Uniform Asymptotic Approximation Method with Pöschl-Teller Potential

被引:0
|
作者
Pan, Rui [1 ]
Marchetta, John Joseph [2 ]
Saeed, Jamal [1 ]
Cleaver, Gerald [2 ]
Li, Bao-Fei [3 ,4 ]
Wang, Anzhong [1 ]
Zhu, Tao [3 ,4 ]
机构
[1] Baylor Univ, Phys Dept, GCAP CASPER, Waco, TX 76798 USA
[2] Baylor Univ, Phys Dept, EUCOS CASPER, Waco, TX 76798 USA
[3] Zhejiang Univ Technol, Inst Adv Phys & Math, Hangzhou 310032, Peoples R China
[4] Zhejiang Univ Technol, United Ctr Gravitat Wave Phys UCGWP, Hangzhou 310032, Peoples R China
关键词
loop quantum cosmology; cosmological perturbations; power spectrum; black holes; quasi-normal modes; gravitational waves; 98.80.Cq; 98.80.Qc; 04.50.Kd; 04.60.Bc; LINEAR-DIFFERENTIAL EQUATIONS; QUANTUM; GRAVITY; MODES;
D O I
10.3390/universe9110471
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we study analytical approximate solutions for 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 Poschl-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 less than or similar to 0.15 similar to 10% for the first-order approximation of the UAA method. The approximations can be easily extended to high orders, for 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.
引用
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页数:26
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