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Thermodynamic Topology of $D=4,5$ Horava Lifshitz Black Hole in Two Ensembles

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arxiv 2312.06324 v1 pith:BM2HBEA6 submitted 2023-12-11 hep-th gr-qc

classification hep-thgr-qc
keywords horizonblackensemblefixedholeshoravathermodynamicdifferent
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abstract

We study the thermodynamic topology of four and five dimensional Horava Lifshitz (HL) black holes in Horava gravity. These exotic black hole solutions belong to a special class of of black holes whose thermodynamics exhibit a line of (continuous) second order phase transitions known as $\lambda$ phase transitions akin to those observed in the superfluidity of liquid $^{4}He$. To analyze their thermodynamic topology, we treat the Horava Lifshitz (HL) black holes as topological defects in their thermodynamic spaces and compute the winding numbers at those defects. We work in two different ensembles: fixed $\epsilon$ ensemble and fixed $\zeta$ ensemble, where $\epsilon$ is a parameter of the HL black holes and $\zeta$ is its conjugate parameter. In the fixed $\epsilon$ ensemble, three different horizon types are considered : the spherical horizon for $k=+1$, the flat horizon for $k=0$, and the hyperbolic horizon for $k=-1$. In the fixed $\zeta$ ensemble, two different horizon types are considered : the spherical horizon for $k=+1$, and the hyperbolic horizon for $k=-1$.

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Cited by 2 Pith papers

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

  1. Holographic Fractional Order Phase Transitions in CFTs Dual to AdS Black Holes

    hep-th 2025-06 conditional novelty 5.0 of 10

    The paper finds that holographic CFT phase transitions at Davies temperature-extremum points are of fractional order 3/2, while those at inflection critical points are of order 4/3, for several AdS black hole models.

  2. Probing Thermodynamic Phase Transitions of 4D R-Charged Black Holes via Lyapunov Exponent

    gr-qc 2025-05 conditional novelty 4.0 of 10

    For 4D R-charged black holes, the Lyapunov exponent of unstable circular orbits tracks black hole phase transitions, and its discontinuity near the critical point shows a universal critical exponent of 1/2.

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