首页> 外文期刊>International Journal of Astronomy and Astrophysics >Higher-Order Corrections for the Deflection of Light around a Massive Object. Diagonal Padé Approximants and Ray-Tracing Algorithms
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Higher-Order Corrections for the Deflection of Light around a Massive Object. Diagonal Padé Approximants and Ray-Tracing Algorithms

机译:围绕大质量物体的光偏转的高阶校正。对角Padé近似值和射线追踪算法

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From the Schwarzschild metric we obtain the higher-order terms for the deflection of light around a massive object using the Lindstedt-Poincaré method to solve the equation of motion of a photon around the stellar object. The asymptotic series obtained by this method was obtained up to order 20 in the expansion parameter, and was found to better approximate the numerical solution with higher order terms—a property that can’t be taken for granted for any asymptotic series. Additionally, we obtain diagonal Padé approximants from the perturbation expansion, and we show how these are a better fit for the numerical data than the original formal Taylor series. Furthermore, we use these approximants in ray-tracing algorithms to model the bending of light around massive objects.
机译:根据Schwarzschild度量,我们使用Lindstedt-Poincaré方法求解光子围绕恒星物体的运动方程,从而获得了绕大质量物体的光偏转的高阶项。通过该方法获得的渐近级数在展开参数中的阶数最高为20,并且发现可以更好地近似使用高阶项的数值解-这是任何渐近级数都不可理喻的性质。此外,我们从摄动展开中获得对角Padé近似值,并展示了与原始形式泰勒级数相比,它们更适合数字数据。此外,我们在光线跟踪算法中使用这些近似值来模拟大型物体周围的光的弯曲。

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