Search results for "PACE"

showing 10 items of 21903 documents

Fixed Points for Multivalued Convex Contractions on Nadler Sense Types in a Geodesic Metric Space

2019

In 1969, based on the concept of the Hausdorff metric, Nadler Jr. introduced the notion of multivalued contractions. He demonstrated that, in a complete metric space, a multivalued contraction possesses a fixed point. Later on, Nadler&rsquo

<b>54H25</b>Physics and Astronomy (miscellaneous)GeodesicGeneral MathematicsMathematics::General TopologyFixed-point theorem02 engineering and technologyFixed point01 natural sciencesComplete metric spacegeodesic metric spaceCombinatoricsregular golbal-inf function0202 electrical engineering electronic engineering information engineeringComputer Science (miscellaneous)0101 mathematicsMathematicsStatistics::Applicationslcsh:Mathematics010102 general mathematicsRegular polygonconvex multivalued left A-contractionlcsh:QA1-939Metric spaceHausdorff distancefixed point<b>47H10</b>Chemistry (miscellaneous)<title>MSC</title>020201 artificial intelligence & image processingright A-contractionSymmetry
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Event Horizon Telescope imaging of the archetypal blazar 3C 279 at an extreme 20 microarcsecond resolution

2020

Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Open Access funding provided by Max Planck Society.--All authors: Kim, Jae-Young; Krichbaum, Thomas P.; Broderick, Avery E.; Wielgus, Maciek; Blackburn, Lindy; Gómez, José L.; Johnson, Michael D.; Bouman, Katherine L.; Chael, Andrew; Akiyama, Kazunori; Jorstad, Svetlana; Marscher, Alan P.; Issaoun, Sara; Janssen, Michael; Chan, Chi-kwan; Savolainen, Tuomas; Pesce, Dominic W.; Özel, Feryal; Alberdi, Antxon; Alef, Walt…

ACTIVE GALACTIC NUCLEIBrightnessActive galactic nucleusactive [Galaxies]Astrophysics::High Energy Astrophysical PhenomenaAstronomygalaxies: activeAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSubmillimeter ArrayFLOWSSCALE CIRCULAR-POLARIZATION0103 physical sciencesVery-long-baseline interferometryBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsEvent Horizon Telescope[PHYS]Physics [physics]Jet (fluid)010308 nuclear & particles physicsAstronomy and AstrophysicsFLAREgalaxies: jetsindividual: 3C 279 [Galaxies]LONGVARIABILITYgalaxies: individual: 3C 279GAMMA-RAYQUASARS13. Climate actionSpace and Planetary Sciencetechniques: interferometricBrightness temperatureACCRETION DISKSinterferometric [Techniques]jets [Galaxies]RELATIVISTIC JETS[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & astrophysics
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On the carrier of inertia

2018

A change in momentum will inevitably perturb the all-embracing vacuum, whose reaction we understand as inertia. Since the vacuum's physical properties relate to light, we propose that the vacuum embodies photons, but in pairs without net electromagnetic fields. In this physical form the free space houses energy in balance with the energy of matter in the whole Universe. Likewise, we reason that a local gravitational potential is the vacuum in a local balance with energy that is bound to a body. Since a body couples to the same vacuum universally and locally, we understand that inertial and gravitational masses are identical. By the same token, we infer that gravity and electromagnetism shar…

ANOMALIESPhotonmedia_common.quotation_subjectvacuumUNIVERSEGeneral Physics and AstronomyCosmological constantPHOTONSInertia01 natural sciencesGravitationMomentumGeneral Relativity and Quantum CosmologyGravitational potentialElectromagnetism0103 physical sciences010306 general physics010303 astronomy & astrophysicsCOSMOLOGICAL CONSTANTmedia_commonPhysicsfotonitta114LEAST-ACTIONgravitaatioinertialiike115 Astronomy Space sciencelcsh:QC1-999UniverseTIMEmotion (physical phenomena)GALAXIESClassical mechanicsgravitationWAVEPRINCIPLECLUSTERSlcsh:PhysicsAIP Advances
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Search for neutrino emission from gamma-ray flaring blazars with the ANTARES telescope

2012

The ANTARES telescope observes a full hemisphere of the sky all the time with a duty cycle close to 100%. This makes it well suited for an extensive observation of neutrinos produced in astrophysical transient sources. In the surrounding medium of blazars, i.e. active galactic nuclei with their jets pointing almost directly towards the observer, neutrinos may be produced together with gamma-rays by hadronic interactions, so a strong correlation between neutrinos and gamma-rays emissions is expected. The time variability information of the studied source can be obtained by the gamma-ray light curves measured by the LAT instrument on-board the Fermi satellite. If the expected neutrino flux ob…

ASTROPHYSICSAstrofísicaAstrophysicsNeutrino Astronomy01 natural sciences7. Clean energyLARGE-AREA TELESCOPElaw.inventionlawWATERInstrumentation010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Time-dependent searchCATALOGLIGHTNeutrino astronomyFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaACTIVE GALACTIC NUCLEINuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Active galactic nucleus[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Point sourceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsfermi lat transient sources; neutrino astronomy; time-dependent search; antares; blazarsTelescopeMUONS0103 physical sciencesANTARES; Neutrino Astronomy; Fermi LAT transient sourcesBlazarANTARES010308 nuclear & particles physicsAstronomyAstronomy and AstrophysicsFermi LAT transient sourcesLight curveNeutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]MODEL13. Climate actionFISICA APLICADA:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]Neutrino astronomy[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]BlazarsFermi Gamma-ray Space Telescope
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H-He collision-induced satellite in the Lyman alpha profile of DBA white dwarf stars

2020

The spectra of helium-dominated white dwarf stars with hydrogen in their atmosphere present a distinctive broad feature centered around 1160~\AA\/ in the blue wing of the Lyman-$\alpha$ line. It is extremely apparent in WD 1425+540 recently observed with HST COS. With new theoretical line profiles based on ab initio atomic interaction potentials we show that this feature is a signature of a collision-induced satellite due to an asymptotically forbidden transition. This quasi-molecular spectral satellite is crucial to understanding the asymmetrical shape of Lyman-$\alpha$ seen in this and other white dwarf spectra. Our previous work predicting this absorption feature was limited by molecular…

ATOMIC DATALINE: PROFILEAb initiochemistry.chemical_elementBASIS-SETLINEEXCITED-STATEAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral linePhysics - Atomic PhysicsWHITE DWARF0103 physical sciencesRadiative transferABSORPTIONAstrophysics::Solar and Stellar AstrophysicsAB-INITIO CALCULATIONPhysics::Atomic PhysicsELECTRONIC-TRANSITION MOMENT010306 general physicsSTARS: ATMOSPHERE010303 astronomy & astrophysicsHeliumLine (formation)POTENTIAL-ENERGY CURVEPhysics[PHYS]Physics [physics]BALMER-ALPHAWhite dwarfAstronomy and AstrophysicsMOLECULAR DATAPotential energyDipolechemistryAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceATOMIC PROCESSSHAPE[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Atomic physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Abel transforms with low regularity with applications to X-ray tomography on spherically symmetric manifolds

2017

We study ray transforms on spherically symmetric manifolds with a piecewise $C^{1,1}$ metric. Assuming the Herglotz condition, the X-ray transform is injective on the space of $L^2$ functions on such manifolds. We also prove injectivity results for broken ray transforms (with and without periodicity) on such manifolds with a $C^{1,1}$ metric. To make these problems tractable in low regularity, we introduce and study a class of generalized Abel transforms and study their properties. This low regularity setting is relevant for geophysical applications.

Abel transformsMathematics - Differential GeometryClass (set theory)Pure mathematicsApplied Mathematics010102 general mathematicsgeodesic x-ray tomographySpace (mathematics)01 natural sciencesInjective functionComputer Science ApplicationsTheoretical Computer Science010101 applied mathematicsDifferential Geometry (math.DG)geophysical imagingBroken ray tomographySignal ProcessingMetric (mathematics)PiecewiseFOS: MathematicsTomography0101 mathematicsspherical symmetryMathematical PhysicsMathematics
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Non-archimedean hyperbolicity and applications

2018

Inspired by the work of Cherry, we introduce and study a new notion of Brody hyperbolicity for rigid analytic varieties over a non-archimedean field $K$ of characteristic zero. We use this notion of hyperbolicity to show the following algebraic statement: if a projective variety admits a non-constant morphism from an abelian variety, then so does any specialization of it. As an application of this result, we show that the moduli space of abelian varieties is $K$-analytically Brody hyperbolic in equal characteristic zero. These two results are predicted by the Green-Griffiths-Lang conjecture on hyperbolic varieties and its natural analogues for non-archimedean hyperbolicity. Finally, we use …

Abelian varietyPure mathematicsConjectureMathematics - Number TheoryApplied MathematicsGeneral Mathematics010102 general mathematics[MATH.MATH-AG] Mathematics [math]/Algebraic Geometry [math.AG]Field (mathematics)01 natural sciencesModuli spaceMathematics - Algebraic GeometryMorphism0103 physical sciencesUniformization theoremFOS: MathematicsNumber Theory (math.NT)[MATH.MATH-AG]Mathematics [math]/Algebraic Geometry [math.AG]010307 mathematical physics0101 mathematicsAbelian groupAlgebraic Geometry (math.AG)Projective varietyMathematicsJournal für die reine und angewandte Mathematik (Crelles Journal)
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Centri minori fra modelli nuovi o ritrovati. Le alte Madonie tra opportunità e suggestioni

2022

«Un’architettura basata sulla complessità e sulla contraddizione richiede un impegno speciale verso l’insieme: la sua reale validità deve essere nella sua totalità, o nelle sue implicazioni di totalità» afferma Robert Venturi (Venturi, 2005, p. 16). Questo suggerimento è ancora essenziale per tutti coloro che intendono affrontare da vicino il ruolo del progetto nel territorio dei Centri minori? Sigfried Giedion, nel suo Space, Time and Architecture leggeva l’edificio per l’abitante della città. Aveva voglia di «godersi il panorama, le brezze ed il sole, godere in tutta calma quella naturale libertà di cui il suo lavoro lo privava» (Giedion, 1953, p. 505). A distanza di molti anni, il nostro…

Abitanti di ritorno Modificazione Spazio-Tempo-ArchitetturaSettore ICAR/14 - Composizione Architettonica E UrbanaReturn inhabitants Modification Space-Time-Architecture
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The large trans-Neptunian object 2002 TC 302 from combined stellar occultation, photometry, and astrometry data

2020

All authors: Ortiz, J. L.; Santos-Sanz, P.; Sicardy, B.; Benedetti-Rossi, G.; Duffard, R.; Morales, N.; Braga-Ribas, F.; Fernández-Valenzuela, E.; Nascimbeni, V.; Nardiello, D.; Carbognani, A.; Buzzi, L.; Aletti, A.; Bacci, P.; Maestripieri, M.; Mazzei, L.; Mikuz, H.; Skvarc, J.; Ciabattari, F.; Lavalade, F. Scarfi, G.; Mari, J. M.; Conjat, M.; Sposetti, S.; Bachini, M.; Succi, G.; Mancini, F.; Alighieri, M.; Dal Canto, E.; Masucci, M.; Vara-Lubiano, M.; Gutiérrez, P. J.; Desmars, J.; Lecacheux, J.; Vieira-Martins, R.; Camargo, J. I. B.; Assafin, M.; Colas, F.; Beisker, W.; Behrend, R.; Mueller, T. G.; Meza, E.; Gomes-Junior, A. R.; Roques, F.; Vachier, F.; Mottola, S.; Hellmich, S.; Campo …

Absolute magnitude010504 meteorology & atmospheric sciencesFOS: Physical sciencesAstrophysicsKuiper belt objects: individual: 2002 TC30201 natural sciencesOccultationlaw.inventionTelescopePhotometry (optics)lawGeometric albedoFísica Aplicada0103 physical sciencesTrans-Neptunian object010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciencesPhysics[PHYS]Physics [physics]Earth and Planetary Astrophysics (astro-ph.EP)photometric [Techniques]Astronomy and Astrophysicsgeneral [Kuiper belt]Astrometryindividual: 2002 TC302 [Kuiper belt objects]AstrometryAstrometry; Kuiper belt objects: individual: 2002 TC302; Kuiper belt: general; Occultations; Techniques: photometricLight curveSpace and Planetary Science[SDU]Sciences of the Universe [physics]Kuiper belt: generalOccultations[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Techniques: photometricAstrophysics - Earth and Planetary AstrophysicsAstronomy &amp; Astrophysics
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A parametric description of the 3D structure of the Galactic bar/bulge using the VVV survey

2017

We study the structure of the inner Milky Way using the latest data release of the Vista Variables in Via Lactea (VVV) survey. The VVV is a deep near-infrared, multi-colour photometric survey with a coverage of 300 square degrees towards the Bulge/Bar. We use Red Clump (RC) stars to produce a high-resolution dust map of the VVV's field of view. From de-reddened colour-magnitude diagrams we select Red Giant Branch stars to investigate their 3D density distribution within the central 4 kpc. We demonstrate that our best-fit parametric model of the Bulge density provides a good description of the VVV data, with a median percentage residual of 5$\%$ over the fitted region. The strongest of the o…

Absolute magnitudeInitial mass functionastro-ph.GAMilky WayFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxy: bulgeBulge0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsRed clumpGalaxy: structureAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSLuminosity function (astronomy)Physics010308 nuclear & particles physicsGalactic CenterAstronomyAstronomy and AstrophysicsGalaxy: fundamental parametersAstrophysics - Astrophysics of GalaxiesGalaxy: centregalaxies: individual: Milky WayRed-giant branchSpace and Planetary ScienceGalaxy: formationAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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