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dc.contributor.authorPajer, Enrico
dc.contributor.authorStefanyszyn, David
dc.contributor.authorSupeł, Jakub
dc.date.accessioned2021-01-02T16:16:44Z
dc.date.available2021-01-02T16:16:44Z
dc.date.issued2020-12-30
dc.date.submitted2020-08-05
dc.identifier.otherjhep12(2020)198
dc.identifier.other14487
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/315649
dc.description.abstractAbstract: Poincaré invariance is a well-tested symmetry of nature and sits at the core of our description of relativistic particles and gravity. At the same time, in most systems Poincaré invariance is not a symmetry of the ground state and is hence broken spontaneously. This phenomenon is ubiquitous in cosmology where Lorentz boosts are spontaneously broken by the existence of a preferred reference frame in which the universe is homogeneous and isotropic. This motivates us to study scattering amplitudes without requiring invariance of the interactions under Lorentz boosts. In particular, using on-shell methods and assuming massless, relativistic and luminal particles of any spin, we show that the allowed interactions around Minkowski spacetime are severely constrained by unitarity and locality in the form of consistent factorization. The existence of an interacting massless spin-2 particle enforces (analytically continued) three-particle amplitudes to be Lorentz invariant, even those that do not involve a graviton, such as cubic scalar couplings. We conjecture this to be true for all n-particle amplitudes. Also, particles of spin S > 2 cannot self-interact nor can be minimally coupled to gravity, while particles of spin S > 1 cannot have electric charge. Given the growing evidence that free gravitons are well described by massless, luminal relativistic particles, our results imply that cubic graviton interactions in Minkowski must be those of general relativity up to a unique Lorentz-invariant higher-derivative correction of mass dimension 9. Finally, we point out that consistent factorization for massless particles is highly IR sensitive and therefore our powerful flat-space results do not straightforwardly apply to curved spacetime.
dc.languageen
dc.publisherSpringer Berlin Heidelberg
dc.rightsAttribution 4.0 International (CC BY 4.0)en
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en
dc.subjectRegular Article - Theoretical Physics
dc.subjectScattering Amplitudes
dc.subjectSpontaneous Symmetry Breaking
dc.subjectSpace-Time Sym- metries
dc.titleThe boostless bootstrap: amplitudes without Lorentz boosts
dc.typeArticle
dc.date.updated2021-01-02T16:16:43Z
prism.issueIdentifier12
prism.publicationNameJournal of High Energy Physics
prism.volume2020
dc.identifier.doi10.17863/CAM.62763
dcterms.dateAccepted2020-10-30
rioxxterms.versionofrecord10.1007/jhep12(2020)198
rioxxterms.versionVoR
rioxxterms.licenseref.urihttp://creativecommons.org/licenses/by/4.0/
dc.contributor.orcidPajer, Enrico [0000-0002-7921-4479]
dc.identifier.eissn1029-8479
dc.identifier.arxiv2007.00027


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Attribution 4.0 International (CC BY 4.0)
Except where otherwise noted, this item's licence is described as Attribution 4.0 International (CC BY 4.0)