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1.
Using azimuthally symmetrized cylindrical coordinates, we consider some position-dependent mass (PDM) charged particles moving in position-dependent (PD) magnetic and Aharonov–Bohm flux fields. We focus our attention on PDM-charged particles with m(r)=g(ρ)=ηf(ρ)exp(δρ) (i.e., the PDM is only radially dependent) moving in an inverse power-law-type radial PD-magnetic fields B=B(μ/ρσ)z^. Under such settings, we consider two almost-quasi-free PDM-charged particles (i.e., no interaction potential, V(r)=0) endowed with g(ρ)=η/ρ and g(ρ)=η/ρ2. Both yield exactly solvable Schrödinger equations of Coulombic nature but with different spectroscopic structures. Moreover, we consider a Yukawa-type PDM-charged particle with g(ρ)=ηexp(δρ)/ρ moving not only in the vicinity of the PD-magnetic and Aharonov-Bohm flux fields but also in the vicinity of a Yukawa plus a Kratzer type potential force field V(ρ)=Vexp(δρ)/ρV1/ρ+V2/ρ2. For this particular case, we use the Nikiforov-Uvarov (NU) method to come out with exact analytical eigenvalues and eigenfunctions. Which, in turn, recover those of the almost-quasi-freePDM-charged particle with g(ρ)=η/ρ for V=V1=V2=0=δ. Energy levels crossings are also reported.  相似文献   

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This work is devoted to investigate the structures of compact stars by using spherically static symmetric space-time in the background of f(τ,T) gravity, where τ represents the torsion scalar and T represents the trace of the energy momentum tensor. We develop the field equations by using the concept of quintessence to discuss the motion by using anisotropic fluid distribution with a spherically symmetric metric. We use the convention of junction conditions to evaluate the unknown parameters used in the study of the compact stars. In this study we use the available data of three different compact objects 4U160852, CenX3 and EXO1785240. We discuss the physical and analytical existence of compact stars by satisfying some standard properties of compact stars like the behavior of the energy density, quintessence density, radial and tangential pressures, anisotropy, to elaborate the anisotropic nature of the star. We discuss the sound speeds and casuality conditions to show the stability of the system. Equilibrium of the star is justified by the TOV equation. Red-shift function, compactness, and mass function states the physical existence of the star. It is examined that all these parameters show the viability and stability of the model used in the effects of f(τ,T) gravity.  相似文献   

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The interactions between cool flames and flames with repetitive extinction and ignition (FREI) of stoichiometric n-heptane/air mixture were studied using a micro flow reactor with a controlled temperature profile from 373 to 1300 K. Two different flame dynamics with and without cool flames were observed in reactors with inner diameters dinner of 1 and 2 mm. Cool flames and FREI are spatially separated at dinner= 1 mm, whereas interactions between cool flames and FREI are observed at dinner= 2 mm. At dinner= 1 mm, the brightness intensity from cool flames depends on the inlet velocity (uinlet). Approximately above uinlet= 10 cm/s, the brightness intensity from cool flames decreases with increasing inlet velocity, despite a large amount of mixture input. This is because before low temperature ignition occurs under higher inlet velocity conditions, the mixture archives temperature where negative temperature coefficient is dominant. Reaction front propagation speed of FREI decreases monotonically due to heat loss because the extinction points of FREI are located in higher temperatures than the cool flame region. At dinner= 2 mm, the acceleration of the reaction front in the cool flame region is confirmed experimentally, as predicted in our previous two-dimensional numerical simulations. Additionally, the instantaneous reaction front speed after autoignition is analyzed at dinner= 1 mm. The instantaneous reaction front speed decreases as the time from extinction to ignition tex_ig becomes longer because a moderate mixing zone of reactants and products is formed.  相似文献   

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《Physics letters. A》2020,384(35):126893
Here, the thermoelectric (TE) properties of Na0.74Co1xNbxO2 (x=0.05,0.10) compounds are investigated experimentally and computationally. The experimental measurements are conducted in 300620 K. Positive sign of Seebeck coefficient for both the compounds indicates the dominating p-type character. The maximum experimental values of ZT are observed as ∼ 0.12 and ∼ 0.19 at 620 K for x=0.05 and x=0.10, respectively. The experimental transport properties of these compounds are understood by employing spin-polarized GGA+U (= 4 eV) electronic structure calculations on x=0.0625 compound. On the basis of best experimental and computational matching of transport properties, we have estimated ZT till 1200 K computationally. The highest calculated values of ZT are ∼ 1.36 and ∼ 1.22 at 1200 K for x=0.05 and x=0.10, respectively. The optimum value of efficiency for x=0.05 is calculated as ∼ 6.4%, whereas it reaches ∼ 7.5% for x=0.10.  相似文献   

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In a recent paper, we theoretically investigated the density of states of the composite channel–contact system in the Coulomb and Kondo regimes using the self-consistent field approximation. There are the main experimental observations of vibration features in the Coulomb blockade [H. Park et al., Nature (London) 407, 57 (2000)] and Kondo [L. H. Yu et al., Phys. Rev. Lett. 93, 266802 (2004)] regimes. In the Kondo regime, our results show that one peak at E=μ can be observed in the density of states at low temperatures (0.0026 eV ≤ kBT ≤ 0.0000026 eV). Also, the real part of ∑3 has one minimum peak at E=μ and the real par of ∑2 has one maximum peak at E=μ for 0.01 ≤ μ ≤ 0.07 in the Kondo regime at low temperatures.  相似文献   

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With the help of the nonequilibrium Green's function technique, we theoretically analyze the thermospin property through a typical T-shaped spin valve with spin-flip scattering in the linear regime. The influences of spin-flip coefficient of interdot λ, spin-flip coefficient of intradot η and interdot hopping coefficient t+δσΔt on thermospin property are discussed. As interdot hopping coefficient t is equal to energy level ε, the spectrum of Gs shows Fano-like effect with ε variation. Antiresonance position of Gs is almost unchanged and its width becomes narrower with ε increasing. Spin thermopower Ss is close to the maximum of the peak and charge thermopower Sc is equal to zero for t=ε. As a result, the pure spin thermopower Ss can be obtained, which means that a pure spin current may be produced by a temperature gradient in our system. It is found that spin figure of merit ZTs can reach a considerable value by adjusting key parameters of the system, such as Δt, β, α, ?. The typical T-shaped spin valve can be treated as a stable thermospin battery which allows to convert the heat energy to spin voltage, thus produces the pure spin current in the device.  相似文献   

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《Physics letters. A》2019,383(22):2652-2657
The equilibrated grain boundary groove shape of solid Al in equilibrium with Al-Sn-Mg eutectic liquid was observed by using a Bridgman type directional solidification apparatus. The ratio of the thermal conductivity of the equilibrated liquid to the thermal conductivity of solid Al has been obtained as 0.91. In addition, the average Gibbs-Thomson coefficient, Γ=(4.20±0.35)×108Km, the solid-liquid interfacial energy, σSL=180.68±23.48mJ/m2 and the grain boundary energy, σGB=309.30±29.47mJ/m2, in the Al/Al-Sn-Mg system have been calculated from the measured grain boundary shapes.  相似文献   

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《Physics letters. A》2020,384(13):126265
The exact solvability and impressive pedagogical implementation of the harmonic oscillator's creation and annihilation operators make it a problem of great physical relevance and the most fundamental one in quantum mechanics. So would be the position-dependent mass (PDM) oscillator for the PDM quantum mechanics. We, hereby, construct the PDM creation and annihilation operators for the PDM oscillator via two different approaches. First, via von Roos PDM Hamiltonian and show that the commutation relation between the PDM creation Aˆ+ and annihilation Aˆ operators, [Aˆ,Aˆ+]=1AˆAˆ+1/2=Aˆ+Aˆ+1/2, not only offers a unique PDM-Hamiltonian Hˆ1 but also suggests a PDM-deformation in the coordinate system. Next, we use a PDM point canonical transformation of the textbook constant mass harmonic oscillator analog and obtain yet another set of PDM creation Bˆ+ and annihilation Bˆ operators, hence an “apparently new” PDM-Hamiltonian Hˆ2 is obtained. The “new” PDM-Hamiltonian Hˆ2 turned out to be not only correlated with Hˆ1 but also represents an alternative and most simplistic user-friendly PDM-Hamiltonian, Hˆ=(pˆ/2m(x))2+V(x); pˆ=iħx, that has never been reported before.  相似文献   

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