Search results for "astronomía"

showing 10 items of 247 documents

Space-like (vs. time-like) collinear limits in QCD: Is factorization violated?

2012

We consider the singular behaviour of QCD scattering amplitudes in kinematical configurations where two or more momenta of the external partons become collinear. At the tree level, this behaviour is known to be controlled by factorization formulae in which the singular collinear factor is universal (process independent). We show that this strict (process-independent) factorization is not valid at one-loop and higher-loop orders in the case of the collinear limit in space-like regions (e.g., collinear radiation from initial-state partons). We introduce a generalized version of all-order collinear factorization, in which the space-like singular factors retain some dependence on the momentum a…

High Energy Physics - TheoryNLO COMPUTATIONSNuclear and High Energy PhysicsHADRONIC COLLIDERSCiencias FísicasFOS: Physical sciencesPartonSpace (mathematics)01 natural sciences//purl.org/becyt/ford/1 [https]MomentumHigh Energy Physics - Phenomenology (hep-ph)Factorization0103 physical sciences010306 general physicsMathematical physicsQuantum chromodynamicsPhysics010308 nuclear & particles physicsFísicaCharge (physics)//purl.org/becyt/ford/1.3 [https]Scattering amplitudeAstronomíaHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Gravitational singularityCIENCIAS NATURALES Y EXACTAS
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Double collinear splitting amplitudes at next-to-leading order

2013

We compute the next-to-leading order (NLO) QCD corrections to the $1 \to 2$ splitting amplitudes in different dimensional regularization (DREG) schemes. Besides recovering previously known results, we explore new DREG schemes and analyze their consistency by comparing the divergent structure with the expected behavior predicted by Catani's formula. Through the introduction of scalar-gluons, we show the relation among splittings matrices computed using different schemes. Also, we extended this analysis to cover the double collinear limit of scattering amplitudes in the context of QCD+QED.

High Energy Physics - TheoryNLO COMPUTATIONSNuclear and High Energy PhysicsParticle physicsHADRONIC COLLIDERSCiencias FísicasFOS: Physical sciencesContext (language use)01 natural sciences//purl.org/becyt/ford/1 [https]Dimensional regularizationHigh Energy Physics - Phenomenology (hep-ph)Consistency (statistics)0103 physical sciencesLimit (mathematics)010306 general physicsMathematical physicsQuantum chromodynamicsPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísica//purl.org/becyt/ford/1.3 [https]Scattering amplitudeAstronomíaHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics - Theory (hep-th)Cover (topology)CIENCIAS NATURALES Y EXACTASJournal of High Energy Physics
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Triple collinear splitting functions at NLO for scattering processes with photons

2014

We present splitting functions in the triple collinear limit at next-to-leading order. The computation was performed in the context of massless QCD+QED, considering only processes which include at least one photon. Through the comparison of the IR divergent structure of splitting amplitudes with the expected known behavior, we were able to check our results. Besides that we implemented some consistency checks based on symmetry arguments and cross-checked the results among them. Studying photon-started processes, we obtained very compact results.

High Energy Physics - TheoryNLO COMPUTATIONSNuclear and High Energy PhysicsParticle physicsPhotonCiencias FísicasComputationFOS: Physical sciencesContext (language use)01 natural sciences//purl.org/becyt/ford/1 [https]High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsQuantum chromodynamicsPhysics010308 nuclear & particles physicsScatteringFísica//purl.org/becyt/ford/1.3 [https]Symmetry (physics)AstronomíaMassless particleHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics - Theory (hep-th)CIENCIAS NATURALES Y EXACTASJournal of High Energy Physics
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Aportaciones al cálculo de la latitud en la náutica española de principios del siglo XVII contenidas en el manuscrito de Diego Ramírez de Arellano &l…

2013

In 1620, was named chief pilot of the Casa de Contratación de Sevilla Diego Ramírez de Arellano, author of a manuscript entitled Reconocimiento de los estrechos de Magallanes y San Vicente, con algunas cosas curiosas de navegación. He had participated in the reconnaissance mission referred by the title of the manuscript, and in that book developed same methods and tools for a nautical understood scientifically, and even used a methodology close to modern science, as in refuting the theory about Figueiredo of the linear relationship between longitude and magnetic variation of the needle navigation. This article is based on some conclusions that can get an analysis of the manuscript. It focus…

Historia de las matemáticasHistoria de la astronomíamedia_common.quotation_subjectArtHistory of AstronomyHistory of CartographyHistory of MathematicsHistoria de la náuticaLinear relationshipSpanish Science in 16th CenturyHistory and Philosophy of ScienceMonarchyAZ20-999Historia de la cartografíaHistory of scholarship and learning. The humanitiesNautical historyCiencia española del s. XVIHistory of medicine. Medical expeditionsHumanitiesR131-687media_commonAsclepio
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Alimentación y salud en la Valencia medieval. Teorías y prácticas

2013

The aim of this article is to provide an initial survey about the relationship between food habits and health in a Mediterranean city during the Late Middle Ages, by comparing medical treatises, gastronomic recipes and the archival sources that tell us about the actual expenses in food. Through this comparison, and by using accounting records of aristocratic houses, merchant enterprises, convents and hospitals, we can observe the dietary guidelines that were applied, and their concordance with the galenic principles of University medicine. Moreover, we attempt to assess what were the key factors in the evolution of these theories’ guidelines, and how they were probably rather a way to appro…

HistorymedicineHistoryConcordancelcsh:D111-203lcsh:Medieval historyFood habitsD111-203Social behaviourCrown of Aragon13th-15th centuriesAccounting recordsconsumoMedieval historyMiddle AgesconsumptionfoodgastronomyregiminahealthrecipesCorona de AragónrecetariosKey factorsalimentaciónsaludEthnologygastronomíaValenciasiglos XIII-XVmedicinaDemographyAnuario de Estudios Medievales
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Long-term X-ray variability of the microquasar system LS 5039/RX J1826.2−1450

2003

We report on the results of the spectral and timing analysis of a BeppoSAX observation of the microquasar system LS 5039/RX J1826.2-1450. The source was found in a low-flux state with Fx(1-10 keV)= 4.7 x 10^{-12} erg cm^{-2} s^{-1}, which represents almost one order of magnitude lower than a previous RXTE observation 2.5 years before. The 0.1--10 keV spectrum is described by an absorbed power-law continuum with photon-number spectral index Gamma=1.8+-0.2 and hydrogen column density of NH=1.0^{+0.4}_{-0.3} x 10^{22} cm^{-2}. According to the orbital parameters of the system the BeppoSAX observation covers the time of an X-ray eclipse should one occur. However, the 1.6-10 keV light curve does…

HydrogenVariable starschemistry.chemical_elementFOS: Physical sciencesAstrophysicsCompact starAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAccretion rateRadio astronomyQuasarsQuàsarsEstels binaris de raigs XOrbital elementsPhysicsSpectral indexRX J1826.2−1450Astrophysics (astro-ph)X-rayIndividual Star ; LS 5039 ; RX J1826.2−1450 ; 3EG J1824−1514 – X-rays ; Variable stars ;; General–radio continuumAstronomy and AstrophysicsIndividual StarLight curveGeneral–radio continuum:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]StarsEstelsX-ray binarieschemistrySpace and Planetary ScienceRadioastronomiaLS 50393EG J1824−1514 – X-raysUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaOrder of magnitude:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Cycles of time in the Iberian culture: the astronomical orientation of the temple of El Tossal de Sant Miquel de Llíria

2006

We present an archaeoastronomical study of the temple of the Iberian settlement of El Tossal de Sant Miquel de Llíria (València). We find that the major axis of the building is oriented very close to the east-west cardinal axis. The entrance of the temple is pointing towards an outstanding mountain on the eastern horizon, where the sunrise around the equinoxes takes place. On the other hand, the absence of other constructions just in front of the cultic building seems to support the inference that the astronomical relation was intentional, because it would permit the observation of the sunrise from the temple. The existence of other nearby Iberian sanctuaries showing similar relations with …

Iberian CultureArqueoastronomíaArcheologySantuariosmedia_common.quotation_subjectArtSacred placesReligionArchaeoastronomylcsh:ArchaeologyCultura ibéricalcsh:CC1-960ReligiónHumanitiesmedia_commonTrabajos de Prehistoria
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Cycles of time in the Iberian culture: the astronomical orientation of the temple of El Tossal de Sant Miquel de Llíria

2006

We present an archaeoastronomical study of the temple of the Iberian settlement of El Tossal de Sant Miquel de Llíria (València). We find that the major axis of the building is oriented very close to the east-west cardinal axis. The entrance of the temple is pointing towards an outstanding mountain on the eastern horizon, where the sunrise around the equinoxes takes place. On the other hand, the absence of other constructions just in front of the cultic building seems to support the inference that the astronomical relation was intentional, because it would permit the observation of the sunrise from the temple. The existence of other nearby Iberian sanctuaries showing similar relations with …

Iberian CultureArqueoastronomíaUNESCO::HISTORIA::Otras especialidades históricasSantuarios:HISTORIA::Historia por épocas::Prehistoria [UNESCO]Sacred placesReligionArchaeologyArqueoastronomía; Cultura ibérica; Religión; SantuariosUNESCO::HISTORIA::Historia por épocas::PrehistoriaArchaeoastronomyCultura ibérica:HISTORIA::Otras especialidades históricas [UNESCO]ReligiónCC1-960
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In-situ high-pressure x-ray diffraction study of zinc ferrite nanoparticles

2016

We have studied the high-pressure structural behavior of zinc ferrite (ZnFe2O4) nanoparticles by powder X-ray diffraction measurements up to 47 GPa. We found that the cubic spinel structure of ZnFe2O4 remains up to 33 GPa and a phase transition is induced beyond this pressure. The high-pressure phase is indexed to an orthorhombic CaMn2O4-type structure. Upon decompression the low- and high-pressure phases coexist. The compressibility of both structures was also investigated. We have observed that the lattice parameters of the high-pressure phase behave anisotropically upon compression. Further, we predict possible phase transition around 55 GPa. For comparison, we also studied the compressi…

In situMaterials scienceNanostructurePHASE TRANSITIONSCiencias FísicasNanoparticle02 engineering and technologyCrystal structure01 natural sciencesCRYSTAL STRUCTURE0103 physical sciencesGeneral Materials ScienceOXIDES010306 general physicsX-RAY DIFFRACTIONNANOSTRUCTUREGeneral Chemistry021001 nanoscience & nanotechnologyCondensed Matter PhysicsAstronomíaZinc ferriteCrystallographyHigh pressureX-ray crystallography0210 nano-technologyCIENCIAS NATURALES Y EXACTASSolid State Sciences
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Unveiling the nature of six HMXBs through IR spectroscopy

2008

The International Gamma-Ray Astrophyiscs Laboratory (INTEGRAL) is discovering a large number of new hard X-ray sources, many of them being HMXBs. The identification and spectral characterization of their optical/infrared counterparts is a necessary step to undertake detailed study of these systems. In particular, the determination of the spectral type is crucial in the case of the new class of Supergiant Fast X-ray Transients (SFXTs), which show X-ray properties common to other objects. We used the ESO/NTT SofI spectrograph to observe proposed IR counterparts to HMXBs, obtaining Ks medium resolution spectra (R = 1320) with a S/N >= 100. We classified them through comparison with publishe…

InfraredAstrophysics::High Energy Astrophysical PhenomenaExtinction (astronomy)FOS: Physical sciencesInfrared spectroscopyAstrophysicsAstrophysicsStellar classificationSpectral line:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos X [UNESCO]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos XSpectroscopySpectrographAstrophysics::Galaxy AstrophysicsPhysicsAstrophysics (astro-ph)Astronomy and AstrophysicsAccretion accretion disksX-rays : binaries; Stars : supergiants; Accretion accretion disks; Infrared : starsSpace and Planetary Sciencestars [Infrared]binaries [X-rays]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::EstrellasSupergiantsupergiants [Stars]:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]Astronomy & Astrophysics
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