Papers
Topics
Authors
Recent
Search
2000 character limit reached

Topology of dyonic AdS black holes with quasitopological electromagnetism in Einstein-Gauss-Bonnet gravity

Published 21 Mar 2024 in gr-qc | (2403.14730v2)

Abstract: In this study, we employ the thermodynamic topological method to classify critical points for the dyonic AdS black holes with quasitopological electromagnetism in the Einstein-Gauss-Bonnet background. To this end, we find a small/large black hole phase transition in all dimensions of space-time, the existence of a conventional critical point implies a total topological charge of $Q_t=-1$. The coupling constant $\alpha$ gives rise to a more intricate phase structure, with the emergence of a triple points requires $\alpha\geq0.5$ and $d=6$. Interestingly, the condition for the occurrence of small/intermediate/large phase transition is that the coupling constant a takes a special value ($\alpha=0.5$), the two conventional critical points $CP_{1},CP_{2}$ of the black hole are physical critical point, and the novel critical point $CP_{3}$ that lacks the capability to minimize the Gibbs free energy. The critical points $CP_{1}$ and $CP_{2}$ are observed to occur at the maximum extreme points of temperature in the isobaric curve, while the critical point $CP_{3}$, emerges at the minimum extreme points of temperature. Furthermore, the number of phases at the novel critical point exhibits an upward trend, followed by a subsequent decline at the conventional critical points. With the increase of the coupling constant ($\alpha = 1$), although the system has three critical points, only the conventional $CP_{1}$ is a (physical) critical point, and the conventional $CP_{2}$ serves as the phase annihilation point. This means that the coupling constant $\alpha$ has a non-negligible effect on the phase structure.

Definition Search Book Streamline Icon: https://streamlinehq.com
References (16)
  1. S. H. Hendi and M. H. Vahidinia, Phys. Rev. D 88 (2012) 084045.
  2. S. W. Wei and Y. X. Liu, Phys. Rev. D 87 (2013) 044014.
  3. P.Ku. Yerra and C. Bhamidipati, Phys.Rev.D 105 (2022) 104053.
  4. P.Ku. Yerra and C. Bhamidipati, Phys. Lett B 835 (2022) 137591.
  5. P.Ku. Yerra and C. Bhamidipati, Phys. Rev. D 106 (2022) 064059.
  6. N.J. Gogoiand P. Phukon, Phys. Rev. D 107 (2023) 106009.
  7. D.Wu, Eur.Phys.J.C 83 (2023) 365.
  8. D.Wu, Eur.Phys.J.C 83 (2023) 589.
  9. D.Wu, Phys.Rev.D 107 (2023) 084002.
  10. D.Wu, Phys.Rev.D 107 (2023) 024024.
  11. D.Wu, Phys.Rev.D 108 (2023) 084041.
  12. D. Chen, Y. He and J. Tao Eur. Phys. J. C 83 (2023) 872.
  13. J. X. Mo and W. B. Liu, Phys. Rev. D 89 (2014) 084057.
  14. D. Glavan and C. Lin, Phys. Rev. Lett. 124 (2020) 081301.
  15. E. Babichev and A. Fabbri, Phys. Rev. D 90 (2014) 084019.
  16. A. Dehghani and S.H. Hendi, Phys. Rev. D 104 (2021) 024025.
Citations (11)

Summary

Paper to Video (Beta)

Whiteboard

No one has generated a whiteboard explanation for this paper yet.

Open Problems

We haven't generated a list of open problems mentioned in this paper yet.

Continue Learning

We haven't generated follow-up questions for this paper yet.

Collections

Sign up for free to add this paper to one or more collections.

Tweets

Sign up for free to view the 1 tweet with 2 likes about this paper.