2023
DOI: 10.1007/jhep05(2023)122
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Causality constraints on corrections to Einstein gravity

Abstract: We study constraints from causality and unitarity on 2 → 2 graviton scattering in four-dimensional weakly-coupled effective field theories. Together, causality and unitarity imply dispersion relations that connect low-energy observables to high-energy data. Using such dispersion relations, we derive two-sided bounds on gravitational Wilson coefficients in terms of the mass M of new higher-spin states. Our bounds imply that gravitational interactions must shut off uniformly in the limit G → 0, and prove the sca… Show more

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Cited by 44 publications
(27 citation statements)
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References 87 publications
(153 reference statements)
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“…19 In writing (18) and (19) we took into account the fact that A and B are nonidentical particles. 20 The situation in d = 5 is analogous to the simple example discussed in [49]. 21 In the gapped theories the situation is exactly the same [50].…”
Section: Partial Wave Expansionmentioning
confidence: 84%
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“…19 In writing (18) and (19) we took into account the fact that A and B are nonidentical particles. 20 The situation in d = 5 is analogous to the simple example discussed in [49]. 21 In the gapped theories the situation is exactly the same [50].…”
Section: Partial Wave Expansionmentioning
confidence: 84%
“…5 In the most conservative Born model and d = 5, it requires that b > 0. 6 This point has been recently emphasized in [20]. 7 In the context of AdS/CFT the corresponding bound is related to the bound on chaos, see appendix A in [26].…”
Section: Local Growth Boundsmentioning
confidence: 95%
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“…Among possible future directions, it would be especially interesting to investigate how one might isolate string theory in the N = 4 supersymmetric EFT-hedron in a more generic way. Other than imposing monodromy (or that the low-energy amplitude must satisfy some double- 17 The Veneziano amplitude can also be written as A str [zz z z] = (α ′ s) 2 sin(πα ′ t) π Γ(−α ′ s)Γ(−α ′ t)Γ(−α ′ u). (7.17) In this form, its low-energy expansion takes the form of (7.13) with some particular set of ã′ k,q coefficients.…”
Section: Discussionmentioning
confidence: 99%
“…These basic high-energy assumptions facilitate a dispersive representation of the Wilson coefficients which implies that they must lie in a convex region sometimes called the "EFT-hedron" [2]. The allowed region of Wilson coefficients has been explored recently for theories of massless particles, including for scalars [2][3][4], massless pions [5][6][7][8][9][10], photons [11][12][13][14][15], and gravitons [16,17].…”
Section: Introductionmentioning
confidence: 99%