Search results for "ICAD"

showing 10 items of 1297 documents

On the p-length of some finite p-soluble groups

2014

The main aim of this paper is to give structural information of a finite group of minimal order belonging to a subgroup-closed class of finite groups and whose $p$-length is greater than $1$, $p$ a prime number. Alternative proofs and improvements of recent results about the influence of minimal $p$-subgroups on the $p$-nilpotence and $p$-length of a finite group arise as consequences of our study

Normal subgroupSemidirect productFinite groupPure mathematicsClass (set theory)Direct summandGeneral MathematicsPrime numberGrups Teoria deMaximal subgroupMaximal subgroupNormal subgroupApplications of MathematicsTheoretical Mathematical and Computational PhysicsSemidirect productOrder (group theory)ÀlgebraAlgebra over a fieldFinite groupMATEMATICA APLICADAMathematics
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SEARCHES FOR POINT-LIKE AND EXTENDED NEUTRINO SOURCES CLOSE TO THE GALACTIC CENTER USING THE ANTARES NEUTRINO TELESCOPE

2014

A search for cosmic neutrino sources using six years of data collected by the ANTARES neutrino telescope has been performed. Clusters of muon neutrinos over the expected atmospheric background have been looked for. No clear signal has been found. The most signal-like accumulation of events is located at equatorial coordinates R.A. = -46º.8 and decl. = -64º.9 and corresponds to a 2.2 sigma background fluctuation. In addition, upper limits on the flux normalization of an E-2 muon neutrino energy spectrum have been set for 50 pre-selected astrophysical objects. Finally, motivated by an accumulation of seven events relatively close to the Galactic Center in the recently reported neutrino sample…

Normalization (statistics)AstrofísicaParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicslaw.inventionHigh Energy Physics - ExperimentTelescopeHigh Energy Physics - Experiment (hep-ex)neutrinolaw[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Point (geometry)Muon neutrinoNeutrinsNeutrinosInstrumentation and Methods for Astrophysics (astro-ph.IM)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuonCOSMIC cancer databaseGalaxy: center[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]astroparticle physicFísicaneutrinosAstronomy and Astrophysicscenter [Galaxy]Galaxy centerNeutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]13. Climate actionSpace and Planetary Scienceastroparticle physicsFISICA APLICADA:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]High Energy Physics::ExperimentNeutrinoAstroparticle physicsMATEMATICA APLICADAAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysicsastroparticle physics; Galaxy: center; neutrinos
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Measurement of atmospheric neutrino oscillations with the ANTARES neutrino telescope

2012

The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of atmospheric neutrinos are extracted by fitting the event rate as a function of the ratio of the estimated neutrino energy and reconstructed flight path through the Earth. Measurement contours of the oscillation parameters in a two-flavour approximation are derived. Assuming maximal mixing, a mass …

Nuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2Neutrino telescope01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Experiment0103 physical sciencesNeutrinsHigh Energy PhysicsNeutrinos010306 general physicsNeutrino oscillationPhysicsMuonANTARES:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsNeutrino oscillations[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologySolar neutrino problemNeutrino astrophysicsCosmic neutrino backgroundNeutrino detectorFISICA APLICADAMeasurements of neutrino speedFísica nuclearHigh Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Physics Letters B
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A search for time dependent neutrino emission from microquasars with the ANTARES telescope

2014

[EN] Results are presented on a search for neutrino emission from a sample of six microquasars, based on the data collected by the ANTARES neutrino telescope between 2007 and 2010. By means of appropriate time cuts, the neutrino search has been restricted to the periods when the acceleration of relativistic jets was taking place at the microquasars under study. The time cuts have been chosen using the information from the X-ray telescopes RXTE/ASM and Swift/BAT, and, in one case, the gamma-ray telescope Fermi/LAT. No statistically significant excess has been observed, thus upper limits on the neutrino fluences have been derived and compared to the predictions by models. Constraints have bee…

Nuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyLuminositylaw.inventionTelescopeneutrinoAstrophysical jetlawMicroquasars0103 physical sciencesmicroquasarNeutrinos010303 astronomy & astrophysicsAstroparticle physicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyFísicaAstronomy and AstrophysicsSolar neutrino problemNeutrino detectorSpace and Planetary ScienceFISICA APLICADANuclear and High Energy Physics; Astronomy and Astrophysics; Space and Planetary ScienceHigh Energy Physics::ExperimentNeutrinoAstroparticle physicsAstrophysics - High Energy Astrophysical PhenomenaANTARES neutrino telescopeFermi Gamma-ray Space Telescope
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Enantioselective Synthesis of 4-Substituted Dihydrocoumarins through a Zinc Bis(hydroxyamide)-Catalyzed Conjugate Addition of Terminal Alkynes

2013

A new enantioselective catalyst for the conjugate addition of terminal alkynes has been developed. Terminal alkynes react with 3-alkoxycarbonylcoumarins in the presence of diethylzinc and bis(hydroxyamide) ligands to give chiral non-racemic dihydrocoumarins substituted with an alkynyl group on the C-4 position with good yields and enantiomeric excesses up to 95%.

Nucleophilic additionChemistryStereochemistryN O ligandsEnantioselective synthesischemistry.chemical_elementAlkynylationGeneral ChemistryZincCatalysisOxygen heterocyclesAlkynylationFISICA APLICADAAsymmetric catalysismedia_common.cataloged_instanceEuropean unionNucleophilic additionmedia_commonConjugateAdvanced Synthesis & Catalysis
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Matrices A such that A^{s+1}R = RA* with R^k = I

2018

[EN] We study matrices A is an element of C-n x n such that A(s+1)R = RA* where R-k = I-n, and s, k are nonnegative integers with k >= 2; such matrices are called {R, s+1, k, *}-potent matrices. The s = 0 case corresponds to matrices such that A = RA* R-1 with R-k = I-n, and is studied using spectral properties of the matrix R. For s >= 1, various characterizations of the class of {R, s + 1, k, *}-potent matrices and relationships between these matrices and other classes of matrices are presented. (C) 2018 Elsevier Inc. All rights reserved.

Numerical AnalysisClass (set theory)Algebra and Number TheorySpectral properties0211 other engineering and technologies021107 urban & regional planning010103 numerical & computational mathematics02 engineering and technologyMatrius (Matemàtica)01 natural sciencesCombinatoricsMatrix (mathematics)Discrete Mathematics and CombinatoricsGeometry and Topology0101 mathematicsÀlgebra linealMATEMATICA APLICADA{R s+1 k *}-potent matrixK-involutoryMathematics
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Constructing adaptive generalized polynomial chaos method to measure the uncertainty in continuous models: A computational approach

2015

Due to errors in measurements and inherent variability in the quantities of interest, models based on random differential equations give more realistic results than their deterministic counterpart. The generalized polynomial chaos (gPC) is a powerful technique used to approximate the solution of these equations when the random inputs follow standard probability distributions. But in many cases these random inputs do not have a standard probability distribution. In this paper, we present a step-by-step constructive methodology to implement directly a useful version of adaptive gPC for arbitrary distributions, extending the applicability of the gPC. The paper mainly focuses on the computation…

Numerical AnalysisMathematical optimizationPolynomial chaosGeneral Computer ScienceDifferential equationApplied MathematicsComputingConstructiveMeasure (mathematics)Theoretical Computer ScienceCHAOS (operating system)Generalized polynomialRandom differential equationsModeling and SimulationConvergence (routing)Applied mathematicsProbability distributionMATEMATICA APLICADAAdaptive polynomial chaosMathematics
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Argullol a vueltas con la opinión pública

2007

OPINIÓN PÚBLICAVidal-Beneyto JoséEspacio públicodictaduraOpiniónTertuliasEl PaísHabermasRAFAEL ARGULLOLDescalificaciónPeriodistasImpugnaciónDiversidad opinativaEmpresariosArgullolOpinión publicadaOpinión de los públicosSondeosMario Vargas LlosaEditorialPiedra de toqueTribunaPolíticosSociedad mediática de masaObstinaciónSindicatosNotoriedadPublicaciones: Obra periodística: Cartas al director
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Concatenated logic functions using nanofluidic diodes with all-electrical inputs and outputs

2018

[EN] Nanopore-based logical schemes in ionic solutions typically involve single gates and chemical inputs. The design of computer-like functions requires the consecutive concatenation of several gates and the use of electrical potentials and currents to facilitate the downstream transfer of electrochemical information. We have demonstrated the robust operation of concatenated logic functions using biomimetic nanofluidic diodes based on single pore membranes. To this end, we have implemented first the logic functions AND and OR with combinations of single nanopores using all-electrical input and output signals. The concatenation of these gates allows the output of the OR gate to act as one o…

OR gateComputer scienceConcatenation02 engineering and technologySignal transduction010402 general chemistry01 natural sciencesSignallaw.inventionlcsh:ChemistrylawElectrochemistryElectronic engineeringHardware_ARITHMETICANDLOGICSTRUCTURESElectronic circuitTransistor021001 nanoscience & nanotechnology0104 chemical sciencesNanofluidic diodelcsh:Industrial electrochemistrylcsh:QD1-999FISICA APLICADAElectrochemical logic functionsInverter0210 nano-technologyAND gatelcsh:TP250-261Hardware_LOGICDESIGNNOR gateElectrochemistry Communications
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Optimization of a decellularized protocol of porcine tracheas. Long-term effects of cryopreservation. A histological study

2021

[EN] Objective: The aim of this study was to optimize a decellularization protocol in the trachea of Sus scrofa domestica (pig) as well as to study the effects of long-term cryopreservation on the extracellular matrix of decellularized tracheas. Methods: Porcine tracheas were decellularized using Triton X-100, SDC, and SDS alone or in combination. The effect of these detergents on the extracellular matrix characteristics of decellularized porcine tracheas was evaluated at the histological, biomechanical, and biocompatibility level. Morphometric approaches were used to estimate the effect of detergents on the collagen and elastic fibers content as well as on the removal of chondrocytes from …

OctoxynolSwine0206 medical engineeringTracheal stenosisBiomedical EngineeringMedicine (miscellaneous)Bioengineering02 engineering and technologyCryopreservationBiomaterialsAndrology03 medical and health sciences0302 clinical medicineMedicineSDSCryopreservationDecellularizationTissue EngineeringTissue Scaffoldsbusiness.industryTracheal histologyDecellularized tracheasAirway tissue engineeringGeneral Medicine020601 biomedical engineeringTracheal StenosisSus scrofa domesticaExtracellular MatrixTrachea030220 oncology & carcinogenesisFISICA APLICADAbusiness
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