Higher derivative corrections to the entropic force from holography

Zhang, Ziqiang; Luo, Zhijun; Hou, Defu

doi:10.1016/j.aop.2018.02.004

Cited by 12 publications

(4 citation statements)

References 49 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…From the entropic point of view, the effective entropic force due to the change in entropy obeys [44][45][46][47][48][49][50][51][52]]…”

Section: Entropy Force Generated By the Horizon Interactionmentioning

confidence: 99%

Phase transitions and entropy force of charged de Sitter black holes with cloud of string and quintessence

Ma,

Zhang,

Zhao

et al. 2019

Preprint

View full text Add to dashboard Cite

In this paper, we investigate the combined effects of the cloud of strings and quintessence on the thermodynamics of a Reissner-Nordström-de Sitter black hole. Based on the equivalent thermodynamic quantities considering the correlation between the black hole horizon and the cosmological horizon, we extensively discuss the phase transitions of the space-time. Our analysis prove that similar to the case in AdS space-time, second-order phase transitions could take place under certain conditions, with the absence of first-order phase transition in the charged de Sitter black holes with cloud of string and quintessence. The effects of different thermodynamic quantities on the phase transitions are also quantitatively discussed, which provides a new approach to study the thermodynamic qualities of unstable dS space-time. Focusing on the entropy force generated by the interaction between the black hole horizon and the cosmological horizon, as well as the Lennard-Jones force between two particles, our results demonstrate the strong degeneracy between the entropy force of the two horizons and the ratio of the horizon positions, which follows the surprisingly similar law given the relation between the Lennard-Jones force and the ratio of two particle positions. Therefore, the study of the entropy force between two horizons, is not only beneficial to the deep exploration of the three modes of cosmic evolution, but also helpful to understand the correlation between the microstates of particles in black holes and those in ordinary thermodynamic systems.

show abstract

“…From the entropic point of view, the effective entropic force due to the change in entropy obeys [44][45][46][47][48][49][50][51][52]]…”

Section: Entropy Force Generated By the Horizon Interactionmentioning

confidence: 99%

Phase transitions and entropy force of charged de Sitter black holes with cloud of string and quintessence

Ma,

Zhang,

Zhao

et al. 2019

Preprint

View full text Add to dashboard Cite

show abstract

“…For instance, the ratio of shear viscosity to entropy density [23][24][25][26][27], heavy quark potential [28][29][30], drag force [31][32][33], and jet quenching parameter [34,35] have been discussed under R 4 or R 2 corrections. Other interesting results can be found in [36][37][38][39][40][41][42][43][44][45][46][47][48][49][50][51]. To the best of our knowledge, although the calculation of the stopping distance under R 4 corrections was performed by [52], the R 2 corrections on this quantity have never been addressed in the literature.…”

Section: Introductionmentioning

confidence: 99%

Light quark jet quenching in higher-derivative gravity

2023

Self Cite

View full text Add to dashboard Cite

We study finite-coupling corrections on the energy loss of light quarks in strongly coupled $${\mathcal {N}}=4$$ N = 4 super Yang–Mills (SYM) plasma. We perform the analysis by computing the stopping distance of an image jet induced by a massless source field, characterized by a massless particle falling along the null geodesic in Einstein gravity with curvature-squared ($$R^2$$ R 2 ) corrections. It turns out that the stopping distance in the $$R^2$$ R 2 theories can be larger or smaller than its SYM counterpart depending on the higher-derivative coefficients. Moreover, we evaluate the stopping distance in the Gauss–Bonnet background and find that increasing $$\lambda _\textrm{GB}$$ λ GB (a dimensionless parameter in Gauss–Bonnet gravity) leads to a decrease in the stopping distance, thus enhancing the energy loss of light quarks, in agreement with previous findings for the drag force, jet quenching parameter, and the instantaneous energy loss of light quarks using shooting strings.

show abstract

“…Hashimoto et al, calculating for the first time the entropic force associated with the heavy quark pair using the AdS/CFT correspondence [28], showed that the entropy increases with the inter-quark distance and the peak of the entropy depends on the nature of deconfinement and emerges near the transition point. After those, the entropic force was calculated by using this method several times, for example, for a moving [29] and rotating quarkonium [30], a moving dipole in a Yang-Mills like theory [31], for the chemical potential effect [32], R 2 and R 4 corrections [33] and for the effect of deformation parameter [34].…”

Section: Introductionmentioning

confidence: 99%

The imaginary potential and entropic force of heavy quarkonia in strongly coupled $$ {\mathcal {N}}=4 $$ supersymmetric Yang–Mills plasma on the Coulomb branch

Kioumarsipour

Sadeghi

2022

Eur. Phys. J. C

View full text Add to dashboard Cite

There are two important different mechanisms, the imaginary potential and entropic force, to investigate the dissociation of heavy quarkonia. In this paper, we calculate these two quantities for static and moving quarkonia in the rotating black 3-brane Type IIB supergravity solution dual to $$ {\mathcal {N}}=4 $$ N = 4 super Yang–Mills theory on the Coulomb branch (cSYM) at strong coupling. At $$ T\ne 0 $$ T ≠ 0 , there are two black hole branches: the large and small black hole branches. We investigate the effects of rotating parameter and rapidity for the static and moving quakonium at the large and small black hole branches. We find both mechanisms have the same results. In the large black hole branch: as $$ T/\Lambda $$ T / Λ and $$ \beta $$ β increase the thermal width decreases and so the suppression becomes stronger. In the small black hole branch: increasing $$ T/\Lambda $$ T / Λ leads to increasing the thermal width and the quarkonium dissociates harder but $$ \beta $$ β has an opposite effect.

show abstract

Higher derivative corrections to the entropic force from holography

Cited by 12 publications

References 49 publications

Phase transitions and entropy force of charged de Sitter black holes with cloud of string and quintessence

Phase transitions and entropy force of charged de Sitter black holes with cloud of string and quintessence

Light quark jet quenching in higher-derivative gravity

The imaginary potential and entropic force of heavy quarkonia in strongly coupled $$ {\mathcal {N}}=4 $$ supersymmetric Yang–Mills plasma on the Coulomb branch

Contact Info

Product

Resources

About