Rotation effect for chiral magnetic cosmic string in the Kaluza-Klein theory

被引：0

作者：

Vitoria, R. L. L. ^{[1
]}

Pereira, C. F. S. ^{[2
]}

Leite, E. V. B. ^{[3
]}

Soares, A. R. ^{[4
]}

Belich, H. ^{[2
]}

机构：

[1] Univ Fed Para, Ave Augusto Correa, BR-66075110 Belem, PA, Brazil

[2] Univ Fed Espirito Santo, Dept Ciencias Biol, Ave Fernando Ferrari,514 Goiabeiras, BR-29075910 Vitoria, ES, Brazil

[3] Univ Fed Paraiba, Dept Fis, Caixa Postal 5008, BR-58051900 Joao Pessoa, PB, Brazil

[4] Inst Fed Educ Ciencia & Tecnol Maranhao, Campus Buriticupu, BR-65393000 Buriticupu, Maranhao, Brazil

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS A | 2025年 / 40卷 / 04期

关键词：

Kaluza-Klein theory; topological defect; cosmic string; Aharonov-Bohm effect for bound states; time-like dislocation; GRAVITATIONAL-FIELD; OSCILLATOR; GRAVITY;

D O I：

10.1142/S0217751X24501768

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

In this paper, we have investigated bound state solutions for a scalar particle described in the space-time of a chiral cosmic string subjected to rotational effects in a Kaluza-Klein theory. We saw that combinations between the parameters that describe the generalized space-time impose upper and lower limits for the radial coordinate leading to well-established boundary conditions.

引用

页数：10

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