Pith. sign in

REVIEW

Equivalence between the in-in perturbation theories for quantum fields in Minkowski spacetime and in the Rindler wedge

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2001.05500 v2 pith:QEOPUA5P submitted 2020-01-15 gr-qc hep-th

classification gr-qchep-th
keywords in-incorrelationfunctionsrindlerminkowskivacuumwedgeexpansion
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We investigate the relation between the time-ordered vacuum correlation functions for interacting real scalar fields in Minkowski spacetime and in the Rindler wedge. The correlation functions are constructed perturbatively within the in-in formalism, often employed in calculations in more general spacetimes. We prove to all orders in perturbation theory that the time-ordered vacuum correlation functions can be calculated in the in-in formalism with internal vertices restricted to any Rindler wedge containing the external points. This implies that the Minkowski in-in (or in-out) perturbative expansion of the vacuum correlation functions is reproduced by the Rindler in-in perturbative expansion of these correlators in a thermal state at the Unruh temperature.

Discussion (0). Continue with ORCID to comment.

Pith tools