Kaluza-Klein inspired a model of the inflation with the inversed power law potential in Bianchi type-I universe
Fuente:
arXiv
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| Autores principales: | , , , , , , |
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| Formato: | Preprint |
| Publicado: |
2025
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| _version_ | 1866916800780828672 |
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| author | Wattanakumpolkij, Jaturaporn Ma-ardlerd, Patinya Autthisin, Natthason Chuvala, Pornpatara Lunrasri, Nutthaphat Pongkitivanichkul, Chakrit Samart, Daris |
| author_facet | Wattanakumpolkij, Jaturaporn Ma-ardlerd, Patinya Autthisin, Natthason Chuvala, Pornpatara Lunrasri, Nutthaphat Pongkitivanichkul, Chakrit Samart, Daris |
| contents | This work considers the dynamics of the gauge vector and inflaton (dilaton) fields inspired by Kaluza-Klein theory in an inflationary universe with Bianchi type-I spacetime. The inverse power-law potential of the inflaton field is used to study dynamical system analysis. As a result, all fixed points in the autonomous system are non-hyperbolic fixed points, and one cannot determine their stability. Therefore, a center manifold theory is required to analyze the stability of the dynamical system properly. Interestingly, we found an isotropic attractor point which means that the universe undergoes accelerated expansion (inflation) from an anisotropic phase to an isotropic phase of the universe. According to the dynamical system analysis of the anisotropic Bianchi type-I universe with the inspired Kaluza-Klein model, our results supported the isotropization of the observed universe. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2506_16139 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Kaluza-Klein inspired a model of the inflation with the inversed power law potential in Bianchi type-I universe Wattanakumpolkij, Jaturaporn Ma-ardlerd, Patinya Autthisin, Natthason Chuvala, Pornpatara Lunrasri, Nutthaphat Pongkitivanichkul, Chakrit Samart, Daris General Relativity and Quantum Cosmology This work considers the dynamics of the gauge vector and inflaton (dilaton) fields inspired by Kaluza-Klein theory in an inflationary universe with Bianchi type-I spacetime. The inverse power-law potential of the inflaton field is used to study dynamical system analysis. As a result, all fixed points in the autonomous system are non-hyperbolic fixed points, and one cannot determine their stability. Therefore, a center manifold theory is required to analyze the stability of the dynamical system properly. Interestingly, we found an isotropic attractor point which means that the universe undergoes accelerated expansion (inflation) from an anisotropic phase to an isotropic phase of the universe. According to the dynamical system analysis of the anisotropic Bianchi type-I universe with the inspired Kaluza-Klein model, our results supported the isotropization of the observed universe. |
| title | Kaluza-Klein inspired a model of the inflation with the inversed power law potential in Bianchi type-I universe |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2506.16139 |