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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Dark matter halo parameters amplify the scale of closed timelike orbits in Schwarzschild spacetime, inducing phase lags in gravitational waves while light curves retain distinguishable peaks for certain orbital features.
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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.
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Gravitational emissions and light curves of quasi-periodic orbits in Schwarzschild spacetime embedded in a Dehnen-type dark matter halo
Dark matter halo parameters amplify the scale of closed timelike orbits in Schwarzschild spacetime, inducing phase lags in gravitational waves while light curves retain distinguishable peaks for certain orbital features.