Small-ν correction to the AdS Hagedorn temperature
Determine the leading ν-dependent correction to the Hagedorn temperature R_H(ν) for rotating thermal AdS backgrounds in type II string theory in the limit ν ≪ l_s/l_ads, i.e., compute R_H(ν) when ν acts as a perturbation at finite l_s/l_ads beyond the ν-independent strong-coupling expansion.
References
Finally, we could consider a different limit where \nu \ll l_{ads}. In this limit, \nu is a perturbation of the full AdS computation. Since we don't have control over the \nu=0 behavior for finite l_s/l_{ads}, it is difficult to analyze the leading correction to it by \nu. We therefore cannot say anything valuable about this limit.
— A spin on Hagedorn temperatures and string stars
(2510.17951 - Seitz et al., 20 Oct 2025) in Section 5.1 (The Hagedorn temperature of rotating thermal AdS)