共查询到20条相似文献,搜索用时 15 毫秒
1.
We directly use the quantum-invariant operator method to obtain the closed-form solution to the one-dimensional Dirac equation with a time-changing mass with a little manipulation. The solution got is also applicable forthe case with time-independence mass. 相似文献
2.
Akpan N.Ikot 《理论物理通讯》2013,59(3):268-272
We employ the parametric generalization of the Nikiforov-Uvarov method to solve the Alhaidari formalism of the Dirac equation with a generalized Hylleraas potential of the form V(r) = V0(a+exp(λr))/(b+ exp(λr)) + V1(d+exp(λr))/(b+exp(λr)).We obtain the bound state energy eigenvalue and the corresponding eigenfunction expressed in terms of the Jacobi polynomials.By choosing appropriate parameter in the potential model,the generalized Hylleraas potential reduces to the well known potentials as special cases. 相似文献
3.
We propose a new exactly solvable potential which is formed by modified Kratzer potential plus a new ring-shaped potential η cot2θ/r2. The solutions of the Dirac equation with equal scalar and vector ring-shaped modified Kratzer potential are found by using the Nikiforov-Uvarov method. The nonrelativistic limit of the energy spectrum has been discussed. 相似文献
4.
CHENG Yan-Fu DAI Tong-Qing 《理论物理通讯》2007,48(3):431-434
We propose a new exactly solvable potential which is Formed by modified Kratzer potential plus a new ring-shaped potential η cot^2 θ/r^2 The solutions of the Dirac equation with equal scalar and vector ring-shaped modified Kratzer potential are found by using the Nikiforov-Uvarov method. The nonrelativistic limit of the energy spectrum has been discussed. 相似文献
5.
In this paper the one-dimensional Dirac equation with linear
potential has been solved by the method of canonical transformation.
The bound-state wavefunctions and the corresponding energy spectrum
have been obtained for all bound states. 相似文献
6.
Antonio Zecca 《International Journal of Theoretical Physics》2002,41(3):421-428
The Dirac equation in a curved space–time endowed with compatible affine connection is reconsidered. After a detailed decomposition of the total action, the equation is obtained by varying with respect to the Dirac spinor and the torsion field. The result is a known Dirac-like equation with constraints that can be interpreted as the equation of a self-interacting spin 1/2 particle in curved space–time. The scheme is then translated into the language of the 2-spinor formalism of curved space–time based on the choice of a null tetrad frame. The spinorial equation so obtained coincides with the standard one in case of no torsion, while in general it remains a nonlinear equation describing a self-interacting spin 1/2 particle. The nonlinearity is produced by the interaction of the particle with its own current that remains conserved as in the free torsion case. 相似文献
7.
The energy eigenvalues of a Dirac particle for the hyperbolic-type potential field have been computed approximately. It is obtained a transcendental function of energy, F(E), by writing in terms of confluent Heun functions. The numerical values of energy are then obtained by fixing the zeros on "E-axis" for both complex functions Re[F(E)] and Im[F(E)]. 相似文献
8.
In this work, the time-dependent Dirac equation is investigated under generalized uncertainty principle(GUP) framework. It is possible to construct the exact solutions of Dirac equation when the time-dependent potentials satisfied the proper conditions. In(1+1) dimensions, the analytical wave functions of the Dirac equation under GUP have been obtained for the two kinds time-dependent potentials. 相似文献
9.
Antonio Zecca 《International Journal of Theoretical Physics》2006,45(1):44-52
Exact solutions of the Dirac equation in the Robertson–Walker space-time are obtained by an elementary separation method that represents a straightforward improvement of previous results. The radial equations are integrated by reporting them to hypergeometric equations. The separated time equations are solved exactly for three models of universe expansion and integrated by series in a case of the standard cosmological model. The integration of both radial and time equations represents an improvement of previous results. 相似文献
10.
In the present paper, we solve the radial parts of Dirac equation between the inner and the outer horizon in the Schwarzschild-de
Sitter (SdS for short) geometry. Complete physical parameter space is divided into two regions depending on the height of
the potential barrier and the energy of the incoming particle. In each region, we concentrate on two limiting cases. The first
case is when the two horizons are close to each other and the second case is when the horizons are far apart. In each case,
we give the semi-analytical solution by using WKB (Wentzel-Krames-Brillouin) approximation and show the instantaneous reflection
and transmission coefficients as well as the radial wave functions graphically.
PACS: 04.20.-q, 04.70.-s, 04.70.Dy, 95.30.Sf 相似文献
11.
12.
We prove that the absolutely continuous spectrum of Dirac operators on the half-line with square integrable potentials fills the whole real axis. We also establish an estimate on the number of eigenvalues for Coulomb-like potentials. 相似文献
13.
The pseudospin symmetry in the Makarov potential is investigated systematically by solving the Dirac equation. The analytical solution for the Makarov potential with pseudospin symmetry is obtained by Nikiforov-Uvarov (N-U) method. The eigenfunctions and eigenenergies are presented with equal mixture of vector and scalar potentials in opposite signs, for which is exact. 相似文献
14.
The Dirac equation is solved for Killingbeck potential. Under spin symmetry limit, the energy eigenvalues and the corresponding wave functions are obtained by using wave function ansatz method. 相似文献
15.
The pseudospin symmetry in the Makarov potential is investigated systematically by solving the Dirac equation. The analytical solution forthe Makarov potential with pseudospin symmetry is obtained byNikiforov-Uvarov (N-U) method. The eigenfunctions and eigenenergies arepresented with equal mixture of vector and scalar potentials in oppositesigns, for which is exact. 相似文献
16.
JU Guo-Xing REN Zhong-Zhou 《理论物理通讯》2008,49(2):319-326
The Dirac equations with vector and scalar potentials of the Coulomb types in two and three dimensions are solved using the supersymmetric quantum mechanics method. For the system of such potentials, the analytical expressions of the matrix dements for both position and momentum operators are obtained. 相似文献
17.
I. Sakalli 《General Relativity and Gravitation》2003,35(8):1321-1335
The Dirac equation is considered in the uniform electromagnetic field space of Bertotti-Robinson with charge coupling. The methods of separation of variables and decoupling are easily achieved. The separated axial equation is reduced to a rare Riccati type of differential equation. The behaviour of potentials, their asymptotic solutions and the conserved currents of the Dirac equation are found. 相似文献
18.
Yaming Chen Songhe Song & Huajun Zhu 《advances in applied mathematics and mechanics.》2014,6(4):494-514
In this paper, we propose two new explicit multi-symplectic splitting methods for the nonlinear Dirac (NLD) equation.
Based on its multi-symplectic formulation, the NLD equation is split into one linear multi-symplectic system and
one nonlinear infinite Hamiltonian system. Then multi-symplectic Fourier pseudospectral method and multi-symplectic Preissmann scheme are employed to discretize the linear subproblem, respectively. And the nonlinear subsystem is solved by a symplectic scheme. Finally, a composition method is applied to obtain the final schemes for the NLD equation. We find that the two proposed schemes preserve the total symplecticity and can be solved explicitly. Numerical experiments are presented to show the effectiveness of the proposed methods. 相似文献
19.
20.
Shahpoor Moradi 《International Journal of Theoretical Physics》2009,48(4):969-980
The exact solutions of the Dirac equation are discussed for a Robertson-Walker spacetime with asymptotically Minkowskian in and out regions. We obtain the mode solutions which reduce to positive and negative Minkowskian spinors in asymptotically regions.
Using the obtained solutions we compute the density of created particles. 相似文献