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Investigating the Generalized Uncertainty Principle Effects on Hawking Radiation in Rotating Linear Dilaton Black Holes

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arxiv 2404.13450 v1 pith:KEHUILF5 submitted 2024-04-20 gr-qc

Erdem Sucu This is my paper · ORCID
classification gr-qc
keywords blackemissionhawkingdilatoneffectsgeneralizedholeslinear
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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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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Scalar, Vector Perturbations and Effective Hawking Radiation of Cylindrical Black Holes in $f(\mathcal{R})$ and Ricci-Inverse Gravity

    gr-qc 2024-12 reject novelty 2.0 of 10

    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.

  2. Quasinormal Modes and GUP-Corrected Hawking Radiation of BTZ Black Holes within Modified Gravity Frameworks

    gr-qc 2024-12 reject novelty 2.0 of 10

    QNM frequencies and GUP-corrected Hawking temperatures of BTZ black holes in f(R) and Ricci-Inverse gravity are expressed in terms of an effective cosmological constant, but key derivations contain errors.

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