The impact of initial conditions on quasi-normal modes
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arXiv
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| Auteurs principaux: | , , |
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| Format: | Preprint |
| Publié: |
2024
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| _version_ | 1866917856760823808 |
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| author | Chavda, Ameya Lagos, Macarena Hui, Lam |
| author_facet | Chavda, Ameya Lagos, Macarena Hui, Lam |
| contents | This study investigates the influence of initial conditions on the evolution and properties of linear quasi-normal modes (QNMs). Using a toy model in which the quasi-normal mode can be unambiguously identified, we highlight an aspect of QNMs that is long known yet often ignored: the amplitude of a QNM (after factoring out the corresponding exponential with a complex frequency) is not constant but instead varies with time. We stress that this is true even within the regime of validity of linear perturbation theory. The precise time variation depends on the initial conditions. In particular, it is possible to find initial conditions for which the QNM fails to materialize; it is also possible to find those for which the QNM amplitude grows indefinitely. Focusing on cases where the QNM amplitude does stabilize at late times, we explore how the timescale for amplitude stabilization depends on the shape and location of the initial perturbation profile. Our findings underscore the need for care in fitting linear QNMs to ringdown data. They also suggest recent computations of quadratic QNMs, sourced purely by {\it stabilized} linear QNMs, do not fully capture what determines the amplitude of the quadratic QNMs, even at late times. Our results motivate a detailed investigation of the initial perturbations generated in the aftermath of a binary merger. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2412_03435 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The impact of initial conditions on quasi-normal modes Chavda, Ameya Lagos, Macarena Hui, Lam General Relativity and Quantum Cosmology This study investigates the influence of initial conditions on the evolution and properties of linear quasi-normal modes (QNMs). Using a toy model in which the quasi-normal mode can be unambiguously identified, we highlight an aspect of QNMs that is long known yet often ignored: the amplitude of a QNM (after factoring out the corresponding exponential with a complex frequency) is not constant but instead varies with time. We stress that this is true even within the regime of validity of linear perturbation theory. The precise time variation depends on the initial conditions. In particular, it is possible to find initial conditions for which the QNM fails to materialize; it is also possible to find those for which the QNM amplitude grows indefinitely. Focusing on cases where the QNM amplitude does stabilize at late times, we explore how the timescale for amplitude stabilization depends on the shape and location of the initial perturbation profile. Our findings underscore the need for care in fitting linear QNMs to ringdown data. They also suggest recent computations of quadratic QNMs, sourced purely by {\it stabilized} linear QNMs, do not fully capture what determines the amplitude of the quadratic QNMs, even at late times. Our results motivate a detailed investigation of the initial perturbations generated in the aftermath of a binary merger. |
| title | The impact of initial conditions on quasi-normal modes |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2412.03435 |