Abstract:In this article, we study the DKP equation for the oscillator in a Gödel-type space-time background. We derive the final form of this equation in a flat class of Gödel-type space-time and solve it analytically, and evaluate the eigenvalues and corresponding eigenfunctions, in detail.
“…A particularly simple Type D metric has recently examined a member of a linear class of Gödel-type metrics [5]. Previously, relativistic quantum motion of spin-0 particle without interactions [6], linear confinement of a scalar particle subject to a scalar and vector potentials of Coulomb-types [7], Dirac equation [8], spin-0 system of DKP equation [9], and DKP oscillator [10] was investigated in this Type D metric.…”
Section: Characterization Of a Linear Class Of Gödel-type Metricsmentioning
confidence: 99%
“…With this solution for xðsÞ, we can solve for yðsÞ by simply substituting into Equation (10), with the result…”
Section: Geodesics For Observers and Light Raysmentioning
confidence: 99%
“…This is trivial in the ẑ direction: p z = 0. From Equation (10) we see that for _ y = 0 at all s, we need to fix the value of p y :…”
Section: Geodesics For Observers and Light Raysmentioning
The light rays and wave fronts in a linear class of the Gödel-type metric are examined to reveal the causality-violating features of the space-time. Noncausal features demonstrated by the development of unusual wave front singularities are shown to be related to the nonmonotonic advance of time along the light rays, as measured by a system of observers at rest with respect to one another with synchronized clocks.
“…A particularly simple Type D metric has recently examined a member of a linear class of Gödel-type metrics [5]. Previously, relativistic quantum motion of spin-0 particle without interactions [6], linear confinement of a scalar particle subject to a scalar and vector potentials of Coulomb-types [7], Dirac equation [8], spin-0 system of DKP equation [9], and DKP oscillator [10] was investigated in this Type D metric.…”
Section: Characterization Of a Linear Class Of Gödel-type Metricsmentioning
confidence: 99%
“…With this solution for xðsÞ, we can solve for yðsÞ by simply substituting into Equation (10), with the result…”
Section: Geodesics For Observers and Light Raysmentioning
confidence: 99%
“…This is trivial in the ẑ direction: p z = 0. From Equation (10) we see that for _ y = 0 at all s, we need to fix the value of p y :…”
Section: Geodesics For Observers and Light Raysmentioning
The light rays and wave fronts in a linear class of the Gödel-type metric are examined to reveal the causality-violating features of the space-time. Noncausal features demonstrated by the development of unusual wave front singularities are shown to be related to the nonmonotonic advance of time along the light rays, as measured by a system of observers at rest with respect to one another with synchronized clocks.
“…. Consider the following stationary space-time [50] (see [5,12,13,44,51]) in the Cartesian coordinates ðx 0 = t, x 1 = x, x 2 = y, x 3 = zÞ which is given by…”
Section: Bosonic Charged Particle: the Kg Equationmentioning
confidence: 99%
“…Substituting the series solution (equation ( 19)) into equation (51), we obtain the following recurrence relation:…”
In this paper, we investigate the relativistic quantum dynamics of spin-0 massive charged particle subject to a homogeneous magnetic field in the Gödel-type space-time with potentials. We solve the Klein-Gordon equation subject to a homogeneous magnetic field in a topologically trivial flat class of Gödel-type space-time in the presence of Cornell-type scalar and Coulomb-type vector potentials and analyze the effects on the energy eigenvalues and eigenfunctions.
In this work, we investigate the relativistic quantum motions of spinzero scalar bosons via the Duffin-Kemmer-Petiau (DKP) equation with a positiondependent mass (PDM) system in the background of the topological defect spacetime produced by a cosmic string. We determine the radial wave equation and obtain the exact analytical solutions of the wave equation for the linear and Cornelltype potential through the Bi-Confluent Heun differential equation. In fact, we have obtained the ground state energy for both potentials.
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