Hot Casimir wormholes

In this paper, we have for the first time considered the consequences of finite temperature contributions to a traversable wormhole. This was done by using finite temperature generalization of the Casimir effect as a source of a hot traversable wormhole. To include finite temperature effects, we have considered the plates positioned either parametrically fixed or radially varying. Such results have been obtained in both high and low-temperature regimes. We explicitly investigate the effect of such finite temperature corrections on the size of a traversable wormhole.