Thermal Casimir Effect in Kerr Space-time
arXiv:1710.03101 · doi:10.1016/j.nuclphysb.2015.07.002
Abstract
We investigate the thermal Casimir effect of a massless scalar field for two parallel plates moving in the equatorial orbit in Kerr space-time. Under the assumption that the typical cavity size is much smaller than the orbital radius, proposed by Sorge, we deduce the analytical expression of the renormalized free energy in this curved space-time. We also get the analytical representation for the renormalized internal energy, and find that there is a thermal correction to the Casimir energy, which depends on the proper temperature and the proper geometrical parameters of the plates. The asymptotic behavior of the Casimir free energy, entropy and internal energy at low temperature is also investigated.
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Cited by in corpus (7)
- Casimir Effect in the Kerr Spacetime with Quintessence
- Casimir Effect in a Schwarzschild-Like Wormhole Spacetime
- Theoretical analysis of Casimir and thermal Casimir effect in stationary space-time
- Thermal Casimir effect in Kerr spacetime with quintessence and massive gravitons
- Thermal Casimir effect for a Dirac field on flat space with a nontrivial circular boundary condition
- Scattering approach for calculating one-loop effective action and vacuum energy
- Thermal Casimir effect in -Minkowski space-time