Uniform Asymptotic Approximation Method with Pöschl-Teller Potential
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arXiv
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| Main Authors: | , , , , , , |
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| Format: | Preprint |
| Published: |
2023
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| _version_ | 1866929200363995136 |
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| author | Pan, Rui Marchetta, John Joseph Saeed, Jamal Cleaver, Gerald Li, Bao-Fei Wang, Anzhong Zhu, Tao |
| author_facet | Pan, Rui Marchetta, John Joseph Saeed, Jamal Cleaver, Gerald Li, Bao-Fei Wang, Anzhong Zhu, Tao |
| contents | In this paper, we study analytical approximate solutions of the second-order homogeneous differential equations with the existence of only two turning points (but without poles), by using the uniform asymptotic approximation (UAA) method. To be more concrete, we consider the Pöschl-Teller (PT) potential, for which analytical solutions are known. Depending on the values of the parameters involved in the PT potential, we find that the upper bounds of the errors of the approximate solutions in general are $\lesssim 0.15\% \sim 10\% $, to the first-order approximation of the UAA method. The approximations can be easily extended to high-order, with which the errors are expected to be much smaller. Such obtained analytical solutions can be used to study cosmological perturbations in the framework of quantum cosmology, as well as quasi-normal modes of black holes. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2309_03327 |
| institution | arXiv |
| publishDate | 2023 |
| record_format | arxiv |
| spellingShingle | Uniform Asymptotic Approximation Method with Pöschl-Teller Potential Pan, Rui Marchetta, John Joseph Saeed, Jamal Cleaver, Gerald Li, Bao-Fei Wang, Anzhong Zhu, Tao General Relativity and Quantum Cosmology In this paper, we study analytical approximate solutions of the second-order homogeneous differential equations with the existence of only two turning points (but without poles), by using the uniform asymptotic approximation (UAA) method. To be more concrete, we consider the Pöschl-Teller (PT) potential, for which analytical solutions are known. Depending on the values of the parameters involved in the PT potential, we find that the upper bounds of the errors of the approximate solutions in general are $\lesssim 0.15\% \sim 10\% $, to the first-order approximation of the UAA method. The approximations can be easily extended to high-order, with which the errors are expected to be much smaller. Such obtained analytical solutions can be used to study cosmological perturbations in the framework of quantum cosmology, as well as quasi-normal modes of black holes. |
| title | Uniform Asymptotic Approximation Method with Pöschl-Teller Potential |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2309.03327 |