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Charged Rotating Dilaton Black Strings

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arxiv hep-th/0412049 v2 pith:ORPWYL2U submitted 2004-12-06 hep-th

classification hep-th
keywords solutionsblackfindfirstrotatingchargedgravityhole
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abstract

In this paper we, first, present a class of charged rotating solutions in four-dimensional Einstein-Maxwell-dilaton gravity with zero and Liouville-type potentials. We find that these solutions can present a black hole/string with two regular horizons, an extreme black hole or a naked singularity provided the parameters of the solutions are chosen suitable. We also compute the conserved and thermodynamic quantities, and show that they satisfy the first law of thermodynamics. Second, we obtain the ($n+1$%)-dimensional rotating solutions in Einstein-dilaton gravity with Liouville-type potential. We find that these solutions can present black branes, naked singularities or spacetimes with cosmological horizon if one chooses the parameters of the solutions correctly. Again, we find that the thermodynamic quantities of these solutions satisfy the first law of thermodynamics.

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

    gr-qc 2025-01 conditional novelty 6.0 of 10

    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.

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