Buchdahl bound, photon ring, ISCO and radial acceleration in Einstein-æther theory
Yi-Hsiung Hsu, Anthony Lasenby, Will Barker, Amel Durakovic, Michael Hobson
TL;DR
This work analyzes spherically symmetric configurations in the minimal Einstein–æther theory with a Maxwell-like kinetic term, focusing on vacuum exterior solutions and interior matter. The authors derive the Eling–Jacobson exterior solution, revealing that finite $K_{b}$ enlarges central radii such as the ISCO and photon ring while preserving a Schwarzschild-like Newtonian limit; they also show a gauge freedom that allows a diagonal metric and a purely time-like æther in vacuum, with a two-variable reduction to $X$ and $Y$ capturing the physics. Extending to matter, they formulate the Einstein–æther TOV equations, introduce an æther energy density, and derive a Buchdahl bound $\frac{M}{r_{b}} \le \frac{4(1-K_{b})}{(3-2K_{b})^{2}}$ for $0\le K_{b}\le 1/2$, with a saturated analytic solution supporting the bound. Numerical results for uniform density illustrate that the bound tightens with $K_{b}$ and that the radial acceleration relation scales as $g_{\text{EA}} \approx \frac{2}{2-K_{b}}\, g_{N}$ at low pressures, indicating a parallel but amplified Newtonian behavior. Overall, the paper provides exact exterior solutions, a gauge-invariant interior framework, and physically interpretable bounds that inform potential observational tests and connections to ÆST.
Abstract
Spherically symmetric Einstein-æther (EÆ) theory with a Maxwell-like kinetic term is revisited. We consider a general choice of the metric and the æther field, finding that:~(i) there is a gauge freedom allowing one always to use a diagonal metric; and~(ii) the nature of the Maxwell equation forces the æther field to be time-like in the coordinate basis. We derive the vacuum solution and confirm that the innermost stable circular orbit (ISCO) and photon ring are enlarged relative to general relativity (GR). Buchdahl's theorem in EÆ theory is derived. For a uniform physical density, we find that the upper bound on compactness is always lower than in GR. Additionally, we observe that the Newtonian and EÆ radial acceleration relations run parallel in the low pressure limit. Our analysis of EÆ theory may offer novel insights into its interesting phenomenological generalization: Æther--scalar--tensor theory (ÆST).
