Abstract:In this work the bound state and scattering problems for a spin-1/2 particle undergone to an Aharonov-Bohm potential in a conical space in the nonrelativistic limit are considered. The presence of a δ-function singularity, which comes from the Zeeman spin interaction with the magnetic flux tube, is addressed by the self-adjoint extension method. One of the advantages of the present approach is the determination of the self-adjoint extension parameter in terms of physics of the problem. Expressions for the ener… Show more
“…Therefore, for ν < 0, the bound state energy is given by [26,59] for the AB effect in curved space and is similar that one found in contact interactions of anyons [74]. It is also possible to express the S-matrix in terms of the bound state energy.…”
Section: A Application Of the Bg Methodssupporting
confidence: 63%
“…This is the scattering phase shift of the AB effect in the cosmic string spacetime [26,59]. It is important to mention that, for α = 1, it reduces to the phase shift for the usual AB effect in flat space δ AB m = π(|m| − |m + φ|)/2 [4].…”
Section: A Application Of the Bg Methodsmentioning
In this work, we review two methods used to approach singular Hamiltonians in (2+1) dimensions. Both methods are based on the self-adjoint extension approach. It is very common to find singular Hamiltonians in quantum mechanics, especially in quantum systems in the presence of topological defects, which are usually modelled by point interactions.In general, it is possible to apply some kind of regularization procedure, as the vanishing of the wave function at the location of the singularity, ensuring that the wave function is square-integrable and then can be associated with a physical state. However, a study based on the self-adjoint extension approach can lead to more general boundary conditions that still gives acceptable physical states. We exemplify the methods by exploring the bound and scattering scenarios of a spin 1/2 charged particle with an anomalous magnetic moment in the Aharonov-Bohm potential in the conical space.
“…Therefore, for ν < 0, the bound state energy is given by [26,59] for the AB effect in curved space and is similar that one found in contact interactions of anyons [74]. It is also possible to express the S-matrix in terms of the bound state energy.…”
Section: A Application Of the Bg Methodssupporting
confidence: 63%
“…This is the scattering phase shift of the AB effect in the cosmic string spacetime [26,59]. It is important to mention that, for α = 1, it reduces to the phase shift for the usual AB effect in flat space δ AB m = π(|m| − |m + φ|)/2 [4].…”
Section: A Application Of the Bg Methodsmentioning
In this work, we review two methods used to approach singular Hamiltonians in (2+1) dimensions. Both methods are based on the self-adjoint extension approach. It is very common to find singular Hamiltonians in quantum mechanics, especially in quantum systems in the presence of topological defects, which are usually modelled by point interactions.In general, it is possible to apply some kind of regularization procedure, as the vanishing of the wave function at the location of the singularity, ensuring that the wave function is square-integrable and then can be associated with a physical state. However, a study based on the self-adjoint extension approach can lead to more general boundary conditions that still gives acceptable physical states. We exemplify the methods by exploring the bound and scattering scenarios of a spin 1/2 charged particle with an anomalous magnetic moment in the Aharonov-Bohm potential in the conical space.
“…The AC effect and consequently the AB effect also has been addressed to bound states. In the context of the method of operators in quantum mechanics such bound states are found by modeling the problem by boundary conditions at the origin [12][13][14][15][16][17][18][19][20][21][22][23] (See also Refs. [24][25][26][27] where bound states also are obtained for Aharonov-Bohm-like systems.…”
“…[33][34][35][36][37][38][39]. The Dirac oscillator embedded in a cosmic string background has inspired a great deal of research in last years [40][41][42][43][44][45][46]. A cosmic string is a linear defect that change the topology of the medium when viewed globally.…”
The quantum dynamics of scalar bosons embedded in the background of a cosmic string is considered. In this work, scalar bosons are described by the Duffin-KemmerPetiau (DKP) formalism. In particular, the effects of this topological defect in the equation of motion, energy spectrum, and DKP spinor are analyzed and discussed in detail. The exact solutions for the DKP oscillator in this background are presented in closed form.
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