Non-perturbative diffeomorphism invariance for doubled fields in Schwinger–Keldysh gravity
Establish a non-perturbative, diffeomorphism-invariant formulation of gravity within the Schwinger–Keldysh doubled-field formalism that enables a unitary-gauge derivation of the open Effective Field Theory of Inflation. Specifically, determine consistent rules for covariantizing indices in the presence of two metrics g^+_{\mu\nu} and g^-_{\mu\nu} (or mixed combinations) so that the ambiguity is resolved and the construction remains local, causal, and compatible with the diagonal symmetry action on the doubled fields.
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While doing this order by order in metric perturbations is straightforward, it is not clear to us how the non-perturbative and diffeomorphism invariant structure of gravity is organised when fields are doubled. For example, one seems to have infinitely many choices to covariantise indices using g_{\mu\nu}+, g_{\mu\nu}- or combinations thereof. We hope to come back to this issue in future research.