Search results for "Names"

showing 10 items of 6843 documents

MOJAVE: Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments. VI. Kinematics Analysis of a Complete Sample of Blazar Jets

2009

We discuss the jet kinematics of a complete flux-density-limited sample of 135 radio-loud active galactic nuclei (AGN) resulting from a 13 year program to investigate the structure and evolution of parsec-scale jet phenomena. Our analysis is based on new 2 cm Very Long Baseline Array (VLBA) images obtained between 2002 and 2007, but includes our previously published observations made at the same wavelength, and is supplemented by VLBA archive data. In all, we have used 2424 images spanning the years 1994-2007 to study and determine the motions of 526 separate jet features in 127 jets. The data quality and temporal coverage (a median of 15 epochs per source) of this complete AGN jet sample r…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusLorentz transformationAstrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstrophysicsKinematicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencessymbols.namesake0103 physical scienceseducationBlazar010303 astronomy & astrophysicsVery Long Baseline ArrayPhysicseducation.field_of_study010308 nuclear & particles physicsAstronomy and AstrophysicsWavelength13. Climate actionSpace and Planetary SciencesymbolsDoppler effectAstrophysics - Cosmology and Nongalactic Astrophysics
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Cold dark matter plus not-so-clumpy dark relics

2017

Various particle physics models suggest that, besides the (nearly) cold dark matter that accounts for current observations, additional but sub-dominant dark relics might exist. These could be warm, hot, or even contribute as dark radiation. We present here a comprehensive study of two-component dark matter scenarios, where the first component is assumed to be cold, and the second is a non-cold thermal relic. Considering the cases where the non-cold dark matter species could be either a fermion or a boson, we derive consistent upper limits on the non-cold dark relic energy density for a very large range of velocity dispersions, covering the entire range from dark radiation to cold dark matte…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Cold dark matterMilky WayCosmic microwave backgroundDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanck010303 astronomy & astrophysicsCondensed Matter::Quantum GasesPhysics010308 nuclear & particles physicsMatter power spectrumAstronomy and AstrophysicsBaryonHigh Energy Physics - Phenomenology13. Climate actionDark radiationsymbolsAstrophysics - Cosmology and Nongalactic Astrophysics
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Testing theories of Gravity and Supergravity with inflation and observations of the cosmic microwave background

2016

Many extensions of Einstein's theory of gravity have been studied and proposed with various motivations like the quest for a quantum theory of gravity to extensions of anomalies in observations at the solar system, galactic and cosmological scales. These extensions include adding higher powers of Ricci curvature $R$, coupling the Ricci curvature with scalar fields and generalized functions of $R$. In addition when viewed from the perspective of Supergravity (SUGRA) many of these theories may originate from the same SUGRA theory interpreted in different frames. SUGRA therefore serves as a good framework for organizing and generalizing theories of gravity beyond General Relativity. All these …

Cosmology and Nongalactic Astrophysics (astro-ph.CO)General relativitymedia_common.quotation_subjectFOS: Physical sciencesLambda-CDM modelCosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)CMBSUGRA01 natural sciencesCosmologyGeneral Relativity and Quantum CosmologyMetric expansion of spacesymbols.namesakeTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanckinflation010306 general physicsMathematical Physicsmedia_commonPhysics010308 nuclear & particles physicsAstronomy and AstrophysicsUniverseHigh Energy Physics - PhenomenologySpace and Planetary SciencesymbolsDark energyCMB; inflation; SUGRAAstrophysics - Cosmology and Nongalactic Astrophysics
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Universal thermodynamic properties of the intracluster medium over two decades in radius in the X-COP sample

2018

The hot plasma in galaxy clusters is expected to be heated to high temperatures through shocks and adiabatic compression. The thermodynamical properties of the gas encode information on the processes leading to the thermalization of the gas in the cluster's potential well as well as non-gravitational processes such as gas cooling, AGN feedback and kinetic energy. In this work we present the radial profiles of the thermodynamic properties of the intracluster medium (ICM) out to the virial radius for a sample of 12 galaxy clusters selected from the Planck all-sky survey. We determine the universal profiles of gas density, temperature, pressure, and entropy over more than two decades in radius…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)galaxies: clusters: intracluster mediumDark matterPopulationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesdark matterVirial theoremsymbols.namesakeIntracluster medium0103 physical sciencesGravitational collapsePlanckAdiabatic processeducation010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsGalaxy clusterPhysicseducation.field_of_study[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Settore FIS/05010308 nuclear & particles physicsThermodynamical quantitiesAstronomy and AstrophysicsX-rays: galaxies: clusters; dark matter; galaxies: clusters: intracluster medium; galaxies: clusters: general; Thermodynamical quantitiesgalaxies: clusters: general13. Climate actionSpace and Planetary ScienceX-rays: galaxies: clustersastro-ph.COsymbols[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic AstrophysicsAstronomy & Astrophysics
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Impact of cosmic inhomogeneities on SNe observations

2009

We study the impact of cosmic inhomogeneities on the interpretation of SNe observations. We build an inhomogeneous universe model that can confront supernova data and yet is reasonably well compatible with the Copernican Principle. Our model combines a relatively small local void, that gives apparent acceleration at low redshifts, with a meatball model that gives sizeable lensing (dimming) at high redshifts. Together these two elements, which focus on different effects of voids on the data, allow the model to mimic the concordance model.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectgr-qcCosmic background radiationFOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences114 Physical sciencesGeneral Relativity and Quantum CosmologyCosmologysymbols.namesakeObservational cosmology0103 physical sciences010306 general physicsmedia_commonPhysicsCOSMIC cancer database010308 nuclear & particles physicsCopernican principleRedshiftUniverseLocal Voidsymbolsastro-ph.COAstrophysics - Cosmology and Nongalactic Astrophysics
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In the realm of the Hubble tension—a review of solutions

2021

The $\Lambda$CDM model provides a good fit to a large span of cosmological data but harbors areas of phenomenology. With the improvement of the number and the accuracy of observations, discrepancies among key cosmological parameters of the model have emerged. The most statistically significant tension is the $4-6\sigma$ disagreement between predictions of the Hubble constant $H_0$ by early time probes with $\Lambda$CDM model, and a number of late time, model-independent determinations of $H_0$ from local measurements of distances and redshifts. The high precision and consistency of the data at both ends present strong challenges to the possible solution space and demand a hypothesis with en…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)satellite: PlanckPhysics and Astronomy (miscellaneous)gravitation: modelPhysics beyond the Standard ModelCosmic microwave backgroundFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsbaryon: oscillation: acoustic01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologysymbols.namesakeTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)cosmological model: parameter space0103 physical sciencesstructurePlanckinflationcosmic background radiation: power spectrum010306 general physicsdark energyneutrino: interactionPhysicssupernova: Type IHubble constant010308 nuclear & particles physicsnew physicsmagnetic field: primordialtensionredshiftAstrophysics - Astrophysics of GalaxiesRedshiftrecombinationHigh Energy Physics - Phenomenology13. Climate actionAstrophysics of Galaxies (astro-ph.GA)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]relativisticsymbolsDark energy[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Phenomenology (particle physics)statisticalAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's law
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Signorini problem with Coulomb's law of friction. Shape optimization in contact problems

1992

Coulomb's lawNumerical Analysissymbols.namesakeClassical mechanicsApplied MathematicsGeneral EngineeringsymbolsShape optimizationSignorini problemMathematicsInternational Journal for Numerical Methods in Engineering
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One-Counter Verifiers for Decidable Languages

2013

Condon and Lipton (FOCS 1989) showed that the class of languages having a space-bounded interactive proof system (IPS) is a proper subset of decidable languages, where the verifier is a probabilistic Turing machine. In this paper, we show that if we use architecturally restricted verifiers instead of restricting the working memory, i.e. replacing the working tape(s) with a single counter, we can define some IPS’s for each decidable language. Such verifiers are called two-way probabilistic one-counter automata (2pca’s). Then, we show that by adding a fixed-size quantum memory to a 2pca, called a two-way one-counter automaton with quantum and classical states (2qcca), the protocol can be spac…

Counter machineTheoryofComputation_COMPUTATIONBYABSTRACTDEVICESTheoretical computer scienceQuantum registerComputer scienceProbabilistic Turing machineProbabilistic logicInteractive proof systemComputer Science::Computational ComplexityDecidabilityAutomatonsymbols.namesakesymbolsProtocol (object-oriented programming)
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Theoretical absorption spectrum of the Ar–CO van der Waals complex

2003

The three-dimensional intermolecular electric dipole moment surface of Ar–CO is calculated at the coupled cluster singles and doubles level of theory with the aug-cc-pVTZ basis set extended with a 3s3p2d1f1g set of midbond functions. Using the rovibrational energies and wave functions of our recent study [J. Chem. Phys. 117, 6562 (2002)], temperature-dependent spectral intensities are evaluated and compared to available experimental data. Based on the theoretical spectrum, alternative assignments of the experimentally observed lines in the fundamental band of CO around 2160 and 2166 cm−1 are suggested. Thomas.Bondo@uv.es

Coupled Cluster CalculationsAbsorption spectroscopyGeneral Physics and AstronomySpectral Line IntensitySpectral linesymbols.namesakePhysics and Astronomy (all)Argon ; Carbon Compounds ; Quasimolecules ; Molecular Moments ; Coupled Cluster Calculations ; Rotational-Vibrational States ; Spectral Line Intensity ; SpectraQuasimoleculesPhysics::Atomic and Molecular ClustersArgonPhysics::Chemical PhysicsPhysical and Theoretical Chemistry:FÍSICA::Química física [UNESCO]Rotational-Vibrational StatesBasis setMolecular MomentsChemistryIntermolecular forceRotational–vibrational spectroscopySpectraCarbon CompoundsUNESCO::FÍSICA::Química físicaElectric dipole momentCoupled clusterPhysics::Space Physicssymbolsvan der Waals forceAtomic physics
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13C NMR spectroscopy of four tertiary methyl norbornenols and norbornanols

1975

Carbon chemical shifts and direct 13C1H coupling constants of 2-endo-methyl-5-norbornen-2-exo-ol, 2-exo-methyl-5-norbornen-2-endo-ol, 2-endo-methylnorbornan-2-exo-ol and 2-exo-methylnorbornan-2-endo-ol have been measured from single samples using a dual probe pulse Fourier transform method.

Coupling constantCarbon-13 NMR satelliteChemistryChemical shiftAnalytical chemistrychemistry.chemical_elementGeneral ChemistryFluorine-19 NMRsymbols.namesakeFourier transform13c nmr spectroscopysymbolsGeneral Materials ScienceTransverse relaxation-optimized spectroscopyCarbonOrganic Magnetic Resonance
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