Generalized Thermodynamic Properties of Lifshitz black holes
Keita Kaniba Mady, Dicko Younouss Hameye

TL;DR
This paper investigates the motion and thermodynamic properties of Lifshitz black holes, deriving generalized effective potentials, analyzing orbit stability, and confirming thermodynamic laws and entropy behavior in these exotic spacetimes.
Contribution
It introduces a generalized effective potential for Lifshitz black holes and derives their thermodynamic properties, including entropy, mass, and temperature, satisfying key thermodynamic principles.
Findings
Bounded orbits are forbidden for positive z and allowed for negative z.
Entropy can still follow the area law in these black holes.
Mass, temperature, and entropy satisfy thermodynamic laws and Smarr formula.
Abstract
The generalized effective potential for motion in Lifshitz geometry (with arbitrary value of both the dynamical exponent and ) is presented. Based on this effective potential energy, we shall show that bounded orbits are forbidden for positive values of and allowed for negative values of . The stability of these bounded orbits are analysed in full detail. Besides, by comparison, we quote a theorem which should be very helpful in searching thermodynamical properties of these gravitational black holes. Based on this theorem, generalized thermodynamic properties of Lifshitz black holes are computed. Examples are given where the entropy still satisfies the area law. The calculated mass, temperature and entropy satisfy both the first thermodynamic principle of black holes and a Smarr formula.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
