Abstract
Abstract
In this work, we analyze the behavior of a spin-0 particle confined inside a sphere in space-time with a double topological deficit, whose line element is given by
ds
2
=
dt
2
−
b
−
2
dr
2
−
r
2
d
θ
2
−
γ
2
r
2
sin
2
θ
d
ϕ
2
, where (b, γ) are real constants. We show that it is possible to confine the particle inside a spherical cone-shaped section with θ < θ
0, where θ
0 is the confinement angle and r < a with a being the radius of the section spherical, and we obtain the angles θ
0 that confine the particle as a function of the angular moments l and m and the parameter of the cosmic string γ. As an application, we analyze the particle confined inside a regular sphere, that is θ
0 = π and r < a,and we investigate how topological defects in space influence the eigenenergies and probability densities of the particle inside the sphere. As a result, we verified that the more intense the topological defect, the greater the energy of the particle, and it will be confined in regions where r → a.
Subject
Condensed Matter Physics,Mathematical Physics,Atomic and Molecular Physics, and Optics