Classical Space-Times from the S Matrix
Duff Neill (MIT), Ira Z. Rothstein (CMU)

TL;DR
This paper demonstrates deriving classical space-times, like Schwarzschild, directly from the S-matrix without using Einstein's equations, employing on-shell techniques and revealing connections between gravity and Yang-Mills solutions.
Contribution
It introduces a method to obtain classical space-times from the S-matrix alone, bypassing the Einstein-Hilbert action, and extends the approach to Yang-Mills solutions, highlighting algebraic relations.
Findings
Derived Schwarzschild space-time from S-matrix as a series in G_N.
Showed that space-times can be obtained without Einstein-Hilbert action.
Linked gravity and Yang-Mills solutions via algebraic relations.
Abstract
We show that classical space-times can be derived directly from the S-matrix for a theory of massive particles coupled to a massless spin two particle. As an explicit example we derive the Schwarzchild space-time as a series in . At no point of the derivation is any use made of the Einstein-Hilbert action or the Einstein equations. The intermediate steps involve only on-shell S-matrix elements which are generated via BCFW recursion relations and unitarity sewing techniques. The notion of a space-time metric is only introduced at the end of the calculation where it is extracted by matching the potential determined by the S-matrix to the geodesic motion of a test particle. Other static space-times such as Kerr follow in a similar manner. Furthermore, given that the procedure is action independent and depends only upon the choice of the representation of the little group, solutions to…
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