Search results for "PPAR"

showing 10 items of 1686 documents

An inquiry-based approach to Maxwell distribution: a case study with engineering students

2013

The concept of distribution is a fundamental component of statistical thinking. This paper describes a teaching approach for it that uses a specific activity related to the field of statistical mechanics. The concept of the velocity distribution of a particle system is dealt with using an inquiry-based approach involving an experimental examination of Maxwell’s distribution. Some outcomes of a teaching experiment held at the Faculty of Engineering of the University of Palermo, Italy are described.

PhysicsDistribution (number theory)Research in physics education Teaching methods and strategies Laboratory experiments and apparatus Laboratory course design organization and evaluationClassical statistical mechanicsSettore FIS/08 - Didattica E Storia Della Fisica05 social sciences050301 educationGeneral Physics and AstronomyStatistical mechanics01 natural sciencesMaxwell–Boltzmann distributionField (geography)symbols.namesakeTheoretical physicsStatistical thinkingComponent (UML)0103 physical sciencessymbolsMathematics education010306 general physics0503 educationEuropean Journal of Physics
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THREE-DIMENSIONAL RELATIVISTIC SIMULATIONS OF ROTATING NEUTRON-STAR COLLAPSE TO A KERR BLACK HOLE

2006

We present a new three-dimensional fully general-relativistic hydrodynamics code using high-resolution shock-capturing techniques and a conformal traceless formulation of the Einstein equations. Besides presenting a thorough set of tests which the code passes with very high accuracy, we discuss its application to the study of the gravitational collapse of uniformly rotating neutron stars to Kerr black holes. The initial stellar models are modeled as relativistic polytropes which are either secularly or dynamically unstable and with angular velocities which range from slow rotation to the mass-shedding limit. We investigate the gravitational collapse by carefully studying not only the dynami…

PhysicsGeneral Relativity and Quantum CosmologyAngular momentumNeutron starClassical mechanicsDynamical horizonRotating black holeEvent horizonAstrophysics::High Energy Astrophysical PhenomenaApparent horizonGravitational collapseDifferential rotation
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General Relativistic Simulations of the Collapsar Scenario

2013

We are exploring the viability of the collapsar model for long-soft gamma-ray bursts. For this we perform state-of-the-art general relativistic hydrodynamic simulations in a dynamically evolving space-time with the CoCoNuT code. We start from massive low metallicity stellar models evolved up to core gravitational instability, and then follow the subsequent evolution until the system collapses forming a compact remnant. A preliminary study of the collapse outcome is performed by varying the typical parameters of the scenario, such as the initial stellar mass, metallicity, and rotational profile of the stellar progenitor. 1D models (without rotation) have been used to test our newly developed…

PhysicsGravitational instabilityStellar mass010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaMetallicityAstronomyAstrophysics01 natural sciencesSupernovaNeutron starApparent horizonMetastability0103 physical sciencesNeutrino010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsProgress in Mathematical Relativity. Proc. of Spanish Relativity Meeting 2012. Springer Verlag.
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Seeing Double:ASASSN-18bt Exhibits a Two-Component Rise in the Early-Time K2 Light Curve

2018

On 2018 Feb. 4.41, the All-Sky Automated Survey for SuperNovae (ASAS-SN) discovered ASASSN-18bt in the K2 Campaign 16 field. With a redshift of z=0.01098 and a peak apparent magnitude of B_{max}=14.31, ASASSN-18bt is the nearest and brightest SNe Ia yet observed by the Kepler spacecraft. Here we present the discovery of ASASSN-18bt, the K2 light curve, and pre-discovery data from ASAS-SN and the Asteroid Terrestrial-impact Last Alert System (ATLAS). The K2 early-time light curve has an unprecedented 30-minute cadence and photometric precision for an SN~Ia light curve, and it unambiguously shows a ~4 day nearly linear phase followed by a steeper rise. Thus, ASASSN-18bt joins a growing list o…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Field (physics)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsRadiusindividual (ASASSN-18bt SN 2018oh) [supernovae]Light curve01 natural sciencesPower lawRedshiftSupernovaApparent magnitude13. Climate actionSpace and Planetary ScienceAsteroid0103 physical sciencesQD010306 general physicsAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsQCQB
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Measuring the black hole spin direction in 3D Cartesian numerical relativity simulations

2015

We show that the so-called flat-space rotational Killing vector method for measuring the Cartesian components of a black hole spin can be derived from the surface integral of Weinberg's pseudotensor over the apparent horizon surface when using Gaussian normal coordinates in the integration. Moreover, the integration of the pseudotensor in this gauge yields the Komar angular momentum integral in a foliation adapted to the axisymmetry of the spacetime. As a result, the method does not explicitly depend on the evolved lapse $\ensuremath{\alpha}$ and shift ${\ensuremath{\beta}}^{i}$ on the respective time slice, as they are fixed to Gaussian normal coordinates while leaving the coordinate label…

PhysicsNuclear and High Energy PhysicsAngular momentumSurface integralFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyPseudotensorGeneral Relativity and Quantum CosmologyNumerical relativityKilling vector fieldQuantum mechanicsApparent horizonNormal coordinatesGauge fixingPhysical Review D
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Three-dimensional relativistic simulations of rotating neutron-star collapse to a Kerr black hole

2004

We present a new three-dimensional fully general-relativistic hydrodynamics code using high-resolution shock-capturing techniques and a conformal traceless formulation of the Einstein equations. Besides presenting a thorough set of tests which the code passes with very high accuracy, we discuss its application to the study of the gravitational collapse of uniformly rotating neutron stars to Kerr black holes. The initial stellar models are modelled as relativistic polytropes which are either secularly or dynamically unstable and with angular velocities which range from slow rotation to the mass-shedding limit. We investigate the gravitational collapse by carefully studying not only the dynam…

PhysicsNuclear and High Energy PhysicsEvent horizonAstrophysics::High Energy Astrophysical PhenomenaWhite holeAstrophysics (astro-ph)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsGeneral Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum CosmologyNumerical relativityNeutron starClassical mechanicsRotating black holeApparent horizonGravitational collapsePhysical Review D
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Spacetime Foam Model of the Schwarzschild Horizon

2003

We consider a spacetime foam model of the Schwarzschild horizon, where the horizon consists of Planck size black holes. According to our model the entropy of the Schwarzschild black hole is proportional to the area of its event horizon. It is possible to express geometrical arguments to the effect that the constant of proportionality is, in natural units, equal to one quarter.

PhysicsNuclear and High Energy PhysicsPhysics::General PhysicsEvent horizonAstrophysics::High Energy Astrophysical PhenomenaKerr metricFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)FuzzballPhoton sphereGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyClassical mechanicsApparent horizonDeriving the Schwarzschild solutionSchwarzschild radiusMathematical physicsHawking radiation
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A pedagogical approach to the Boltzmann factor through experiments and simulations

2009

The Boltzmann factor is the basis of a huge amount of thermodynamic and statistical physics, both classical and quantum. It governs the behaviour of all systems in nature that are exchanging energy with their environment. To understand why the expression has this specific form involves a deep mathematical analysis, whose flow of logic is hard to see and is not at the level of high school or college students' preparation. We here present some experiments and simulations aimed at directly deriving its mathematical expression and illustrating the fundamental concepts on which it is grounded. Experiments use easily available apparatuses, and simulations are developed in the Net-Logo environment…

PhysicsScience instructionBasis (linear algebra)Interface (Java)Settore FIS/08 - Didattica E Storia Della FisicaPhysics::Physics EducationGeneral Physics and AstronomyStatistical mechanicsComputer in educationLaboratory experiments and apparatusBoltzmann distributionExpression (mathematics)Teaching methods and strategieEducationFlow (mathematics)ComputingMilieux_COMPUTERSANDEDUCATIONStatistical physicsQuantum
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Two experiments to approach the Boltzmann factor: chemical reaction and viscous flow

2012

In this paper we discuss a pedagogical approach aimed at pointing out the role played by the Boltzmann factor in describing phenomena usually perceived as regulated by different mechanisms of functioning. Experimental results regarding some aspects of a chemical reaction and of the viscous flow of some liquids are analysed and described in terms of macroscopic variables whose temperature dependence is proportional to the Boltzmann factor. A description of a workshop implementing the approach in the framework of an undergraduate course for engineering education and some preliminary results about its pedagogical relevance are then reported.

PhysicsScience instructionSettore FIS/08 - Didattica E Storia Della Fisica05 social sciencesMaxwell–Boltzmann statisticsViscosity of liquidPhysics::Physics Education050301 educationGeneral Physics and Astronomy01 natural sciencesChemical reactionRate constantLaboratory experiments and apparatusBoltzmann distributionTheoretical physics0103 physical sciencesViscous flowFluid dynamicsActivation energyStatistical physicsBoltzmann factor010306 general physics0503 education
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Status of the EPIC thin and medium filters on-board XMM-Newton after more than 10 years of operation II: analysis of in-flight data

2013

After more than ten years of operation of the EPIC camera on board the X-ray observatory XMM-Newton we have reviewed the status of its thin and medium filters by performing both analysis of data collected in-flight and laboratory measurements on on-ground back-up filters. We have investigated the status of the EPIC thin and medium filters by performing an analysis of the optical loading in the PN offset maps to gauge variations in the optical and UV transmission of the filters. We both investigated repeated observations of single optically bright targets and performed a statistical analysis of the extent of loading versus visual magnitude at different epochs. We report the results of these …

Physicsgenetic structuresbusiness.industryAstrophysics::High Energy Astrophysical PhenomenaX-Rays: XMM-Newton - X-rays: instrumentation - X-rays: filtersEPICXMM-Newton - X-rays: instrumentation - X-rays: filters [X-Rays]eye diseasesOn boardOpticsApparent magnitudeSettore FIS/05 - Astronomia E AstrofisicaTransmission (telecommunications)ObservatoryData analysisStatistical analysissense organsbusinessFlight data
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