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    Buchdahl bound, photon ring, innermost stable circular orbit, and radial acceleration in Einstein-æther theory

    Yi-Hsiung Hsu1,*, Anthony Lasenby1,2,†, Will Barker1,2,3,‡, Amel Durakovic4,3,§, and Michael Hobson1,∥

    • 1Cavendish Laboratory, Astrophysics Group, JJ Thomson Avenue, Cambridge CB3 0HE, United Kingdom
    • 2Kavli Institute for Cosmology, Madingley Road, Cambridge CB3 0HA, United Kingdom
    • 3Central European Institute for Cosmology and Fundamental Physics, Institute of Physics of the Czech Academy of Sciences, Na Slovance 1999/2, 182 00 Prague 8, Czechia
    • 4Observatoire astronomique de Strasbourg, Université de Strasbourg, 11 Rue de l’Université, 67000 Strasbourg, France

    • *Contact author: yhh36@cam.ac.uk
    • †Contact author: a.n.lasenby@mrao.cam.ac.uk
    • ‡Contact author: wb263@cam.ac.uk
    • §Contact author: amel@fzu.cz
    • ∥Contact author: mph@mrao.cam.ac.uk

    Phys. Rev. D 111, 124032 – Published 20 June, 2025

    DOI: https://doi.org/10.1103/4y9j-wyrf

    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 timelike in the coordinate basis. We derive the vacuum solution and confirm that the innermost stable circular orbit 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.

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