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.
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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.