GRMHD and GRRT simulations of accretion onto a spinning Kerr-like wormhole show throat-dominated emission producing quasi-periodic modulations in 230 GHz light curves, distinct from Kerr black holes.
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3 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 3representative citing papers
Simulations show the singularity-free Kerr-Hayward metric yields EHT observables that are functionally indistinguishable from the Kerr metric.
The Bondi spherical accretion model is significantly more sensitive to spacetime geometry and fluid equation of state than the Novikov-Thorne thin disk model, making it better at distinguishing regular black holes from classical ones.
citing papers explorer
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Dynamics and Radiative Signatures of Accretion Flows onto a Kerr-like Wormhole
GRMHD and GRRT simulations of accretion onto a spinning Kerr-like wormhole show throat-dominated emission producing quasi-periodic modulations in 230 GHz light curves, distinct from Kerr black holes.
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On the observational distinguishability of the Kerr and Kerr-Hayward metrics to EHT
Simulations show the singularity-free Kerr-Hayward metric yields EHT observables that are functionally indistinguishable from the Kerr metric.
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Bondi and Novikov-Thorne accretion in regular black holes and Simpson-Visser spacetimes
The Bondi spherical accretion model is significantly more sensitive to spacetime geometry and fluid equation of state than the Novikov-Thorne thin disk model, making it better at distinguishing regular black holes from classical ones.