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How black hole mimickers and Shapiro-free lenses signal effective dark matter

Lirui Yang1,2,3,4,*, Will Barker5,2,3,†, Tobias Mistele6,7,‡, and Amel Durakovic5,8,9,§

  • *Contact author: ly344@cantab.ac.uk
  • †Contact author: barker@fzu.cz
  • ‡Contact author: txm523@case.edu
  • §Contact author: amel.durakovic@pmf.unsa.ba

Phys. Rev. D 113, 024068 – Published 30 January, 2026

DOI: https://doi.org/10.1103/3bnx-gxzg

Abstract

We report the existence of two exotic compact objects in the leading relativistic model of modified Newtonian dynamics, namely æther-scalar-tensor theory. This model is consistent with precision cosmology and gravitational wave constraints on tensor speed. Black hole mimickers could subtly change observations: gravitational waves from their mergers might show unusual echoes or altered ringdown patterns, and images of their horizon-scale shadows might be slightly different from those of a true black hole. Shapiro-free lenses are massless objects that deflect light without any gravitational time delay, producing distinctive lensing events. These predictions connect to ongoing and future gravitational-wave searches, horizon-scale imaging, and time-domain lensing surveys.

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