Abstract
Based on the idea that the vacuum fluctuations of electromagnetic fields can induce instantaneous correlated dipoles, we study the far-zone Casimir-Polder potential between two atoms in the Boulware, Unruh, and Hartle-Hawking vacua outside a Schwarzschild black hole. We show that at spatial infinity, the Casimir-Polder potential in the Boulware vacuum is similar to that in the Minkowski vacuum in flat space-time with a behavior of R7, so it is in the Unruh vacuum as a result of the backscattering of the Hawking radiation from the black hole off the space-time curvature. However, the interatomic Casimir-Polder potential in the Hartle-Hawking vacuum behaves like that in a thermal bath at the Hawking temperature. In the region near the event horizon of the black hole, the modifications caused by the space-time curvature make the interatomic Casimir-Polder potential smaller in all three vacuum states. DOI: http://dx.doi.org/10.1103/PhysRevA.88.064501 ©2013 American Physical Society