The effect of the GUP on massive vector and scalar particles tunneling from a warped DGP gravity black hole

Овгун, Али; Jusufi, Kimet

doi:10.1140/epjp/i2017-11574-9

Cited by 61 publications

(22 citation statements)

References 73 publications

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“…In this section we analyze the effects of considering a quantum correction to the usual black hole thermodynamics. These types of corrections are considered previously for various of black holes [117][118][119][120][121]. We consider an uncertainty principle of the form…”

Section: Thermodynamics Of a Bh-dl-ned A Semiclassial Thermodynamics ...mentioning

confidence: 99%

Nonlinear electrodynamics effects on the black hole shadow, deflection angle, quasinormal modes and greybody factors

Okyay,

Övgün

2021

Preprint

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In this paper, we discuss the effects of nonlinear electrodynamics (NED) on non-rotating black holes, parametrized by the field coupling parameter β and magnetic charge parameter P in detail. Particularly, we survey a large range of observables and physical properties of the magnetically charged black hole, including the thermodynamic properties, observational appearance, quasinormal modes and absorption cross sections. Initially, we show that the NED black hole is always surrounded by an event horizon and any magnetic charge is permissible. We then show that the black hole gets colder with increasing charge. Investigating the heat capacity, we see that the black hole is thermally stable between points of phase transition. Introducing a generalized uncertainty principle (GUP) with a quantum gravity parameter λ extends the range of the stable region, but the effect on temperature is negligible. Then we compute the deflection angle at the weak field limit, by the Gauss-Bonnet theorem and the geodesic equation, and find that even at the first order, the magnetic charge has a contribution due to the "field mass" term. Small changes of the charge contributes greatly to the paths of null geodesics due to the P 2 dependence of the horizon radius. Using a ray-tracing code, we simulate the observational appearance of a NED black hole under different emission profiles, thin disk and spherical accretion. We find that the parameter P has a very strong effect on the observed shadow radius, in agreement with the deflection angle calculations. We finally consider quasinormal modes under massless scalar perturbations of the black hole and the greybody factor. We find that the charge introduces a slight difference in the fundamental frequency of the emitted waveform. We find that the greybody factor of the NED black hole is strongly steepened by the introduction of increasing charge. To present observational constrains, we show that the magnetic charge of the M87 * black hole is between 0 ≤ P ≤ 0.024 in units of M, in agreement with the idea that real astrophysical black holes are mostly neutral. We also find that LIGO/VIRGO and LISA could detect NED black hole perturbations from BHs with masses between 5M and 8.0 • 10 8 M . We finally show that for black holes with masses detected with LIGO so far, charged NED black holes would deviate from Schwarzschild by 5 ∼ 10 Hz in their fundamental frequencies.

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Section: Thermodynamics Of a Bh-dl-ned A Semiclassial Thermodynamics ...mentioning

confidence: 99%

Nonlinear electrodynamics effects on the black hole shadow, deflection angle, quasinormal modes and greybody factors

Okyay,

Övgün

2021

Preprint

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“…Besides, by using the KMM model, researchers derived the GUP corrected Hamilton-Jacobi equation and investigated the modified tunneling rate of particles with arbitrary spins from the event of curved spacetimes [9]. Moreover, the KMM model and ADV model can also be extended to the Proca equation, which leads to the modified Hawking temperature of black holes [10][11][12]. In addition, Vagenas et al studied the validity of the no-cloning theorem within the framework of GUP.…”

Section: Introductionmentioning

confidence: 99%

Higher-order generalized uncertainty principle corrections to the Jeans mass

Feng

Zhou

et al. 2021

Eur. Phys. J. C

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The Jeans instability is regarded as an important tool for analyzing the dynamics of a self-gravitating system. However, this theory is challenging since astronomical observation data show some Bok globules, whose masses are less than the Jeans mass and still have stars or at least undergo the star formation process. To explain this problem, we investigate the effects of the higher-order generalized uncertainty principle on the Jeans mass of the collapsing molecular cloud. The results in this paper show that the higher order generalized uncertainty principle has a very significant effect on the canonical energy and gravitational potential of idea gas, and finally leads to a modified Jeans mass lower than the original case, which is conducive to the generation of stars in small mass Bok globules. Furthermore, we estimate the new generalized uncertainty principle parameter $$\gamma _0$$ γ 0 by applying various data of Bok globules, and find that the range of magnitude of $$\gamma _0$$ γ 0 is $${10^{11}} {-} {10^{12}}$$ 10 11 - 10 12 .

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“…The BHs are the main experimental scalar and vector fields for studying the effects of gravity and there is much literature on the thermodynamical properties of BHs to study the gravity effects under GUP. The BH thermodynamics have been analyzed within the GUP [9][10][11][12][13][14][15][16]. The field equation in the WKB approximation and tunneling of bosons from the BHs in different theory have been analyzed [17,18].…”

Section: Introductionmentioning

confidence: 99%

Stability Analysis of Charged Rotating Black Ring

Ali¹,

Bamba

Asgher

et al. 2020

Symmetry

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We study the electromagnetic field equation along with the WKB approximation. The boson tunneling phenomenon from charged rotating black ring (CRBR) is analyzed. It is examined that reserve radiation consistent with CRBR can be computed in general by neglecting back reaction and self-gravitational of the radiated boson particle. The calculated temperature depends upon quantum gravity and CRBR geometry. We also examine the corrected tunneling rate/probability of boson particles by assuming charge as well as energy conservation laws and the quantum gravity. Furthermore, we study the graphical behavior of the temperature and check the stability and instability of CRBR.

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The effect of the GUP on massive vector and scalar particles tunneling from a warped DGP gravity black hole

Cited by 61 publications

References 73 publications

Nonlinear electrodynamics effects on the black hole shadow, deflection angle, quasinormal modes and greybody factors

Nonlinear electrodynamics effects on the black hole shadow, deflection angle, quasinormal modes and greybody factors

Higher-order generalized uncertainty principle corrections to the Jeans mass

Stability Analysis of Charged Rotating Black Ring

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