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PreprintCC BY 4.0arXiv

Topological black holes of Einsteinian cubic gravity and Born-Infeld-type electrodynamics

  • Askar Ali
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Abstract

In this paper, we examine the new black holes of Einsteinian cubic gravity within the framework of Born-Infeld-type electrodynamics. Initially, we establish the differential equations of motion that characterize an innovative collection of charged black hole solutions in Einsteinian cubic theory. Next, we compute the thermodynamic quantities of these black holes for the case of vanishing bare cosmological constant. We consider this situation because the model is unitary only for the asymptotically flat solutions that allow horizons with spherical topology. We also present that the first law of thermodynamics is fulfilled for these objects. Finally, we examine how the nonlinearity of electric field, electric charge and cubic coupling parameter can impact the local thermal stability of our simulated black holes in both canonical and grand canonical ensembles.

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Cite

BibTeXRIS
BibTeX
@misc{ali2026topological,
  title = {{Topological black holes of Einsteinian cubic gravity and Born-Infeld-type electrodynamics}},
  author = {Askar Ali},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.30206},
  eprint = {2609.30206},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.30206},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Topological black holes of Einsteinian cubic gravity and Born-Infeld-type electrodynamics
AU  - Askar Ali
PY  - 2026
DA  - 2026/09/24
PB  - arXiv
DO  - 10.48550/arxiv.2609.30206
UR  - https://arxiv.org/abs/2609.30206
AB  - In this paper, we examine the new black holes of Einsteinian cubic gravity within the framework of Born-Infeld-type electrodynamics. Initially, we establish the differential equations of motion that characterize an innovative collection of charged black hole solutions in Einsteinian cubic theory. Next, we compute the thermodynamic quantities of these black holes for the case of vanishing bare cosmological constant. We consider this situation because the model is unitary only for the asymptotically flat solutions that allow horizons with spherical topology. We also present that the first law of thermodynamics is fulfilled for these objects. Finally, we examine how the nonlinearity of electric field, electric charge and cubic coupling parameter can impact the local thermal stability of our simulated black holes in both canonical and grand canonical ensembles.
ER  -