Search results for " Conduction"

showing 10 items of 373 documents

Hydrodynamic modelling of ejecta shrapnel in the Vela supernova remnant

2013

Many supernova remnants (SNRs) are characterized by a knotty ejecta structure. The Vela SNR is an excellent example of remnant in which detached clumps of ejecta are visible as X-ray emitting bullets that have been observed and studied in great detail. We aim at modelling the evolution of ejecta shrapnel in the Vela SNR, investigating the role of their initial parameters (position and density) and addressing the effects of thermal conduction and radiative losses. We performed a set of 2-D hydrodynamic simulations describing the evolution of a density inhomogeneity in the ejecta profile. We explored different initial setups. We found that the final position of the shrapnel is very sensitive …

PhysicsShock waveHigh Energy Astrophysical Phenomena (astro-ph.HE)Vela Supernova RemnantAstrophysics::High Energy Astrophysical Phenomenanumerical ISM: individual objects: Vela SNR ISM: kinematics and dynamics ISM: supernova remnants [hydrodynamics shock waves methods]AstronomyFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsThermal conductionVelahydrodynamics shock waves methods: numerical ISM: individual objects: Vela SNR ISM: kinematics and dynamics ISM: supernova remnantsSupernovaSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceRadiative transferAstrophysics::Solar and Stellar AstrophysicsDensity contrastEjectaAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy Astrophysics
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Crushing of Interstellar Gas Clouds in Supernova Remnants: the Role of Thermal Conduction and Radiative Losses

2004

We model hydrodynamic interactions of an old supernova remnant shock wave with a small interstellar gas cloud, taking into account the effects of thermal conduction and radiative losses. In particular, we consider a representative case of a Mach 30 shock impacting on an isolated cloud with density contrast χ = 10 with respect to the ambient medium. Thermal conduction appears to be effective in suppressing the Kelvin-Helmholtz and Rayleigh-Taylor instabilities which would develop at the cloud boundaries. We demonstrate that the radiative losses play a crucial role in the dynamics of the shock-cloud interaction, dominating evolution of the shocked cloud medium.

PhysicsShock waveShock (fluid dynamics)Astrophysics::High Energy Astrophysical PhenomenaAstrophysicsThermal conductionSHOCKSEVAPORATIONInterstellar mediumSupernovaSettore FIS/05 - Astronomia E AstrofisicaRadiative transferRayleigh–Taylor instabilitySupernova remnantAstrophysics::Galaxy AstrophysicsAIP Conference Proceedings
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Density Functional Theory of Multicomponent Quantum Dots

2004

Quantum dots with conduction electrons or holes originating from several bands are considered. We assume the particles are confined in a harmonic potential and assume the electrons (or holes) belonging to different bands to be different types of fermions with isotropic effective masses. The density functional method with the local density approximation is used. The increased number of internal (Kohn-Sham) states leads to a generalisation of Hund's first rule at high densities. At low densitites the formation of Wigner molecules is favored by the increased internal freedom.

PhysicsStrongly Correlated Electrons (cond-mat.str-el)Condensed matter physicsCondensed Matter - Mesoscale and Nanoscale PhysicsFOS: Physical sciencesFermionElectronic structureElectronCondensed Matter PhysicsThermal conductionElectronic Optical and Magnetic MaterialsCondensed Matter - Strongly Correlated ElectronsEffective mass (solid-state physics)Quantum dotMesoscale and Nanoscale Physics (cond-mat.mes-hall)Density functional theoryLocal-density approximation
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Nonequilibrium of Ionization and the Detection of Hot Plasma in Nanoflare‐heated Coronal Loops

2008

Impulsive nanoflares are expected to transiently heat the plasma confined in coronal loops to temperatures of the order of 10 MK. Such hot plasma is hardly detected in quiet and active regions, outside flares. During rapid and short heat pulses in rarified loops the plasma can be highly out of equilibrium of ionization. Here we investigate the effects of the non-equilibrium of ionization (NEI) on the detection of hot plasma in coronal loops. Time-dependent loop hydrodynamic simulations are specifically devoted to this task, including saturated thermal conduction, and coupled to the detailed solution of the equations of ionization rate for several abundant elements. In our simulations, initi…

PhysicsSun: Corona Sun: X-Rays Gamma RaysAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsCoronal loopPlasmaAstrophysicsThermal conductionMagnetic fluxNanoflaresPulse (physics)Settore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceIonizationPhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsAtomic physicsThe Astrophysical Journal
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Hydrodynamic Modeling of Accretion Shock on CTTSs

2009

High resolution (R ~ 600) X-ray observations of some classical T Tauri stars (CTTSs) (TW Hya, BP Tau, V4046 Sgr, MP Mus and RU Lupi) have shown the presence of X-ray plasma at T ~ 2–3 × 106 K and denser than n e ~ 1011 cm-3 [1, 2, 3, 4, 5], which suggests an origin different from the coronal one (n e ~ 1010 cm_3). Stationary models demonstrated that X-ray emission from CTTSs could also be produced by the accreting material [6]. We address this issue with the aid of a time-dependent hydrodynamic numerical model describing the impact of an accretion stream onto the chromosphere of a CTTS (see [7] for more details). Our simulations include the effects of gravity, radiative losses from opticall…

PhysicsT Tauri starGravity (chemistry)Settore FIS/05 - Astronomia E AstrofisicaShock (fluid dynamics)Accretion (meteorology)Stars: X-raysStars: coronaRadiative transferAstrophysicsPlasmaThermal conductionChromosphere
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A Ioffe Trap Magnet for the Project 8 Atom Trapping Demonstrator

2020

The goal of the Project 8 experiment (B. Monreal and J. Formaggio, 2009) is to measure the absolute neutrino mass using tritium, which involves precisely measuring the energies of the beta-decay electrons in the high-energy tail of the spectrum (A. A. Esfahani et al. , 2017). The experimental installation of Project 8 Atom Trapping Demonstrator requires a magnet with rather unusual field properties. The magnet has to contain within the cold mass a large volume enclosed by a continuous, uninterrupted boundary higher than 2 T, whereas the field in a substantial volume inside this boundary has to be of the order of 10−4 T or less. A 1-T solenoid field provides the background field necessary fo…

PhysicsToroidMagnetic separationSuperconducting magnetElectronCondensed Matter PhysicsThermal conduction01 natural sciences7. Clean energyElectronic Optical and Magnetic MaterialsElectromagnetic coilMagnet0103 physical sciencesDuct (flow)Electrical and Electronic EngineeringAtomic physics010306 general physics
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MHD evolution of a fragment of a CME core in the outer solar corona

2007

Detailed hydrodynamic modeling explained several features of a fragment of the core of a Coronal Mass Ejection observed with SoHO/UVCS at 1.7 Ro on 12 December 1997, but some questions remained unsolved. We investigate the role of the magnetic fields in the thermal insulation and the expansion of an ejected fragment (cloud) traveling upwards in the outer corona. We perform MHD simulations including the effects of thermal conduction and radiative losses of a dense spherical or cylindrical cloud launched upwards in the outer corona, with various assumptions on the strength and topology of the ambient magnetic field; we also consider the case of a cylindrical cloud with an internal magnetic fi…

Physicsbusiness.industryAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsThermal conductionAstrophysicsCoronaMagnetic fieldSpace and Planetary ScienceThermal insulationBeta (plasma physics)Physics::Space PhysicsRadiative transferCoronal mass ejectionAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamicsbusinessSun: coronal mass ejections (CMEs) – magnetohydrodynamics (MHD) – Sun: corona
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Electric conduction in semiconductors: a pedagogical model based on the Monte Carlo method

2008

We present a pedagogic approach aimed at modelling electric conduction in semiconductors in order to describe and explain some macroscopic properties, such as the characteristic behaviour of resistance as a function of temperature. A simple model of the band structure is adopted for the generation of electron–hole pairs as well as for the carrier transport in moderate electric fields. The semiconductor behaviour is described by substituting the traditional statistical approach (requiring a deep mathematical background) with microscopic models, based on the Monte Carlo method, in which simple rules applied to microscopic particles and quasi-particles determine the macroscopic properties. We …

Physicsbusiness.industryMonte Carlo methodGAASGeneral Physics and AstronomyElectron holeFunction (mathematics)Thermal conductionSemiconductorSimple (abstract algebra)Electric fieldQuasiparticleStatistical physicsDRIFT VELOCITYbusinessSILICON
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Electrical Characterization of CdTe pixel detectors with Al Schottky anode

2014

Abstract Pixelated Schottky Al/p-CdTe/Pt detectors are very attractive devices for high-resolution X-ray spectroscopic imaging, even though they suffer from bias-induced time instability (polarization). In this work, we present the results of the electrical characterization of a (4×4) pixelated Schottky Al/p-CdTe/Pt detector. Current–voltage ( I–V ) characteristics and current transients were investigated at different temperatures. The results show deep levels that play a dominant role in the charge transport mechanism. The conduction mechanism is dominated by the space charge limited current (SCLC) both under forward bias and at high reverse bias. Schottky barrier height of the Al/CdTe con…

PhysicspolarizationNuclear and High Energy PhysicsSchottky contactbusiness.industrySchottky barrierSettore FIS/01 - Fisica SperimentaleSchottky diodeCdTeThermal conductionSpace chargeCadmium telluride photovoltaicsSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Settore FIS/03 - Fisica Della MateriaAnodeX-ray and gamma ray spectroscopypixel detectorOptoelectronicsPolarization (electrochemistry)businessCdTe; Schottky contacts; polarization; pixel detectors; X-ray and gamma ray spectroscopyInstrumentationVoltage
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Thermodynamic pressure in nonlinear nonequilibrium thermodynamics of dilute nonviscous gases.

2000

In this paper, using extended thermodynamics, we build up a nonlinear theory for a dilute nonviscous gas under heat flux. The fundamental fields are the density, the velocity, the internal energy density, and the heat flux. The constitutive theory is builtup without approximations. We single out the nonlinear complete expressions of the Gibbs equation and of the nonequilibrium pressure. In particular, we determine the complete expressions furnished by the theory for the nonequilibrium pressure tensor and thermodynamic pressure, i.e., the derivative of the nonequilibrium internal specific entropy with respect to the specific volume, times the nonequilibrium temperature. In a second-order app…

Physicssymbols.namesakeEntropy (classical thermodynamics)Nonlinear systemInternal energyFundamental thermodynamic relationHeat fluxGibbs–Helmholtz equationsymbolsThermodynamicsNon-equilibrium thermodynamicsThermal conductionPhysical review. E, Statistical, nonlinear, and soft matter physics
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