Constraints Between Equations of State and Mass-Radius Relationships in General Clusters of Stellar Systems
arXiv:1808.09306 · doi:10.1103/PhysRevD.99.023007
Abstract
In this article we prove three obstruction results on the existence of equations of state in clusters of stellar systems fulfilling mass-radius relationships and some additional bound (on the mass, on the radius or a causal bound). The theorems are proved in large generality. We start with a motivating example of TOV systems and we close by applying our results in stellar systems arising from experimental data.