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| Auteurs principaux: | , |
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| Format: | Preprint |
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2026
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| Accès en ligne: | https://arxiv.org/abs/2602.13074 |
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| _version_ | 1866918339459153920 |
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| author | Li, Wen Chen, Chao |
| author_facet | Li, Wen Chen, Chao |
| contents | In this paper, we revisit the linear perturbation (including the comoving curvature perturbation and field perturbation) dynamics in the SR-USR-SR inflation with instantaneous transitions. Using the junction method and asymptotic expansions of Hankel functions, we derive accurate asymptotic expressions for the time evolution of mode functions and the resulting power spectrum, based on three systematic rules for identifying the dominant terms across transitions. Our results reveal that a finite dip of the final power spectrum arises from the cancellation between two growing modes within the linear perturbation theory, rather than between constant and growing terms as previously suggested. We also provide analytical descriptions of the amplitude enhancement and oscillatory features in the linear power spectrum, in agreement with numerical computations. These simple, tractable formulas not only facilitate theoretical calculations but also yield testable predictions for future CMB observations. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2602_13074 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Evolution of Linear Perturbations under Time-Dependent Hubble Friction I: SR-USR-SR Inflation Li, Wen Chen, Chao General Relativity and Quantum Cosmology Cosmology and Nongalactic Astrophysics In this paper, we revisit the linear perturbation (including the comoving curvature perturbation and field perturbation) dynamics in the SR-USR-SR inflation with instantaneous transitions. Using the junction method and asymptotic expansions of Hankel functions, we derive accurate asymptotic expressions for the time evolution of mode functions and the resulting power spectrum, based on three systematic rules for identifying the dominant terms across transitions. Our results reveal that a finite dip of the final power spectrum arises from the cancellation between two growing modes within the linear perturbation theory, rather than between constant and growing terms as previously suggested. We also provide analytical descriptions of the amplitude enhancement and oscillatory features in the linear power spectrum, in agreement with numerical computations. These simple, tractable formulas not only facilitate theoretical calculations but also yield testable predictions for future CMB observations. |
| title | Evolution of Linear Perturbations under Time-Dependent Hubble Friction I: SR-USR-SR Inflation |
| topic | General Relativity and Quantum Cosmology Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2602.13074 |