The paper derives effective potentials and GUP-modified Hawking thermodynamics for cylindrical black holes in f(R) and Ricci-Inverse gravity, but the advertised quasinormal mode analysis is absent.
Investigating the Generalized Uncertainty Principle Effects on Hawking Radiation in Rotating Linear Dilaton Black Holes
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abstract
The impact of the Generalized Uncertainty Principle (GUP) on Hawking particle emission in a rotating linear dilaton black hole (RLDBH) spacetime is examined in this thesis. The concerned study presents a thermal emission model for black holes (BHs) that incorporates the influence of gravitational lens particles through GUP during the quantum tunneling process. The findings suggest that with GUP support, the temperature of Hawking radiation decreases as GUP parameters increase and rises with an increasing BH mass. The thesis also delves into the repercussions of these discoveries on the information loss paradox and adjusted entropy, while also exploring the potential utilization of astrophysical data to confirm GUP effects. In conclusion, our work underscores the significant role of GUP in the thermal emission of non-asymptotically flat (NAF), stationary BHs and its capacity to shed light on the intricate relationship between astrophysics and quantum gravity.
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Scalar, Vector Perturbations and Effective Hawking Radiation of Cylindrical Black Holes in $f(\mathcal{R})$ and Ricci-Inverse Gravity
The paper derives effective potentials and GUP-modified Hawking thermodynamics for cylindrical black holes in f(R) and Ricci-Inverse gravity, but the advertised quasinormal mode analysis is absent.