Algorithmic construction of static perfect fluid spheres
Damien Martin (Victoria University of Wellington), Matt Visser, (Victoria University of Wellington)

TL;DR
This paper refines Lake's algorithm for constructing static perfect fluid spheres, providing explicit formulas and a clearer physical interpretation, enabling the generation of new solutions and better understanding of existing ones.
Contribution
It presents a re-cast of Lake's algorithm using physically meaningful variables, with explicit formulas for mass, pressure, and central pressure, and facilitates the discovery of new solutions.
Findings
Explicit formulas for mass and pressure profiles
Closed-form expression for central pressure
Generation of new exact solutions
Abstract
Perfect fluid spheres, both Newtonian and relativistic, have attracted considerable attention as the first step in developing realistic stellar models (or models for fluid planets). Whereas there have been some early hints on how one might find general solutions to the perfect fluid constraint in the absence of a specific equation of state, explicit and fully general solutions of the perfect fluid constraint have only very recently been developed. In this article we present a version of Lake's algorithm [Phys. Rev. D 67 (2003) 104015; gr-qc/0209104] wherein: (1) we re-cast the algorithm in terms of variables with a clear physical meaning -- the average density and the locally measured acceleration due to gravity, (2) we present explicit and fully general formulae for the mass profile and pressure profile, and (3) we present an explicit closed-form expression for the central pressure.…
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