Search results for "proper"

showing 10 items of 3167 documents

Combining a context aware neural network with a denoising autoencoder for measuring string similarities

2020

Abstract Measuring similarities between strings is central for many established and fast-growing research areas, including information retrieval, biology, and natural-language processing. The traditional approach to string similarity measurements is to define a metric with respect to a word space that quantifies and sums up the differences between characters in two strings; surprisingly, these metrics have not evolved a great deal over the past few decades. Indeed, the majority of them are still based on making a simple comparison between character and character distributions without considering the words context. This paper proposes a string metric that encompasses similarities between str…

Artificial neural networkProperty (programming)Computer sciencebusiness.industryString (computer science)020206 networking & telecommunicationsContext (language use)02 engineering and technologycomputer.software_genre01 natural sciencesTheoretical Computer ScienceHuman-Computer InteractionCharacter (mathematics)0103 physical sciencesMetric (mathematics)0202 electrical engineering electronic engineering information engineeringArtificial intelligenceString metricbusiness010301 acousticscomputerSoftwareWord (computer architecture)Natural language processingComputer Speech & Language
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Top management team demography and firm operating performance: a path analysis

2020

PurposeThis paper examined the relationship between TMT demographic properties and firm performance using diversity and level variables and measuring differing constructs of firm performance representing divergent strategies.Design/methodology/approachStructural equation modelling was used to test the relationships between TMT demographic properties and firm performance measured as return on net operating assets (RNOA), and its disaggregates profit margin (PM) and asset turnover (ATO). Data were from 89 Finnish firms during the years 2008–2011, resulting in 320 observations.FindingsTMT team tenure had associations with RNOA through both PM and ATO while TMT age, age diversity, firm tenure, …

Asset turnoverStrategy and Managementoperating performanceMicroeconomicsNet operating assets0502 economics and businessTop managementProfit marginpath analysisBusiness and International ManagementPath analysis (statistics)yritysjohtajattulosohjaustop management teamikärakenneteam properties05 social sciencesdisaggretation050209 industrial relationstuloksetfirm performanceUpper echelonsupper echelonsBusinessjohtoryhmät050203 business & managementJournal of Strategy and Management
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Internal Simulation of an Agent’s Intentions

2013

We present the Associative Self-Organizing Map (A-SOM) and propose that it could be used to predict an agent’s intentions by internally simulating the behaviour likely to follow initial movements. The A-SOM is a neural network that develops a representation of its input space without supervision, while simultaneously learning to associate its activity with an arbitrary number of additional (possibly delayed) inputs. We argue that the A-SOM would be suitable for the prediction of the likely continuation of the perceived behaviour of an agent by learning to associate activity patterns over time, and thus a way to read its intentions.

Associative Self-Organizing Map; Internal Simulation;ContinuationArtificial neural networkbusiness.industryComputer scienceAssociative Self-Organizing MapRepresentation (systemics)Artificial intelligenceSpace (commercial competition)businessInternal SimulationAssociative property
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Cosmological bounds on neutrino statistics

2018

We consider the phenomenological implications of the violation of the Pauli exclusion principle for neutrinos, focusing on cosmological observables such as the spectrum of Cosmic Microwave Background anisotropies, Baryon Acoustic Oscillations and the primordial abundances of light elements. Neutrinos that behave (at least partly) as bosonic particles have a modified equilibrium distribution function that implies a different influence on the evolution of the Universe that, in the case of massive neutrinos, can not be simply parametrized by a change in the effective number of neutrinos. Our results show that, despite the precision of the available cosmological data, only very weak bounds can …

AstrofísicaCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaCosmic microwave backgroundFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsNeutrino properties01 natural sciencesPartícules (Física nuclear)symbols.namesakePauli exclusion principleHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesis0103 physical sciencesStatisticsAnisotropy010303 astronomy & astrophysicsPhysicsCosmologia010308 nuclear & particles physicsBig bang nucleosynthesisSpectrum (functional analysis)High Energy Physics::PhenomenologyObservableAstronomy and AstrophysicsCosmological neutrinos neutrino properties big bang nucleosynthesis cosmological parameters from CMBRCosmological parameters from CMBRHigh Energy Physics - Phenomenologysymbolsastro-ph.COBig bang nucleosynthesis; Cosmological neutrinos; Cosmological parameters from CMBR; Neutrino properties; astro-ph.CO; astro-ph.CO; High Energy Physics - Phenomenology; Astronomy and AstrophysicsCosmological neutrinosHigh Energy Physics::ExperimentBaryon acoustic oscillationsNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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Non-linear evolution of the cosmic neutrino background

2012

We investigate the non-linear evolution of the relic cosmic neutrino background by running large box-size, high resolution N-body simulations which incorporate cold dark matter (CDM) and neutrinos as independent particle species. Our set of simulations explore the properties of neutrinos in a reference Lambda CDM model with total neutrino masses between 0.05-0.60 eV in cold dark matter haloes of mass 10(11) – 10(15) h(-1) M-circle dot, over a redshift range z = 0 – 2. We compute the halo mass function and show that it is reasonably well fitted by the Sheth-Tormen formula, once the neutrino contribution to the total matter is removed. More importantly, we focus on the CDM and neutrino proper…

AstrofísicaCosmology and Nongalactic Astrophysics (astro-ph.CO)Cold dark mattercosmological neutrinosFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencesMomentumSettore FIS/05 - Astronomia e Astrofisica0103 physical sciencesPeculiar velocity010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsneutrino propertiesPhysicsCosmologia010308 nuclear & particles physicsHalo mass functionAstronomy and Astrophysicsneutrino masses from cosmologyRedshiftCosmic neutrino background13. Climate actionHigh Energy Physics::ExperimentHaloNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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VLBA observations of a rare multiple quasar imaging event caused by refraction in the interstellar medium

2013

We report on the first detection of the theoretically-predicted rare phenomenon of multiple parsec-scale imaging of an active galactic nucleus induced by refractive effects due to localized foreground electron density enhancements, e.g., in an AU-scale plasma lens(es) in the ionized component of the Galactic interstellar medium. We detected multiple imaging in the low galactic latitude (b=-2 deg) quasar 2023+335 from the 15.4 GHz MOJAVE observations when the source was undergoing an ESE. While the parsec-scale jet of the source normally extends along PA -20 deg, in the 28 May 2009 and 23 July 2009 images a highly significant multi-component pattern of secondary images is stretched out nearl…

AstrofísicaProper motionActive galactic nucleusCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAngular diameter0103 physical sciencesVery-long-baseline interferometry010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsLine (formation)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsScatteringAstronomy and AstrophysicsQuasarInterstellar mediumSpace and Planetary ScienceAstronomiaAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysics
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Modeling the shock-cloud interaction in SN 1006: unveiling the origin of nonthermal X-ray and gamma-ray emission

2016

The supernova remnant SN 1006 is a source of high-energy particles and its southwestern limb is interacting with a dense ambient cloud, thus being a promising region for gamma-ray hadronic emission. We aim at describing the physics and the nonthermal emission associated with the shock-cloud interaction to derive the physical parameters of the cloud (poorly constrained by the data analysis), to ascertain the origin of the observed spatial variations in the spectral properties of the X-ray synchrotron emission, and to predict spectral and morphological features of the resulting gamma-ray emission. We performed 3-D magnetohydrodynamic simulations modeling the evolution of SN 1006 and its inter…

AstrofísicaProper motionMagnetohydrodynamics (MHD)[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::High Energy Astrophysical PhenomenaHadronFOS: Physical sciencesContext (language use)AstrophysicsISM: individual objects: SN 100601 natural sciencesISM: cloudslaw.inventionSettore FIS/05 - Astronomia E AstrofisicalawISM: cloud0103 physical sciencesMagnetohydrodynamic driveSupernova remnant010303 astronomy & astrophysicsISM: supernova remnantAstrophysics::Galaxy Astrophysicsacceleration of particlesISM: supernova remnantsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsclouds; ISM: individual objects: SN 1006; ISM: supernova remnants; Magnetohydrodynamics (MHD); X-rays: ISM; Astronomy and Astrophysics; Space and Planetary Science [Acceleration of particles; ISM]X-rayAstronomy and AstrophysicsAstronomy and AstrophysicAcceleration of particleSynchrotronX-rays: ISMShock (mechanics)Astronomía13. Climate actionSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Sterile Neutrinos in Light of Recent Cosmological and Oscillation Data: a Multi-Flavor Scheme Approach

2008

Light sterile neutrinos might mix with the active ones and be copiously produced in the early Universe. In the present paper, a detailed multi-flavor analysis of sterile neutrino production is performed. Making some justified approximations allows us to consider not only neutrino interactions with the primeval medium and neutrino coherence breaking effects, but also oscillation effects arising from the presence of three light (mostly-active) neutrino states mixed with two heavier (mostly-sterile) states. First, we emphasize the underlying physics via an analytical description of sterile neutrino abundances that is valid for cases with small mixing between active and sterile neutrinos. Then,…

AstrofísicaSterile neutrinoParticle physicscosmological neutrinosAstrophysics::High Energy Astrophysical PhenomenaCosmic microwave backgroundFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyMiniBooNEHigh Energy Physics - Phenomenology (hep-ph)astro-ph0103 physical sciencesScale structurephysics of the early universe010306 general physicsneutrino propertiesPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)Astronomy and Astrophysicshep-phHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoPhenomenology (particle physics)Coherence (physics)
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Dark radiation sterile neutrino candidates after Planck data

2013

Recent Cosmic Microwave Background (CMB) results from the Planck satellite, combined with previous CMB data and Hubble constant measurements from the Hubble Space Telescope, provide a constraint on the effective number of relativistic degrees of freedom 3.62(-0.48)(+0.50) at 95% CL. New Planck data provide a unique opportunity to place limits on models containing relativistic species at the decoupling epoch. We present here the bounds on sterile neutrino models combining Planck data with galaxy clustering information. Assuming N-eff active plus sterile massive neutrino species, in the case of a Planck+WP+HighL+HST analysis we find m(nu,sterile)(eff) < 0.36 eV and 3.14 < N-eff < 4.15 at 95% …

AstrofísicaSterile neutrinocosmological neutrinosHadronCosmic microwave backgroundAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesPartícules (Física nuclear)symbols.namesake0103 physical sciencesneutrino properties; dark energy theory; neutrino theory; cosmological neutrinosdark energy theoryPlanck010303 astronomy & astrophysicsAxionAstrophysics::Galaxy Astrophysicsneutrino propertiesPhysicsCosmologia010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsDecoupling (cosmology)neutrino theory13. Climate actionDark radiationsymbolsHigh Energy Physics::ExperimentHubble's law
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Pregiudizio classico e moderno nei confronti dei richiedenti asilo: un contributo alla validazione italiana della Prejudice Against Asylum Seekers Sc…

2021

In this study, we tested the validity of the Italian version of the Prejudice Against Asylum Seekers Scale (PAAS), which measures classic and modern prejudice toward asylum seekers. A sample of 740 participants (227 males and 513 females, aged 18-67) completed the scale. The results were consistent with the original 2-factor model providing an acceptable fit for the data. This study, however, suggests taking out two items from the scale. The two correlated factors showed significant associations with right-wing authoritarianism, social dominance orientation, and national identification. No gender differences emerged, but only those related to religious affiliation, age, and political orient…

Asylum seekers Classical and modern prejudice Psychometric propertiesSettore M-PSI/05 - Psicologia Sociale
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