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Higher Dimensional Charged Rotating Solutions in (A)dS Space-times

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arxiv hep-th/0209238 v3 pith:4GNDFPS3 submitted 2002-09-27 hep-th

Adel Awad (U. of Cincinnati) This is my paper · ORCID
classification hep-th
keywords solutionsblackcalculatechargedrotatingspace-timesangularanti
verification ladder T0 review T1 audit T2 compute T3 formal
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We present a class of solutions to the Einstein-Maxwell equations in d-dimensions, all of which are asymptotically (anti)-de Sitter space-times. They describe electrically charged rotating solutions, which are generalizations of those found by Lemos (gr-qc/9404041). These solutions have toroidal, planar or cylindrical horizons and can be interpreted as black holes, or black strings/branes. We calculate the inverse temperature and entropy, and then we use the Brown-York stress-tensor to calculate mass and angular momenta of these solutions.

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Cited by 5 Pith papers

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

  1. Thermodynamics of charged rotating black strings in extended phase space

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    Charged rotating AdS black strings show a specific-heat divergence that is interpreted as a second-order, Van der Waals-like critical point, while uncharged strings show no such criticality.

  2. Weyl double copy in Lifshitz spacetimes

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    The regularization prescription for the Weyl double copy restores consistency with the Kerr-Schild double copy across three distinct Lifshitz black hole examples.

  3. Topological Thermodynamics of Black Holes: Revisiting the methods of winding numbers calculation

    gr-qc 2025-11 conditional novelty 4.0 of 10

    The φ-mapping and residue methods for black-hole winding numbers are proven equivalent when M''S'−S''M'≠0, and neutral and charged black strings both have W=+1.

  4. Rotating and non-rotating AdS black holes in $f({\cal T})$ gravity non-linear electrodynamics

    gr-qc 2019-08 conditional novelty 4.0 of 10

    New charged AdS black hole solutions are constructed for quadratic f(T) gravity with a specific nonlinear electrodynamics source, generalizing earlier Maxwell solutions and producing entropy that deviates from the area law.

  5. Imaginary potential and thermal width in the spinning black hole background from holography

    hep-ph 2025-01 conditional novelty 3.0 of 10

    In the planar limit of the Myers-Perry black hole, increasing the boost parameter makes the imaginary quarkonium potential appear at smaller separations and enlarges the thermal width, most strongly for transverse pai...

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