3D GRMHD simulations of accretion onto a JMN-1 horizonless singularity produce a magnetically arrested disk with an accretion rate of ~3e-6 Eddington matching M87* observations and EHT-consistent images, plus central brightness inside the shadow as a discriminant from black holes.
Gravity versus astrophysics in black hole images and photon rings: equatorial emissions and spherically symmetric spacetimes
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Sufficiently compact astrophysical objects can produce mirror-like reflection images of sources through extreme gravitational lensing in Schwarzschild spacetime.
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GRMHD accretion beyond the black hole paradigm: Light from within the shadow
3D GRMHD simulations of accretion onto a JMN-1 horizonless singularity produce a magnetically arrested disk with an accretion rate of ~3e-6 Eddington matching M87* observations and EHT-consistent images, plus central brightness inside the shadow as a discriminant from black holes.
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Revisiting The Gravitational Mirroring In Presence of Compact Objects
Sufficiently compact astrophysical objects can produce mirror-like reflection images of sources through extreme gravitational lensing in Schwarzschild spacetime.