Cardy-Verlinde Formula and entropy bounds in Kerr-Newman-AdS$_4$/dS$_4$ black holes backgrounds
Jiliang Jing

TL;DR
This paper verifies the Cardy-Verlinde formula for Kerr-Newman-AdS$_4$ and Kerr-Newman-dS$_4$ black holes, exploring entropy bounds and the roles of energy terms, supporting the dS/CFT correspondence.
Contribution
It extends the Cardy-Verlinde formula to Kerr-Newman-AdS$_4$ and Kerr-Newman-dS$_4$ black holes, clarifying energy contributions and entropy bounds in these spacetimes.
Findings
The Casimir energy must include rotational and electric potential terms.
The entropy bounds are tightened by electric charge.
Supports the dS/CFT correspondence through entropy analysis.
Abstract
The Cardy-Verlinde formula is further verified by using the Kerr-Newman-AdS and Kerr-Newman-dS black holes. In the Kerr-Newman-AdS spacetime, we find that, for strongly coupled CFTs with AdS duals, to cast the entropy of the CFT into the Cardy-Verlinde formula the Casimir energy must contains the terms , which associate with rotational and electric potential energies, and the extensive energy includes the term . For the Kerr-Newman-dS black hole, we note that the Casimir energy is negative but the extensive energy is positive on the cosmological horizon; while the Casimir energy is positive but the extensive energy is negative on the event horizon (the definitions for the two energies possess the same forms as the corresponding quantities of the Kerr-Newman-AdS black hole). Thus we have to…
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.
