram. We have investigated the connection between these states and the canonical behaviour and found that the shape of the power spectral continuum and the values of the best-fit model parameters to the noise components in all three states indicate that the source shows properties similar to the canonical very hi…

PhysicsAccretionSuperluminal motionContinuum (measurement)Astrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)BinariesFOS: Physical sciencesAstronomy and AstrophysicsModel parametersAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Individual StarsSpace and Planetary ScienceX-raysGRS 1915+105UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaAccretion discIndividual Stars ; GRS 1915+105 ; Binaries ; X-rays ; Accretion ; Accretion disc:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Hβ photometry for UVBY standard stars

1988

From 1984 to 1986 the authors made several observational campaigns at Calar Alto and La Palma Observatories using the uvby and β photometric systems to monitor a selected sample of late-type variable stars. In this paper they present the β values for 38 uvby standard stars to contribute to the uvby-β calibration works on late-type stars. In the final discussion, the β computed values are plotted against the Stroemgren b-y, m_(1), and c_(1) indices.

PhysicsAstrofísicaAstronomíaStarsPhotometry (astronomy)Space and Planetary ScienceAstronomy and AstrophysicsBeta (velocity)AstrophysicsVariable star
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Quantifying the contamination by old main-sequence stars in young moving groups: the case of the Local Association

2009

The associations and moving groups of young stars are excellent laboratories for investigating stellar formation in the solar neighborhood. Previous results have confirmed that a non-negligible fraction of old main-sequence stars is present in the lists of possible members of young stellar kinematic groups. A detailed study of the properties of these samples is needed to separate the young stars from old main-sequence stars with similar space motion, and identify the origin of these structures. We used stars possible members of the young (~ 10 - 650 Myr) moving groups from the literature. To determine the age of the stars, we used several suitable age indicators for young main sequence star…

PhysicsAstrofísicaLocal associationStar formationFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstronomíaStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsEquivalent widthSolar and Stellar Astrophysics (astro-ph.SR)Main sequenceAstrophysics::Galaxy AstrophysicsLine (formation)
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Numerical evidence of hyperscaling violation in wetting transitions of the random-bond Ising model in d = 2 dimensions

2017

We performed extensive simulations of the random-bond Ising model confined between walls where competitive surface fields act. By properly taking the thermodynamic limit we unambiguously determined wetting transition points of the system, as extrapolation of localization-delocalization transitions of the interface between domains of different orientation driven by the respective fields. The finite-size scaling theory for wetting with short-range fields establishes that the average magnetization of the sample, with critical exponent β, is the proper order parameter for the study of wetting. While the hyperscaling relationship given by γ+2β=ν +ν requires β=1/2 (γ=4, ν =3, and ν =2), the therm…

PhysicsCiencias AstronómicasCondensed matter physicsCiencias FísicasHYPERSCALINGTransitionsOrder (ring theory)WettingTRANSITIONSHyperscaling//purl.org/becyt/ford/1.3 [https]Orientation (vector space)Astronomía//purl.org/becyt/ford/1 [https]MagnetizationWetting transitionThermodynamic limitExponentIsing modelCritical exponentCIENCIAS NATURALES Y EXACTASWETTING
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Role of dispersion on zero-average-index bandgaps

2009

We consider periodic multilayers combining ordinary positive index materials and dispersive metamaterials with negative index in some frequency ranges. These structures can exhibit photonic bandgaps which, in contrast with the usual Bragg gaps, are not based on interference mechanisms. Changing the dispersion models for the constituent metamaterial, we investigate its role in the production of zero-average-index bandgaps. In particular, we show the effect of each constitutive parameter on both bandgap edges. Finally, we give some approximated analytical expressions in terms of average parameters for the determination of the upper and lower limits of the zero-average refractive-index bandgap…

PhysicsCondensed matter physicsbusiness.industryWave propagationBand gapCiencias FísicasPHOTONIC CRYSTALSPhysics::OpticsMetamaterialStatistical and Nonlinear PhysicsInterference (wave propagation)Atomic and Molecular Physics and OpticsNEGATIVE INDEXAstronomíaCondensed Matter::Materials ScienceOpticsPHOTONIC BAND GAPNegative refractionDispersion (optics)MULTILAYERSPhotonicsbusinessRefractive indexCIENCIAS NATURALES Y EXACTAS
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Coherence loss in phase-referenced VLBI observations

2010

Context. Phase-referencing is a standard calibration technique in radio interferometry, particularly suited for the detection of weak sources close to the sensitivity limits of the interferometers. However, effects from a changing atmosphere and inaccuracies in the correlator model may affect the phase-referenced images, and lead to wrong estimates of source flux densities and positions. A systematic observational study of signal decoherence in phase-referencing and its effects in the image plane has not been performed yet. Aims. We systematically studied how the signal coherence in Very-Long-Baseline-Interferometry (VLBI) observations is affected by a phase-reference calibration at differe…

PhysicsDynamic rangePhase (waves)Astrophysics::Instrumentation and Methods for AstrophysicsFluxAstronomy and AstrophysicsContext (language use)interferometers [Instrumentation]AstrophysicsAtmospheric effectsComputational physicsTechniques : interferometric; Atmospheric effects; Instrumentation : interferometersInterferometrySpace and Planetary ScienceVery-long-baseline interferometrySource separationinterferometric [Techniques]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicas:ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicas [UNESCO]Coherence (physics)
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m-bonacci metamaterial multilayers: location of the zero-average index bandgap edges

2009

We examine quasiperiodic multilayers arranged in m-bonacci sequences, which combine ordinary positiveindex materials and dispersive metamaterials with negative index in a certain frequency range. When the volume-averaged refractive index of the nonperiodic multilayer equals zero, the structure does not propagate light radiation and exhibits a forbidden band. We identify some analytical expressions to determine the upper and lower limits of the above zero-average refractive-index bandgap. We recognize that these limits are not explicitly dependent on the geometrical parameters of the stack of layers. © 2009 Optical Society of America. Fil: Monsoriu, J.A.. Universidad Politécnica de Valencia;…

PhysicsFibonacci numberbusiness.industryBand gapCiencias FísicasPHOTONIC CRYSTALSPhysics::OpticsMetamaterialFIBONACCIAtomic and Molecular Physics and OpticsNEGATIVE INDEXAstronomíaOpticsStack (abstract data type)METAMATERIALSQuasiperiodic functionReflection coefficientbusinessRefractive indexCIENCIAS NATURALES Y EXACTASPhotonic crystal
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Point field models for the galaxy point pattern modelling the singularity of the two-point correlation function

2002

There is empirical evidence that the two-point correlation function of the galaxy distribution follows, for small scales, reasonably well a power-law expression $\xi(r)\propto r^{-\gamma}$ with $\gamma$ between 1.5 and 1.9. Nevertheless, most of the point field models suggested in the literature do not have this property. This paper presents a new class of models, which is produced by modifying point fields commonly used in cosmology to mimic the galaxy distribution, but where $\gamma=2$ is too large. The points are independently and randomly shifted, leading to the desired reduction of the value of $\gamma$.

PhysicsGalaxy statistics ; Large-scale structure of universe ; Statistical methodField (physics)Distribution (number theory)Astrophysics (astro-ph)FOS: Physical sciencesLarge-scale structure of universeAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxy statisticsExpression (computer science)UNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]CosmologyGalaxySingularityCorrelation functionSpace and Planetary SciencePoint (geometry)Statistical physicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaStatistical method:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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