Topological defects and scalar field modes in cosmological backgrounds
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arXiv
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| Main Authors: | , , , |
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| Format: | Preprint |
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2026
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| _version_ | 1866918310809960448 |
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| author | Saharian, A. A. Mirzoyan, G. V. Harutyunyan, G. H. Avagyan, R. M. |
| author_facet | Saharian, A. A. Mirzoyan, G. V. Harutyunyan, G. H. Avagyan, R. M. |
| contents | We study topological defects with a general structure in higher-dimensional cosmological backgrounds described by a set of angle deficit parameters. As special cases, they include higher-dimensional generalizations of cosmic strings and global monopoles. The corresponding complete set of mode functions is presented for a massive scalar field with a general curvature coupling parameter. For general scale factors and radial functions in the line element, the angular parts of the scalar modes are expressed in terms of associated Legendre functions. De Sitter and Milne universes are considered as examples of cosmological expansion. For the de Sitter bulk, we present the time-dependent parts of the mode functions in inflationary, hyperbolic, and global coordinates. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2601_20349 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Topological defects and scalar field modes in cosmological backgrounds Saharian, A. A. Mirzoyan, G. V. Harutyunyan, G. H. Avagyan, R. M. High Energy Physics - Theory General Relativity and Quantum Cosmology We study topological defects with a general structure in higher-dimensional cosmological backgrounds described by a set of angle deficit parameters. As special cases, they include higher-dimensional generalizations of cosmic strings and global monopoles. The corresponding complete set of mode functions is presented for a massive scalar field with a general curvature coupling parameter. For general scale factors and radial functions in the line element, the angular parts of the scalar modes are expressed in terms of associated Legendre functions. De Sitter and Milne universes are considered as examples of cosmological expansion. For the de Sitter bulk, we present the time-dependent parts of the mode functions in inflationary, hyperbolic, and global coordinates. |
| title | Topological defects and scalar field modes in cosmological backgrounds |
| topic | High Energy Physics - Theory General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2601.20349 |