2021
DOI: 10.1016/j.nuclphysb.2021.115362
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Black string in massive gravity

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Cited by 13 publications
(16 citation statements)
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“…It is expected that the quantum corrections to the black M2-M5 bound state will modify the thermodynamic stability of this solution. Such modification to the thermodynamic behavior from quantum corrections has been studied for various black objects [46][47][48][49]. The stability of this system can be investigated using its specific heat C = T 0 (∂S/∂T 0 ).…”
Section: Quantum Effective Informational Metricsmentioning
confidence: 99%
See 2 more Smart Citations

Quantum Thermodynamics of an M2-M5 Brane System

Pourhassan,
Aounallah,
Faizal
et al. 2022
Preprint
Self Cite
“…It is expected that the quantum corrections to the black M2-M5 bound state will modify the thermodynamic stability of this solution. Such modification to the thermodynamic behavior from quantum corrections has been studied for various black objects [46][47][48][49]. The stability of this system can be investigated using its specific heat C = T 0 (∂S/∂T 0 ).…”
Section: Quantum Effective Informational Metricsmentioning
confidence: 99%
“…Thus, it possible to use the Jacobson formalism to investigate the quantum fluctuation to the geometry of spacetime using the thermal fluctuations [45]. Thus, motivated from Jacobson formalism, the thermal fluctuations have been used to analyze quantum fluctuations of various black hole solutions [46][47][48][49]. These thermal fluctuations can be neglected for large black holes because the temperature of black holes scales inversely with their size.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation

Quantum Thermodynamics of an M2-M5 Brane System

Pourhassan,
Aounallah,
Faizal
et al. 2022
Preprint
Self Cite
“…Generically, black strings are higher-dimensional asymptotically flat vacuum solutions with extended topology of their horizon that represent interesting counterexamples to topological censorship [38] and to uniqueness theorems in higher-dimensional GR [39][40][41]. They are also known in the presence of nonlinear matter content and in theories beyond GR (for an incomplete list of developments see [28,[42][43][44][45][46][47][48][49][50][51][52][53]). Nevertheless, it is well-known that these solutions usually suffer from the Gregory-Laflamme instability: a long-wavelength linear instability driven by an unstable mode traveling along the extended direction [33,54,55].…”
Section: Introductionmentioning
confidence: 99%
“…Since the dRGT solution is one of solutions with asymptotically dS/AdS spacetime, it is possible to obtain the black string solution [42]. Consequently, the solution for the charged black string as well as rotating black string are explored [43,44].…”
Section: Introductionmentioning
confidence: 99%