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Analytically Approximation Solution to Einstein-Cubic Gravity

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arxiv 2207.13435 v1 pith:L2MHUWAY submitted 2022-07-27 gr-qc hep-th

Analytically Approximation Solution to Einstein-Cubic Gravity

classification gr-qc hep-th
keywords solutionsobtainanalyticapproximateblackeinstein-cubicfirstgravity
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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In this work, we introduce an analytical approximate black hole solution in Einstein-Cubic gravity. To obtain complete solutions, we construct the near horizon and asymptotic solutions as the first step. Then, the approximate analytic solutions are obtained through continued fraction expansion. We also compute the thermodynamic quantities and use the first law and Smarr formula to obtain the analytic solutions for the near horizon quantities. Finally, we follow the same approach to obtain the new static black hole solutions with different metric functions.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Static stable timelike circular orbits and Aschenbach effect in horizonless solutions of Einsteinian cubic gravity

    gr-qc 2026-01 conditional novelty 6.0

    In Einsteinian cubic gravity, horizonless solutions possess static stable circular orbits at the ISCO, with a non-monotonic ZAMO velocity profile (Aschenbach effect).