Search results for "Quantum"

showing 10 items of 9714 documents

Study of the reflection spectrum of the accreting neutron star GX 3+1 using XMM-Newton and INTEGRAL

2015

Broad emission features of abundant chemical elements, such as Iron, are commonly seen in the X-ray spectra of accreting compact objects and their studies can provide useful information about the geometry of the accretion processes. In this work, we focus our attention on GX 3+1, a bright, persistent accreting low mass X-ray binary, classified as an atoll source. Its spectrum is well described by an accretion disc plus a stable comptonizing, optically thick corona which dominates the X-ray emission in the 0.3-20 keV energy band. In addition, four broad emission lines are found and we associate them with reflection of hard photons from the inner regions of the accretion disc where doppler an…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSpectral lineSettore FIS/05 - Astronomia E AstrofisicaIonizationAstrophysics::Solar and Stellar AstrophysicsEmission spectrumAccretion accretion discAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)AstronomyAstronomy and AstrophysicsX-rays: binarieStars: neutronNeutron starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceReflection (physics)X-rays: individual (GX 3+1)Low MassRelativistic quantum chemistryAstrophysics - High Energy Astrophysical Phenomena
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GRAVITATIONAL WAVE SIGNATURES IN BLACK HOLE FORMING CORE COLLAPSE

2013

We present numerical simulations in general relativity of collapsing stellar cores. Our initial model consists of a low metallicity rapidly-rotating progenitor which is evolved in axisymmetry with the latest version of our general relativistic code CoCoNuT, which allows for black hole formation and includes the effects of a microphysical equation of state (LS220) and a neutrino leakage scheme to account for radiative losses. The motivation of our study is to analyze in detail the emission of gravitational waves in the collapsar scenario of long gamma-ray bursts. Our simulations show that the phase during which the proto-neutron star (PNS) survives before ultimately collapsing to a black hol…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics01 natural sciencesInstabilityGeneral Relativity and Quantum Cosmology0103 physical sciencesRadiative transferAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsEinstein Telescope010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsVirgo ClusterBlack holeSupernovaNeutron starAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaThe Astrophysical Journal
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Relativistic positioning systems: Perspectives and prospects

2013

Relativistic positioning systems are interesting {\em technical objects} for applications around the Earth and in the Solar system. But above all else, they are basic {\em scientific objects} allowing developing relativity from its own concepts. Some past and future features of relativistic positioning systems, with special attention to the developments that they suggest for an {\em epistemic relativity} (relativistic experimental approach to physics), are analyzed. This includes {\em relativistic stereometry}, which, together with relativistic positioning systems, allows to introduce the general relativistic notion of (finite) {\em laboratory} (space-time region able to perform experiments…

Astrophysics::High Energy Astrophysical PhenomenaNuclear TheoryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum Cosmology
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Are pulsars born with a hidden magnetic field?

2015

The observation of several neutron stars in the center of supernova remnants and with significantly lower values of the dipolar magnetic field than the average radio-pulsar population has motivated a lively debate about their formation and origin, with controversial interpretations. A possible explanation requires the slow rotation of the proto-neutron star at birth, which is unable to amplify its magnetic field to typical pulsar levels. An alternative possibility, the hidden magnetic field scenario, considers the accretion of the fallback of the supernova debris onto the neutron star as responsible for the submergence (or screening) of the field and its apparently low value. In this paper …

Astrophysics::High Energy Astrophysical Phenomenageneral [Pulsars]FOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyPulsar0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsAstronomía y AstrofísicaPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)AstronomyAstronomy and Astrophysicsneutron [Stars]Magnetic fieldmagnetic field [Stars]Work (electrical)Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Towards asteroseismology of core-collapse supernovae with gravitational-wave observations – I. Cowling approximation

2017

Gravitational waves from core-collapse supernovae are produced by the excitation of different oscillation modes in the protoneutron star (PNS) and its surroundings, including the shock. In this work we study the relationship between the post-bounce oscillation spectrum of the PNS–shock system and the characteristic frequencies observed in gravitational-wave signals from core-collapse simulations. This is a fundamental first step in order to develop a procedure to infer astrophysical parameters of the PNS formed in core-collapse supernovae. Our method combines information from the oscillation spectrum of the PNS, obtained through linear perturbation analysis in general relativity of a backgr…

Astrophysics::High Energy Astrophysical Phenomenaoscillations [Stars]general [Supernovae]Collapse (topology)FOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesAsteroseismologyGeneral Relativity and Quantum CosmologyGravitational waves0103 physical sciencesCuriemedia_common.cataloged_instanceAstrophysics::Solar and Stellar AstrophysicsEuropean unionCowling010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)media_commonAstronomía y AstrofísicaPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)numerical [Methods]010308 nuclear & particles physicsGravitational waveAsteroseismologyAstronomyAstronomy and Astrophysicsneutron [Stars]SupernovaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena
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ATLAS measurements of the properties of jets for boosted particle searches

2012

Measurements are presented of the properties of high transverse momentum jets, produced in proton-proton collisions at a center-of-mass energy of √s=7  TeV. The data correspond to an integrated luminosity of 35  pb−1 and were collected with the ATLAS detector in 2010. Jet mass, width, eccentricity, planar flow and angularity are measured for jets reconstructed using the anti-kt algorithm with distance parameters R=0.6 and 1.0, with transverse momentum pT>300  GeV and pseudorapidity |η|<2. The measurements are compared to the expectations of Monte Carlo generators that match leading-logarithmic parton showers to leading-order, or next-to-leading-order, matrix elements. The generators describ…

Atlas detectorMonte Carlo methodParton7. Clean energy01 natural sciencesNucleonHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentNUCLEONATLAS; jets; boostedQCDetectors de radiacióQuantum chromodynamicsPhysicsLarge Hadron ColliderAcceleradors de partículesSettore FIS/01 - Fisica SperimentaleATLASINCLUSIVE JET CROSS SECTIONLarge Hadron ColliderPseudorapidityTransverse momentumComputingMethodologies_DOCUMENTANDTEXTPROCESSINGLHCFRAGMENTATIONNucleonParticle Physics - ExperimentjetsNuclear and High Energy PhysicsParticle physicsCiências Naturais::Ciências Físicas530 PhysicsAstrophysics::High Energy Astrophysical Phenomena:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2530Partícules (Física nuclear)Proton-proton collisionsNuclear physics0103 physical sciencesddc:530High Energy Physics010306 general physicsCiencias ExactasScience & TechnologyATLAS detector010308 nuclear & particles physicsFísicaMODELHADRON-HADRON COLLISIONSCol·lisions (Física nuclear)PARTON DISTRIBUTIONSExperimental High Energy PhysicsHigh Energy Physics::ExperimentModel
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Design, construction and commissioning of the Braunschweig Icing Wind Tunnel

2018

Beyond its physical importance in both fundamental and climate research, atmospheric icing is considered as a severe operational condition in many engineering applications like aviation, electrical power transmission and wind-energy production. To reproduce such icing conditions in a laboratory environment, icing wind tunnels are frequently used. In this paper, a comprehensive overview on the design, construction and commissioning of the Braunschweig Icing Wind Tunnel is given. The tunnel features a test section of 0.5 m  ×  0.5 m with peak velocities of up to 40 m s−1. The static air temperature ranges from −25 to +30 °C. Supercooled droplet icing with liquid water contents up to 3 g m−3 c…

Atmospheric Science010504 meteorology & atmospheric sciencesMeteorologyMesoscale meteorology02 engineering and technology7. Clean energy01 natural sciencesArticlelaw.inventionPhysics::GeophysicsIcing conditions0203 mechanical engineeringlawddc:6Veröffentlichung der TU Braunschweigicing wind tunnelddc:62lcsh:TA170-171WolkenphysikPhysics::Atmospheric and Oceanic Physics0105 earth and related environmental sciencesIcingWind tunnel[SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphere020301 aerospace & aeronauticsIce crystalslcsh:TA715-787lcsh:Earthwork. FoundationsCondensed Matter::Mesoscopic Systems and Quantum Hall EffectAtmospheric icinglcsh:Environmental engineeringPhysics::Space PhysicsParticleEnvironmental scienceAstrophysics::Earth and Planetary AstrophysicsCloud chamberddc:620Publikationsfonds der TU BraunschweigMarine engineering
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The challenge of simulating the sensitivity of the Amazonian clouds microstructure to cloud condensation nuclei number concentrations

2019

The realistic representation of cloud-aerosol interactions is of primary importance for accurate climate model projections. The investigation of these interactions in strongly contrasting clean and polluted atmospheric conditions in the Amazon area has been one of the motivations for several field observations, including the airborne Aerosol, Cloud, Precipitation, and Radiation Interactions and DynamIcs of CONvective cloud systems &ndash; Cloud Processes of the Main Precipitation Systems in Brazil: A Contribution to Cloud Resolving Modeling and to the GPM (Global Precipitation Measurement) (ACRIDICON-CHUVA) campaign based in Manaus, Brazil in September 2014. In this work we combine in situ …

Atmospheric Science010504 meteorology & atmospheric sciencesaerosolNuclear TheoryCloud computingAtmospheric sciences01 natural scienceslcsh:ChemistryCloud base0103 physical sciencesddc:550Cloud condensation nucleicloudPrecipitationmicrophysicsWolkenphysikNuclear Experiment010303 astronomy & astrophysicsPhysics::Atmospheric and Oceanic PhysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesEffective radiusCondensed Matter::Quantum Gasescloud condenstion nucleiLidarbusiness.industryCondensed Matter::Otherlcsh:QC1-999Aerosollcsh:QD1-999Environmental scienceClimate modelbusinessGlobal Precipitation Measurementlcsh:Physics
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Influence of clouds on the spectral actinic flux density in the lower troposphere (INSPECTRO): overview of the field campaigns

2008

Ultraviolet radiation is the key factor driving tropospheric photochemistry. It is strongly modulated by clouds and aerosols. A quantitative understanding of the radiation field and its effect on photochemistry is thus only possible with a detailed knowledge of the interaction between clouds and radiation. The overall objective of the project INSPECTRO was the characterization of the three-dimensional actinic radiation field under cloudy conditions. This was achieved during two measurement campaigns in Norfolk (East Anglia, UK) and Lower Bavaria (Germany) combining space-based, aircraft and ground-based measurements as well as simulations with the one-dimensional radiation transfer model UV…

Atmospheric ScienceAIRBORNEMODEL INTERCOMPARISON IPMMI010504 meteorology & atmospheric sciencesPHOTOCHEMICAL ACTIVITYmedia_common.quotation_subjectFluxPHOTOLYSIS FREQUENCY-MEASUREMENTRadiationAtmospheric sciences01 natural sciencesBROKEN CLOUDlaw.inventionTroposphere010309 opticslcsh:Chemistrylaw0103 physical sciencesddc:550MEASUREMENTSZenithABSORPTION CROSS-SECTIONSmedia_commonRemote sensingMonochromator0105 earth and related environmental sciences[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereVERTICAL-DISTRIBUTIONStray lightlcsh:QC1-999UVJSpectroradiometerlcsh:QD1-999Sky13. Climate actionQUANTUM YIELDSEnvironmental science/dk/atira/pure/subjectarea/asjc/1900/1902lcsh:PhysicsAEROSOL EXTINCTION
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Approaches to relativistic positioning around Earth and error estimations

2016

In the context of relativistic positioning, the coordinates of a given user may be calculated by using suitable information broadcast by a 4-tuple of satellites. Our 4-tuples belong to the Galileo constellation. Recently, we estimated the positioning errors due to uncertainties in the satellite world lines (U-errors). A distribution of U-errors was obtained, at various times, in a set of points covering a large region surrounding Earth. Here, the positioning errors associated to the simplifying assumption that photons move in Minkowski space-time (S-errors) are estimated and compared with the U-errors. Both errors have been calculated for the same points and times to make comparisons possib…

Atmospheric ScienceGeneral relativityAerospace EngineeringFOS: Physical sciencesContext (language use)General Relativity and Quantum Cosmology (gr-qc)Error analysis for the Global Positioning SystemPrecise Point Positioning01 natural sciencesGeneral Relativity and Quantum CosmologyGravitational field0103 physical sciencesStatistical physics010303 astronomy & astrophysicsPhysicsSpacecraft010308 nuclear & particles physicsbusiness.industryAstronomy and AstrophysicsGeophysicsClassical mechanicsSpace and Planetary ScienceGeneral Earth and Planetary SciencesSatellitebusinessSchwarzschild radius
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