2021
DOI: 10.1007/jhep07(2021)083
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(2, 2) Scattering and the celestial torus

Abstract: Analytic continuation from Minkowski space to (2, 2) split signature spacetime has proven to be a powerful tool for the study of scattering amplitudes. Here we show that, under this continuation, null infinity becomes the product of a null interval with a celestial torus (replacing the celestial sphere) and has only one connected component. Spacelike and timelike infinity are time-periodic quotients of AdS3. These three components of infinity combine to an S3 represented as a toric fibration over the interval.… Show more

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Cited by 72 publications
(104 citation statements)
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“…The 2-spinors λ α , λ α denote its spinor-helicity variables. Working in Klein space R 2,2 [14] with flat metric of split signature (+ + − −), we take them to be real-valued and independent of each other. Under a little group scaling, |λ, λ, transforms as…”
Section: Preliminariesmentioning
confidence: 99%
See 1 more Smart Citation
“…The 2-spinors λ α , λ α denote its spinor-helicity variables. Working in Klein space R 2,2 [14] with flat metric of split signature (+ + − −), we take them to be real-valued and independent of each other. Under a little group scaling, |λ, λ, transforms as…”
Section: Preliminariesmentioning
confidence: 99%
“…In this work, we wish to focus on a refinement of the shadow transform in Lorentzian signature, namely the light transform. The authors of [14] studied CCFT on the celestial torus of flat space R 2,2 with a split signature metric. This is a Lorentzian CFT and hence contains light ray operators with analytically continued spins [2].…”
Section: Introductionmentioning
confidence: 99%
“…3 Throughout this paper we treat left and right movers as independent on the celestial sphere, which means we effectively work in (2, 2) signature, i.e. Klein space [62]. The SL(2, R)R here is the global subgroup of the VirR superrotations.…”
Section: Introductionmentioning
confidence: 99%
“…Recall we are working with independent left and right coordinates, i.e. (2, 2) signature[62] 15. To make connection with the standard four-point KLT formula as described in[74,75], it is convenient to set z1 = 1, z2 = 0 using SL(2, R) covariance and expand O (h P , hP ) (z3, z3) in powers of z3, z3.…”
mentioning
confidence: 99%
“…They do not however form representations of the Poincaré group. Another basis of interest[21] which do furnish Poincaré representations, and moreover include the soft currents[22] are those with real integral ∆. In this paper we assume that ∆ lies on the unitary principal series but many of our formulae can be generalized to the integral case.…”
mentioning
confidence: 99%