Power laws, scale invariance, and generalized Frobenius series: Applications to Newtonian and TOV stars near criticality
Nicolas Yunes (Washington University in Saint Louis), Matt Visser, (Victoria University of Wellington)

TL;DR
This paper develops a formalism for analyzing scale invariant differential equations, deriving power-law solutions and their deviations, and applies it to models of Newtonian and relativistic stars near collapse, revealing oscillatory power-law behaviors.
Contribution
It introduces a generalized Frobenius series approach for scale invariant equations and extends classical stellar models to include oscillatory and self-similar solutions.
Findings
Power-law solutions characterize star behavior near collapse.
Oscillatory power-law behavior is observed in models approaching criticality.
The formalism extends classical stellar solutions to more general cases.
Abstract
We present a self-contained formalism for analyzing scale invariant differential equations. We first cast the scale invariant model into its equidimensional and autonomous forms, find its fixed points, and then obtain power-law background solutions. After linearizing about these fixed points, we find a second linearized solution, which provides a distinct collection of power laws characterizing the deviations from the fixed point. We prove that generically there will be a region surrounding the fixed point in which the complete general solution can be represented as a generalized Frobenius-like power series with exponents that are integer multiples of the exponents arising in the linearized problem. This Frobenius-like series can be viewed as a variant of Liapunov's expansion theorem. As specific examples we apply these ideas to Newtonian and relativistic isothermal stars and…
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