Nonlocal effective actions in semiclassical gravity: thermal effects in stationary geometries

Understand

We compute the gravitational effective action by integrating out quantum matter fields in a weak gravitational field, using the Schwinger-Keldysh (in-in) formalism.

• We pay particular attention to the role of the initial quantum state in the structure of the nonlocal terms in the effective action, with an eye to nonlinear completions of the theory that may be relevant in astrophysics and cosmology.
• In this first paper we consider a quantum scalar field in thermal equilibrium, in a stationary gravitational field.
• We obtain a covariant expression for the nonlocal effective action, that can be expressed in terms of the curvature tensor, the four-velocity of the thermal bath and the local Tolman temperature.