Search results for "Game"

showing 10 items of 1663 documents

Effects of tributyltin(IV) chloride on the gametes and fertilization ofAscidia malaca (Ascidiacea: Tunicata)

2003

Ascidia malaca gametes before fertilization incubated in 10-5 or 10-7 M solutions of tributyltin(IV) chloride, TBTCl, for 3 h appear highly damaged under transmission electron microscopy observation. Also, the fertilization process is affected by the compound: the damaged spermatozoa are present in the vitelline coat and the egg does not cleave. An increase of microbodies, structurally similar to peroxisomes, have been detected in the egg peripheral cytoplasm, probably in relation to their role in alleviating damage to some cellular components. The results have shown that the reproduction of ascidians under unfavourable environmental conditions is prevented. Copyright © 2003 John Wiley &amp…

Ascidianmedia_common.quotation_subjectgameteanimal cellChloridereproductionInorganic Chemistrychemistry.chemical_compoundGametes and reproductionHuman fertilizationenvironmental factortransmission electron microscopymedicinetributyltin chlorideMicrobodycontrolled studyperoxisomevitelline membranemedia_commonAscidiaceanonhumanbiologyChemistryPeroxisomes proliferationarticleGeneral Chemistrybiology.organism_classificationCell biologycell damagemicrobodyAscidiamedicine.anatomical_structurespermatozoonTributyltin(IV) chlorideChemistry (miscellaneous)fertilizationSettore CHIM/03 - Chimica Generale E InorganicacytoplasmTributyltinGameteoocyte cleavageReproductionAscidiaceacell structuremedicine.drugApplied Organometallic Chemistry
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Mapping research on legacy of mega sporting events: structural changes, consequences, and stakeholder evaluations in empirical studies

2019

Findings from empirical studies on the legacy of hosting a mega sporting event are inconclusive. This paper considers empirical studies published in English language peer-reviewed journals between ...

Asian gamesHistoryEmpirical researchbusiness.industryEvent (computing)Tourism Leisure and Hospitality ManagementGeography Planning and DevelopmentStakeholderEnglish languagePublic relationsbusinessMega-Leisure Studies
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Predicting hospital associated disability from imbalanced data using supervised learning.

2019

Hospitalization of elderly patients can lead to serious adverse effects on their functional capability. Identifying the underlying factors leading to such adverse effects is an active area of medical research. The purpose of the current paper is to show the potential of artificial intelligence in the form of machine learning to complement the existing medical research. This is accomplished by studying the outcome of hospitalization of elderly patients as a supervised learning task. A rich set of features characterizing the medical and social situation of elderly patients is leveraged and using confusion matrices, association rule mining, and two different classes of supervised learning algo…

Association rule learningmedicine.medical_treatmentvanhuksetMedicine (miscellaneous)sairaalahoitoOutcome (game theory)Task (project management)03 medical and health sciences0302 clinical medicineArtificial IntelligenceMedicineHumanstoimintarajoitteetDisabled PersonsSet (psychology)Adverse effectFinlandta316030304 developmental biologyAgedta1130303 health sciencesRehabilitationbusiness.industrySupervised learningennusteetta3142medicine.diseaseMedical researchHospitalizationmachine learningkoneoppiminenhospital associated disabilityMedical emergencySupervised Machine Learningtiedonlouhintabusiness030217 neurology & neurosurgeryrandom forestArtificial intelligence in medicine
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A Standard Siren Measurement of the Hubble Constant from GW170817 without the Electromagnetic Counterpart

2019

We perform a statistical standard siren analysis of GW170817. Our analysis does not utilize knowledge of NGC 4993 as the unique host galaxy of the optical counterpart to GW170817. Instead, we consider each galaxy within the GW170817 localization region as a potential host; combining the redshift from each galaxy with the distance estimate from GW170817 provides an estimate of the Hubble constant, $H_0$. We then combine the $H_0$ values from all the galaxies to provide a final measurement of $H_0$. We explore the dependence of our results on the thresholds by which galaxies are included in our sample, as well as the impact of weighting the galaxies by stellar mass and star-formation rate. Co…

AstrofísicaGravitacióCosmology and Nongalactic Astrophysics (astro-ph.CO)010504 meteorology & atmospheric sciencesStellar massStar (game theory)AstronomyFOS: Physical sciencesPREDICTIONSInterval (mathematics)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & AstrophysicsMASSdistance scale01 natural sciencessymbols.namesake0103 physical sciencesRange (statistics)distance scale; gravitational waves010303 astronomy & astrophysicsgravitational waveAstrophysics::Galaxy AstrophysicsQB0105 earth and related environmental sciencesPhysicsSettore FIS/01Science & TechnologyAstronomy and AstrophysicsAstronomy and AstrophysicRedshiftGalaxyWeightingGALAXIESdistance scale; gravitational waves; Astronomy and Astrophysics; Space and Planetary SciencePhysics and Astronomygravitational wavesSpace and Planetary SciencePhysical Sciencessymbols[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]STARSAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's lawAstrophysical Journal Letters
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CONSTRAINTS ON THE PROGENITOR SYSTEM AND THE ENVIRONS OF SN 2014J FROM DEEP RADIO OBSERVATIONS

2014

We report deep EVN and eMERLIN observations of the Type Ia SN 2014J in the nearby galaxy M 82. Our observations represent, together with JVLA observations of SNe 2011fe and 2014J, the most sensitive radio studies of Type Ia SNe ever. By combining data and a proper modeling of the radio emission, we constrain the mass-loss rate from the progenitor system of SN 2014J to $\dot{M} \lesssim 7.0\times 10^{-10}\, {\rm M_{\odot}\, yr^{-1}}$ (3-$\sigma$; for a wind speed of $100\, {\rm km s^{-1}}$). If the medium around the supernova is uniform, then $n_{\rm ISM} \lesssim 1.3 {\rm cm^3}$ (3-$\sigma$), which is the most stringent limit for the (uniform) density around a Type Ia SN. Our deep upper lim…

AstrofísicaPhysicsSN2014J)Red giantStar (game theory)FOS: Physical sciencesmass-loss [stars]Astronomy and AstrophysicsAstrophysicsType (model theory)Galaxyindividual: SN2011fe SN2014J [Supernovae]SupernovaAstrophysics - Solar and Stellar Astrophysicsindividual (SN2011fe [Supernovae]Space and Planetary ScienceAstronomy Astrophysics and CosmologySolar and Stellar Astrophysics (astro-ph.SR)The Astrophysical Journal
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Magnetorotational Collapse of Supermassive Stars: Black Hole Formation, Gravitational Waves and Jets

2017

We perform MHD simulations in full GR of uniformly rotating stars that are marginally unstable to collapse. Our simulations model the direct collapse of supermassive stars (SMSs) to seed black holes (BHs) that can grow to become the supermassive BHs at the centers of quasars and AGNs. They also crudely model the collapse of massive Pop III stars to BHs, which could power a fraction of distant, long gamma-ray bursts (GRBs). The initial stellar models we adopt are $\Gamma = 4/3$ polytropes seeded with a dynamically unimportant dipole magnetic field (B field). We treat initial B-field configurations either confined to the stellar interior or extending out from the interior into the stellar ext…

AstrofísicaStar (game theory)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)7. Clean energy01 natural sciencesGeneral Relativity and Quantum CosmologyArticleLuminosity0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Supermassive black hole010308 nuclear & particles physicsTorusQuasarRedshiftBlack hole13. Climate actionAstronomiaAstrophysics - High Energy Astrophysical PhenomenaDimensionless quantity
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GW170817, General Relativistic Magnetohydrodynamic Simulations, and the Neutron Star Maximum Mass

2017

Recent numerical simulations in general relativistic magnetohydrodynamics (GRMHD) provide useful constraints for the interpretation of the GW170817 discovery. Combining the observed data with these simulations leads to a bound on the maximum mass of a cold, spherical neutron star (the TOV limit): ${M_{\rm max}^{\rm sph}}\lesssim 2.74/\beta$, where $\beta$ is the ratio of the maximum mass of a uniformly rotating neutron star (the supramassive limit) over the maximum mass of a nonrotating star. Causality arguments allow $\beta$ to be as high as $1.27$, while most realistic candidate equations of state predict $\beta$ to be closer to $1.2$, yielding ${M_{\rm max}^{\rm sph}}$ in the range $2.16…

AstrofísicaStar (game theory)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyArticleInterpretation (model theory)Causality (physics)Quantum mechanics0103 physical sciencesBeta (velocity)Limit (mathematics)Magnetohydrodynamic drive010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsMathematical physicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsNeutron starAstronomiaMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena
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Magnetic Ergostars, Jet Formation and Gamma-Ray Bursts: Ergoregions versus Horizons

2020

We perform the first fully general relativistic, magnetohydrodynamic simulations of dynamically stable hypermassive neutron stars with and without ergoregions to assess the impact of ergoregions on launching magnetically--driven outflows. The hypermassive neutron stars are modeled by a compressible and causal equation of state and are initially endowed with a dipolar magnetic field extending from the stellar interior into its exterior. We find that, after a few Alfv\'en times, magnetic field lines in the ergostar (star that contains ergoregions) and the normal star have been tightly wound in both cases into a helical funnel within which matter begins to flow outward. The maximum Lorentz fac…

AstrofísicaStar (game theory)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyLuminositysymbols.namesakeAstrophysical jet0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsEquation of state (cosmology)Black holeLorentz factorNeutron starsymbolsAstrophysics::Earth and Planetary AstrophysicsGamma-ray burstAstrophysics - High Energy Astrophysical Phenomena
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Discontinuous Gradient Constraints and the Infinity Laplacian

2012

Motivated by tug-of-war games and asymptotic analysis of certain variational problems, we consider a gradient constraint problem involving the infinity Laplace operator. We prove that this problem always has a solution that is unique if a certain regularity condition on the constraint is satisfied. If this regularity condition fails, then solutions obtained from game theory and $L^p$-approximation need not coincide.

Asymptotic analysisGeneral Mathematicsta111010102 general mathematicsMathematical analysisinfinity Laplace operator01 natural sciences010101 applied mathematicsConstraint (information theory)Mathematics - Analysis of PDEsOperator (computer programming)Infinity LaplacianFOS: Mathematics0101 mathematicsGame theorygradient constraint problemsAnalysis of PDEs (math.AP)MathematicsInternational Mathematics Research Notices
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Contribuições e efeitos dos videogames na atenção à diversidade

2021

[Resumen] Este artículo presenta los resultados de una revisión de la literatura sobre estudios centrados en las contribuciones y los efectos de los videojuegos en la atención a la diversidad. Para ello, se tomó como muestra las investigaciones recogidas en las bases de datos Scopus, wos, eric, ProQuest Dissertations & Theses Global (pqdt), Dialnet y csic-isoc y en los buscadores académicos Rebiun, Teseo y ScienceDirect. Después de considerar algunos aspectos del análisis bibliométrico, con el propósito de contextualizar la autoría y la procedencia de los artículos, se procedió a analizar en profundidad el contenido de los documentos seleccionados, de acuerdo con los objetivos de este estud…

Atenção à diversidadeeducationinclusive educationeducação;atenção à diversidadevideojuegoseducação inclusivavideo gamesEducationatención a la diversidadeducación inclusivaattention to diversityEducaçãovideogamesEducacióeducación
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