Search results for "Velocity"

showing 10 items of 881 documents

Dynamical efficiency of collisionless magnetized shocks in relativistic jets

2010

The so-called internal shock model aims to explain the light-curves and spectra produced by non-thermal processes originated in the flow of blazars and gamma-ray bursts. A long standing question is whether the tenuous collisionless shocks, driven inside a relativistic flow, are efficient enough to explain the amount of energy observed as compared with the expected kinetic power of the outflow. In this work we study the dynamic efficiency of conversion of kinetic-to- thermal/magnetic energy of internal shocks in relativistic magnetized outflows. We find that the collision between shells with a non-zero relative velocity can yield either two oppositely moving shocks (in the frame where the co…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsShock waveShock (fluid dynamics)Magnetic energyAstrophysics::High Energy Astrophysical PhenomenaRelative velocityFOS: Physical sciencesRarefaction020206 networking & telecommunications02 engineering and technologyKinetic energyComputational physicsAstrophysical jet0202 electrical engineering electronic engineering information engineering020201 artificial intelligence & image processingAstrophysics - High Energy Astrophysical PhenomenaBlazarAstrophysics::Galaxy AstrophysicsAIP Conference Proceedings
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NuSTARandXMM–Newtonbroad-band spectrum of SAX J1808.4–3658 during its latest outburst in 2015

2018

The first discovered accreting millisecond pulsar, SAX J1808.4-3658, went into X-ray outburst in April 2015. We triggered a 100 ks XMM-Newton ToO, taken at the peak of the outburst, and a 55 ks NuSTAR ToO, performed four days apart. We report here the results of a detailed spectral analysis of both the XMM-Newton and NuSTAR spectra. While the XMM-Newton spectrum appears much softer than in previous observations, the NuSTAR spectrum confirms the results obtained with XMM-Newton during the 2008 outburst. We find clear evidence of a broad iron line that we interpret as produced by reflection from the inner accretion disk. For the first time, we use a self-consistent reflection model to fit the…

High Energy Astrophysical Phenomena (astro-ph.HE)line: formation line: identification stars: individual: SAX J1808.4-3658 stars: magnetic fields stars: neutron X-rays: binaries X-rays: generalPhysics010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesBroad bandAstronomy and AstrophysicsAstrophysics01 natural sciencesSpectral lineRadial velocityNeutron starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceMillisecond pulsarInclination angle0103 physical sciencesSpectral analysisAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsLine (formation)Monthly Notices of the Royal Astronomical Society
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Limits on neutrino Lorentz violation from multimessenger observations of TXS 0506+056

2019

The observation by the IceCube Collaboration of a high-energy ($E \gtrsim 200$ TeV) neutrino from the direction of the blazar TXS 0506+056 and the coincident observations of enhanced $\gamma$-ray emissions from the same object by MAGIC and other experiments can be used to set stringent constraints on Lorentz violation in the propagation of neutrinos that is linear in the neutrino energy: $\Delta v = - E/M_1$, where $\Delta v$ is the deviation from the velocity of light, and $M_1$ is an unknown high energy scale to be constrained by experiment. Allowing for a difference in neutrino and photon propagation times of $\sim 10$ days, we find that $M_1 \gtrsim 3 \times 10^{16}$ GeV. This improves …

High Energy Physics - TheoryNuclear and High Energy PhysicsHigh energyParticle physicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)Lorentz transformationgr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesComputer Science::Digital LibrariesGeneral Relativity and Quantum CosmologyIceCubesymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Coincident0103 physical sciences010306 general physicsBlazarParticle Physics - PhenomenologyHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEMultimessenger010308 nuclear & particles physicsGeneral Relativity and Cosmologyhep-thHigh Energy Physics::PhenomenologyLorentz violationGamma rayhep-phlcsh:QC1-999High Energy Physics - PhenomenologyPhoton propagationHigh Energy Physics - Theory (hep-th)Astrophysical neutrinosVelocity of lightsymbolsastro-ph.COHigh Energy Physics::ExperimentNeutrinoTXS 0506+056Astrophysics - High Energy Astrophysical PhenomenaParticle Physics - Theorylcsh:PhysicsBlazarsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysics Letters
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Gauge and Yukawa unification with broken R-parity

1998

We study gauge and Yukawa coupling unification in the simplest extension of the Minimal Supersymmetric Standard Model (MSSM) which incorporates R-Parity violation through a bilinear superpotential term. Contrary to what happens in the MSSM, we show that bottom-tau unification at the scale M_GUT where the gauge couplings unify can be achieved for any value of tan(beta) by choosing appropriately the sneutrino vacuum expectation value. In addition, we show that bottom-tau-top unification occurs in a slightly wider tan(beta) range than in the MSSM.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsParticle physicsUnificationHigh Energy Physics::PhenomenologySuperpotentialYukawa potentialFOS: Physical sciencesFísicaGauge (firearms)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)R-parityHigh Energy Physics::ExperimentBeta (velocity)Vacuum expectation valueMinimal Supersymmetric Standard ModelPhysics Letters B
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Quantum Backreaction on Three-Dimensional Black Holes and Naked Singularities

2016

We analytically investigate backreaction by a quantum scalar field on two rotating Ba\~nados-Teitelboim-Zanelli (BTZ) geometries: that of a black hole and that of a naked singularity. In the former case, we explore the quantum effects on various regions of relevance for a rotating black hole space-time. We find that the quantum effects lead to a growth of both the event horizon and the radius of the ergosphere, and to a reduction of the angular velocity, compared to the unperturbed values. Furthermore, they give rise to the formation of a curvature singularity at the Cauchy horizon and show no evidence of the appearance of a superradiant instability. In the case of a naked singularity, we f…

High Energy Physics - Theoryblack hole: rotationeffect: quantumvelocitysemiclassicalEvent horizonperturbationspace-time: black holeGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)angular momentum01 natural sciencesErgospherePenrose processGeneral Relativity and Quantum Cosmologyhorizon[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc][ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]black hole: BTZGeneral Relativity and Quantum CosmologyQuantum mechanics0103 physical sciencescurvature: singularity010306 general physicsRing singularityPhysics010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]formationNaked singularitycoupling: conformalstabilityfield theory: scalarBlack holeClassical mechanicsHigh Energy Physics - Theory (hep-th)Apparent horizonback reaction: quantum[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]massGravitational singularitysuperradianceblack hole: geometry
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On gravitational waves in Born-Infeld inspired non-singular cosmologies

2017

We study the evolution of gravitational waves for non-singular cosmological solutions within the framework of Born-Infeld inspired gravity theories, with special emphasis on the Eddington-inspired Born-Infeld theory. We review the existence of two types of non-singular cosmologies, namely bouncing and asymptotically Minkowski solutions, from a perspective that makes their features more apparent. We study in detail the propagation of gravitational waves near these non-singular solutions and carefully discuss the origin and severity of the instabilities and strong coupling problems that appear. We also investigate the role of the adiabatic sound speed of the matter sector in the regularisatio…

High Energy Physics - Theorycosmological modelCosmology and Nongalactic Astrophysics (astro-ph.CO)[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmology[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th][ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]GravitationTheoretical physicsGeneral Relativity and Quantum CosmologyBorn–Infeld modelgravitational radiation: propagation0103 physical sciencesMinkowski spacestrong couplingphysics of the early universeMinkowski010306 general physicsAdiabatic processmodified gravityPhysics010308 nuclear & particles physicsGravitational waveNon singular[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Astronomy and Astrophysicsalternatives to inflationstabilityvelocity: acousticBorn-Infeld modelregularizationHigh Energy Physics - Theory (hep-th)gravitationRegularization (physics)adiabaticStrong coupling[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]primordial gravitational waves (theory)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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Modélisation numérique d’impacts à hautes vitesses par la méthode sans maillage Smoothed Particles Hydrodynamics. Application aux micro-impacts dans …

2021

Investigations on the ballistic behaviours of soft tissue materials are significant research in a medical and pharmaceutical framework. They mainly focus on particles penetrating or traveling into the soft materials. For instance, in the needle-free drug delivery, the micro-scale particles as drug powders are injected into skin with high velocity, and several factors should be considered such as the particle diameters, trajectories, and momentum or velocities of projectile in this process. There have been investigated by some experiments, but there is still no study from the numerical insights.The numerical methods are suitable to study these kinds of processes. Although grid-based methods …

High-Velocity impact[SPI.OTHER]Engineering Sciences [physics]/OtherMicro-Impacts[SPI.OTHER] Engineering Sciences [physics]/OtherTissus mousImpact à hautes vitesseSoft tissuesSmoothed Particles HydrodynamicsPénétrations à micro-Échelle
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Large eddy simulations on the effect of the irregular roughness shape on turbulent channel flows

2019

Abstract Large Eddy Simulations (LES) are carried out to investigate on the mean flow in turbulent channel flows over irregular rough surfaces. Here the attention is focused to selectively investigate on the effect induced by crests or cavities of the roughness. The irregular shape is generated through the super-imposition of sinusoidal functions having random amplitude and four different wave-lengths. The irregular roughness profile is reproduced along the spanwise direction in order to obtain a 2D rough shape. The analysis of the mean velocity profiles shows that roughness crests induce higher effect in the outer-region whereas roughness cavities cause the highest effects in the inner-reg…

Higher order statisticMaterials scienceTurbulence simulationTurbulent channel flows Large eddy simulation02 engineering and technologyReynolds stressSurface finish01 natural sciencesReynolds numberSettore ICAR/01 - Idraulica010305 fluids & plasmasPhysics::Fluid Dynamicssymbols.namesake0203 mechanical engineering0103 physical sciencesMean flowReynolds equationAnisotropyChannel flowFluid Flow and Transfer ProcessesTurbulenceMean velocity profileMechanical EngineeringIrregular roughneReynolds numberSinusoidal functionMechanicsCondensed Matter PhysicsOpen-channel flowShear stre020303 mechanical engineering & transportsAmplitudeReynolds streTurbulence Irregular shapeTurbulence intensityLESsymbolsTurbulence modulationInternational Journal of Heat and Fluid Flow
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Dry deposition models for radionuclides dispersed in air: a new approach for deposition velocity evaluation schema

2017

In the framework of a National Research Program funded by the Italian Minister of Economic Development, the Department of Energy, Information Engineering and Mathematical Models (DEIM) of Palermo University and ENEA Research Centre of Bologna, Italy is performing several research activities to study physical models and mathematical approaches aimed at investigating dry deposition mechanisms of radioactive pollutants. On the basis of such studies, a new approach to evaluate the dry deposition velocity for particles is proposed. Comparisons with literature experimental data show that the proposed dry deposition scheme allows to capture the main phenomena involved in the dry deposition process…

HistoryRadionuclidePhysical model010504 meteorology & atmospheric sciencesMathematical modelbusiness.industryChemistryMechanical engineering01 natural sciences010305 fluids & plasmasComputer Science ApplicationsEducationResearch centreDry deposition pollutant radionuclides deposition velocity0103 physical sciencesProcess engineeringbusinessSettore ING-IND/19 - Impianti Nucleari0105 earth and related environmental sciencesJournal of Physics: Conference Series
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Dry deposition of particle on urban areas

2019

Abstract Dry deposition process is recognized as an important pathway among the removal processes of radioactive pollutants in atmosphere. There is not a unique and accepted theoretical description of involved dry deposition phenomena due to the complexity of the fluid-dynamic processes that influence the deposition flux, but also because there is a lack of experimental data covering all scenarios of interest. In this paper, that is the result of a National Research Program a research activity conducted by DEIM Department of the University of Palermo and ENEA and funded by the Italian Minister of Economic Development, a new schema for parameterization of particle dry deposition velocity on …

HistorygeographyDry deposition velocity air pollution urban areasparticle depositiongeography.geographical_feature_categoryDeposition (aerosol physics)Environmental engineeringEnvironmental scienceUrban areaSettore ING-IND/19 - Impianti NucleariComputer Science ApplicationsEducationParticle depositionJournal of Physics: Conference Series
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