English

Perturbative solution to the Lane-Emden equation: An eigenvalue approach

Solar and Stellar Astrophysics 2016-11-24 v1

Abstract

Under suitable scaling, the structure of self-gravitating polytropes is described by the standard Lane-Emden equation (LEE), which is characterised by the polytropic index nn. Here we use the known exact solutions of the LEE at n=0n=0 and 11 to solve the equation perturbatively. We first introduce a scaled LEE (SLEE) where polytropes with different polytropic indices all share a common scaled radius. The SLEE is then solved perturbatively as an eigenvalue problem. Analytical approximants of the polytrope function, the radius and the mass of polytropes as a function of nn are derived. The approximant of the polytrope function is well-defined and uniformly accurate from the origin down to the surface of a polytrope. The percentage errors of the radius and the mass are bounded by 8.1×1078.1 \times 10^{-7} per cent and 8.5×1058.5 \times 10^{-5} per cent, respectively, for n[0,1]n\in[0,1]. Even for n[1,5)n\in[1,5), both percentage errors are still less than 22 per cent.

Keywords

Cite

@article{arxiv.1611.07202,
  title  = {Perturbative solution to the Lane-Emden equation: An eigenvalue approach},
  author = {Kenny L. S. Yip and T. K. Chan and P. T. Leung},
  journal= {arXiv preprint arXiv:1611.07202},
  year   = {2016}
}
R2 v1 2026-06-22T17:00:26.886Z