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The instability of a black hole with $f(R)$ global monopole under extended uncertainty principle

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arxiv 1908.08201 v1 pith:Z4CQW6YM submitted 2019-08-22 hep-th gr-qc

classification hep-thgr-qc
keywords blackholeglobalmonopoleeffectsevolutionextendedinstability
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abstract

We consider the evolution of black hole involving an $f(R)$ global monopole based on the Extended Uncertainty Principle (EUP). The black hole evolutions refer to the instability due to the Parikh-Kraus-Wilczeck tunneling radiation or fragmentation. It is found that the EUP corrections make the entropy difference larger to encourage the black hole to radiate more greatly. We also show that the appearance of the EUP effects result in the black hole's division. The influence from global monopole and the revision of general relativity can also adjust the black hole evolution simultaneously, but can not change the final result that the black hole will not be stable because of the EUP's effects.

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Cited by 1 Pith paper

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  1. Extended uncertainty principle inspired black hole in a G\"odel Universe

    gr-qc 2025-05 reject novelty 4.0 of 10

    A Godel-rotation-modified uncertainty principle is used to define a corrected black hole mass, producing enlarged horizon, shadow, and deflection with lower bounds a/M ~ 10^5 from EHT and PPN data.

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