Verlinde’s emergent gravity in an <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" id="mml3" display="inline" overflow="scroll" altimg="si1.gif"><mml:mi>n</mml:mi></mml:math>-dimensional, non-additive Tsallis’ scenario

Zamora, D.J.; Rocca, Mario Carlos; Plastino, A.; Ferri, Gustavo Luis

doi:10.1016/j.physa.2018.05.031

Cited by 6 publications

(5 citation statements)

References 26 publications

Supporting

Mentioning

Contrasting

Unclassified

Order By: Relevance

“…[30] had made a guess of between gravity and entropic force. That was later proved [31][32][33][34][35][36][37] in a classical scenario. In addition, people proposed that gravity is a 5 Advances in High Energy Physics manifestation of material information through combining a thermal gravitation treatment to Hooft's holographic principle.…”

Section: Entropic Force Between Two Horizonsmentioning

confidence: 88%

Phase Transition and Entropic Force in Reissner-Nordström-de Sitter Spacetime

Zhang

et al. 2022

Advances in High Energy Physics

View full text Add to dashboard Cite

In this paper, thermodynamic properties of the Reissner-Nordström-de Sitter (RN-dS) black hole have been studied on the basis of the correlation between the black hole and cosmological horizons. It is found that the RN-dS black hole experiences a phase transition, when its state parameters satisfy certain conditions. From the analysis of the interaction between two horizons in RN-dS spacetime, we get the numerical solution of the interaction between two horizons. It makes us to realize the force between the black hole and cosmological horizons, which can be regarded as a candidate to explain our accelerating expansion universe. That provides a new window to explore the physical mechanism of the cosmic accelerating expansion.

show abstract

Section: Entropic Force Between Two Horizonsmentioning

confidence: 88%

Phase Transition and Entropic Force in Reissner-Nordström-de Sitter Spacetime

Zhang

et al. 2022

Advances in High Energy Physics

View full text Add to dashboard Cite

show abstract

“…Gravity emerges as a consequence of information regarding the positions of material bodies, combining a thermal gravitation treatment with 't Hooft's holographic principle. The ensuing conjecture was later proved [24][25][26][27][28][29][30][31] in a classical scenario. Accordingly, gravitation ought to be viewed as an emergent phenomenon.…”

Section: Introductionmentioning

confidence: 91%

“…The definition of the entropic force in the thermodynamic system is [24][25][26][27][28][29][30][31][32][33][34][35][36][37]…”

Section: Entropic Force Between the Two Ho-rizons In Epmd Ds Space-timementioning

confidence: 99%

Entropic force between two horizons of dilaton black holes with a power-Maxwell field *

et al. 2021

View full text Add to dashboard Cite

In this paper, we consider -dimensional topological dilaton de Sitter black holes with a power-Maxwell field as thermodynamic systems. The thermodynamic quantities corresponding to the black hole horizon and the cosmological horizon are interrelated. Therefore, the total entropy of the space-time should be the sum of the entropies of the black hole horizon and the cosmological horizon plus a correction term which is produced by the association of the two horizons. We analyze the entropic force produced by the correction term at given temperatures, which is affected by the parameters and dimensions of the space-time. It is shown that the change of entropic force with the position ratio of the two horizons in some regions is similar to that of the variation of the Lennard-Jones force with the position of particles. If the effect of entropic force is similar to that of the Lennard-Jones force, and other forces are absent, the motion of the cosmological horizon relative to the black hole horizon should have an oscillating process. The entropic force between the two horizons is probably one of the participants in driving the evolution of the universe.

show abstract

“…Gravity emerges as a consequence of information regarding the positions of material bodies, combining a thermal gravitation treatment to 't Hooft's holographic principle. The ensuing conjecture was later proved [24][25][26][27][28][29][30][31] in a classical scenario. Accordingly, gravitation ought to be viewed as an emergent phenomenon.…”

Section: Introductionmentioning

confidence: 99%

Entropic force between two horizons of dilaton black holes with a power-Maxwell field

Zhao,

Zhang,

Gao

et al. 2021

Preprint

View full text Add to dashboard Cite

In this paper, we consider (n+1)-dimensional topological dilaton de Sitter black holes with power-Maxwell field as thermodynamic systems. The thermodynamic quantities corresponding to the black hole horizon and the cosmological horizon respectively are interrelated. So the total entropy of the space-time should be the sum of the entropies of the black hole horizon and the cosmological horizon plus a corrected term which is produced by the association of the two horizons. We analyze the entropic force produced by the corrected term at given temperatures, which is affected by parameters and dimensions of the space-time. It is shown that the change of entropic force with the position ratio of two horizons in some region is similar to that of Lennard-Jones force with the position of particles. If the effect of entropic force is similar to that of Lennard-Jones force, and other forces are absent, the motion of the cosmological horizon relative to the black hole horizon would have an oscillating process. The entropic force between the two horizons is probably one of the participants to drive the evolution of universe.

show abstract

Verlinde’s emergent gravity in an n-dimensional, non-additive Tsallis’ scenario

Cited by 6 publications

References 26 publications

Phase Transition and Entropic Force in Reissner-Nordström-de Sitter Spacetime

Phase Transition and Entropic Force in Reissner-Nordström-de Sitter Spacetime

Entropic force between two horizons of dilaton black holes with a power-Maxwell field *

Entropic force between two horizons of dilaton black holes with a power-Maxwell field

Contact Info

Product

Resources

About