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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f(Q,T) gravity with linear form and affine EoS is constrained by CC, Pantheon+SH0ES and DESI BAO data, yielding a present universe age consistent with Planck within 1σ.
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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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The $f(Q, T)$ gravity and affine EoS: observational aspects
f(Q,T) gravity with linear form and affine EoS is constrained by CC, Pantheon+SH0ES and DESI BAO data, yielding a present universe age consistent with Planck within 1σ.