Thermodynamic phase transition based on the nonsingular temperature

Eune, Myungseok; Gim, Yongwan; Kim, Wontae

doi:10.1103/physrevd.91.044037

Cited by 9 publications

(7 citation statements)

References 52 publications

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“…Since the modified Hawking temperature T modified H and its corresponding thermodynamic phase transition have been studied in detail in Refs. [49][50][51], we only focus on the Eq. ( 14) and its corresponding thermodynamic phase transition in upcoming contents.…”

Section: The Modified Thermodynamics Of Schwarzschild Black Hole In T...mentioning

confidence: 99%

The thermodynamics and phase transition of a rainbow black hole

2019

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In this work, we construct a new kind of rainbow functions, which has generalized uncertainty principle parameter. Then, we investigate modified thermodynamic quantities and phase transition of rainbow Schwarzschild black hole by employing this new kind of rainbow functions. Our results demonstrate that the rainbow gravity and generalized uncertainty principle have a great effect on the picture of Hawking radiation. They prevent black holes from total evaporation and cause a remnant. In addition, after analyzing the modified local thermodynamic quantities, we find that the effect of rainbow gravity and the generalized uncertainty principle lead to one first-order phase transition, two second-order phase transitions, and two Hawking-Page-type phase transitions in the thermodynamic system of rainbow Schwarzschild black hole.

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Section: The Modified Thermodynamics Of Schwarzschild Black Hole In T...mentioning

confidence: 99%

The thermodynamics and phase transition of a rainbow black hole

2019

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“…Next, let us calculate the free energy of the black hole in order to study phase transition between the black holes and the hot flat space [24,28].…”

Section: The Critical Effective In Charged Black Hole In Cavitymentioning

confidence: 99%

“…We will keep the charge inside the cavity also fixed. This will define a canonical ensemble [23][24][25][26][27][28]. We will study the phase structure and the thermodynamic properties of the various dimensional charged black hole in this ensemble.…”

Section: Introductionmentioning

confidence: 99%

The Phase Transition of Higher Dimensional Charged Black Holes

Guo¹,

Zhang³

et al. 2016

Advances in High Energy Physics

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In this paper,we have studied phase transitions of higher dimensional charge black hole with spherical symmetry. we calculated the local energy and local temperature, and find that these state parameters satisfy the first law of thermodynamics . We analyze the critical behavior of black hole thermodynamic system by taking state parameters (Q, Φ) of black hole thermodynamic system, in accordance with considering to the state parameters (P, V ) of Van der Waals system respectively. we obtain the critical point of black hole thermodynamic system, and find the critical point is independent of the dual independent variables we selected. This result for asymptotically flat space is consistent with that for AdS spacetime, and is intrinsic property of black hole thermodynamic system.

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“…Utilizing the method described above, the literature [26][27][28][29][30][31][32] have studied the charged black hole and black branes, obtained the requirements to meet the thermodynamic equilibrium conditions, and discussed the phase transition and critical phenomena. More recently, Eune et al (2015) investigated the phase transition based on the corrections of Schwarzschild black hole radiation temperature [33]. More specifically, both of the charged black hole and the radiation field outside the black hole were considered in their work, under the condition that they are both in the equilibrium state.…”

Section: Introductionmentioning

confidence: 99%

The Thermodynamic Relationship between the RN-AdS Black Holes and the RN Black Hole in Canonical Ensemble

Zhang

Liu³

et al. 2017

Advances in High Energy Physics

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In this paper, by analyzing the thermodynamic properties of charged AdS black hole and asymptotically flat space-time charged black hole in the vicinity of the critical point, we establish the correspondence between the thermodynamic parameters of asymptotically flat space-time and nonasymptotically flat space-time, based on the equality of black hole horizon area in the two different space-time. The relationship between the cavity radius (which is introduced in the study of asymptotically flat space-time charged black holes) and the cosmological constant (which is introduced in the study of nonasymptotically flat space-time) is determined. The establishment of the correspondence between the thermodynamics parameters in two different space-time is beneficial to the mutual promotion of different time-space black hole research, which is helpful to understand the thermodynamics and quantumproperties of black hole in space-time.

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Thermodynamic phase transition based on the nonsingular temperature

Cited by 9 publications

References 52 publications

The thermodynamics and phase transition of a rainbow black hole

The thermodynamics and phase transition of a rainbow black hole

The Phase Transition of Higher Dimensional Charged Black Holes

The Thermodynamic Relationship between the RN-AdS Black Holes and the RN Black Hole in Canonical Ensemble

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