Abstract

We study the scattering problem in the static patch of de Sitter space, i.e. the problem of field evolution between the past and future horizons of a de Sitter observer. We formulate the problem in terms of off-shell fields in Poincare coordinates. This is especially convenient for conformal theories, where the static patch can be viewed as a flat causal diamond, with one tip at the origin and the other at timelike infinity. As an important example, we consider Yang-Mills theory at tree level. We find that static-patch scattering for Yang-Mills is subject to BCFW-like recursion relations. These can reduce any static-patch amplitude to one with N−1MHV helicity structure, dressed by ordinary Minkowski amplitudes. We derive all the N−1MHV static-patch amplitudes from self-dual Yang-Mills field solutions. Using the recursion relations, we then derive from these an infinite set of MHV amplitudes, with arbitrary number of external legs.

Highlights

  • We study the scattering problem in the static patch of de Sitter space, i.e. the problem of field evolution between the past and future horizons of a de Sitter observer

  • We formulate the problem in terms of off-shell fields in Poincare coordinates. This is especially convenient for conformal theories, where the static patch can be viewed as a flat causal diamond, with one tip at the origin and the other at timelike infinity

  • We find that static-patch scattering for Yang-Mills is subject to BCFW-like recursion relations

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Summary

Outline of the paper

It is crucial to set up the calculation in a way that makes best use of available symmetries. In [9], we proposed a general strategy for the static-patch problem, which makes use of the larger symmetry of dS4 as a whole This involves artificially extending the static patch’s boundaries into geodesically complete cosmological horizons, each one defining a Poincare patch. For Yang-Mills theory, the static-patch scattering problem, while less trivial than the Minkowski S-matrix, is easier than standard (A)dS boundary correlators, despite having nominally lower symmetry. The results for these amplitudes are given in eqs. These are given in eqs. (5.2)–(5.3). section 6 is devoted to discussion and outlook

Geometry and kinematics
Flat coordinates adapted to past horizon
Lightlike plane waves and initial horizon data
Non-linear corrections and final horizon data
Self-dual solution
Anti-self-dual field strength perturbation
Minkowski S-matrix as special case of the static-patch amplitudes
BCFW-type recursion
Comparison with scalar field theory
Proof of the recursion for Yang-Mills theory
MHV scattering
Discussion
Full Text
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