Answers are grounded in this paper and cite their sources.
We study black hole solutions in R⁴×S¹ space, using an expansion to second order in the square of the ratio of the radius of the horizon, μ, and the circumference of the compact dimension, L. A study of geometric and thermodynamic properties indicates that the black hole fills the space in the compact dimension at ϵ=(μ/L)²0.1. At the same value of $ϵ$ the entropies of the uniform black string and of the black hole are approximately equal.
No takes yet. Share an insight, caveat, or question.
Karasik et al. (2005) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: