2021
DOI: 10.48550/arxiv.2112.11755
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Crossing Symmetric Spinning S-matrix Bootstrap: EFT bounds

Abstract: We develop crossing symmetric dispersion relations for describing 2-2 scattering of identical external particles carrying spin. This enables us to import techniques from Geometric Function Theory and study two sided bounds on low energy Wilson coefficients. We consider scattering of photons, gravitons in weakly coupled effective field theories. We provide general expressions for the locality/null constraints. Consideration of the positivity of the absorptive part leads to an interesting connection with the rec… Show more

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Cited by 6 publications
(15 citation statements)
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References 51 publications
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“…This conjecture was confirmed by the beautiful results of [93] where they used the power of the null-constraints together with the scattering amplitude in impact parameter space, or equivalently at −Λ 2 < t < 0 to define a set of positive integrals which could be used to constrain the leading s 2 terms in the scattering amplitudes even in the presence of the massless spin-2 pole. These bounds have been put on the leading order corrections to Einstein gravity in [94], complementing the results of [88][89][90]. An interesting observation is that strong bounds can be obtained by assuming that the lower spin partial waves dominate in the dispersion relation, as shown in explicit examples, via geometric function theory or via SDP numerically [88][89][90]94].…”
Section: Unitarity and Causality Bounds For Gravitational Eftsmentioning
confidence: 83%
See 3 more Smart Citations
“…This conjecture was confirmed by the beautiful results of [93] where they used the power of the null-constraints together with the scattering amplitude in impact parameter space, or equivalently at −Λ 2 < t < 0 to define a set of positive integrals which could be used to constrain the leading s 2 terms in the scattering amplitudes even in the presence of the massless spin-2 pole. These bounds have been put on the leading order corrections to Einstein gravity in [94], complementing the results of [88][89][90]. An interesting observation is that strong bounds can be obtained by assuming that the lower spin partial waves dominate in the dispersion relation, as shown in explicit examples, via geometric function theory or via SDP numerically [88][89][90]94].…”
Section: Unitarity and Causality Bounds For Gravitational Eftsmentioning
confidence: 83%
“…These bounds have been put on the leading order corrections to Einstein gravity in [94], complementing the results of [88][89][90]. An interesting observation is that strong bounds can be obtained by assuming that the lower spin partial waves dominate in the dispersion relation, as shown in explicit examples, via geometric function theory or via SDP numerically [88][89][90]94].…”
Section: Unitarity and Causality Bounds For Gravitational Eftsmentioning
confidence: 83%
See 2 more Smart Citations
“…As we will see, these Feynman blocks in the Celestial variables have remarkable properties. One of the main advantages of working with the CSDR is that it leads to a fascinating connection with an area of mathematics called Geometric Function Theory (GFT) [24][25][26]. The origin of two sided bounds on Wilson coefficients gets related to the famous Bieberbach conjecture (de Branges' theorem).…”
mentioning
confidence: 99%