2019
DOI: 10.1007/jhep10(2019)189
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Massive higher spins: effective theory and consistency

Abstract: We construct the effective field theory for a single massive higher-spin particle in flat spacetime. Positivity bounds of the S-matrix force the cutoff of the theory to be well below the naive strong-coupling scale, forbid any potential and make therefore higher-derivative operators important even at low energy. As interesting application, we discuss in detail the massive spin-3 theory and show that an extended Galileon-like symmetry of the longitudinal modes, even with spin, emerges at high energy.1 arXiv:190… Show more

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Cited by 54 publications
(61 citation statements)
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“…[35,36]. This requirement of IR consistency has led to a program of bounding couplings in various EFTs of interest, including corrections to general relativity [37][38][39][40], nonlinear electrodynamics [34], massive gravity [41][42][43][44] and higher-spin states [45][46][47][48][49][50][51], certain scalar theories [52][53][54][55][56] including the proof of the four-dimensional a-theorem [57], the electroweak EFT [58,59], and Einstein-Maxwell theory with applications to the Weak Gravity Conjecture [60][61][62][63][64]. The IR consistency program, taking a bottom-up approach to constraining EFTs, has evolved in tandem with the swamp- Figure 1: Schematic depiction of bounds derived in this work.…”
Section: Introductionmentioning
confidence: 99%
“…[35,36]. This requirement of IR consistency has led to a program of bounding couplings in various EFTs of interest, including corrections to general relativity [37][38][39][40], nonlinear electrodynamics [34], massive gravity [41][42][43][44] and higher-spin states [45][46][47][48][49][50][51], certain scalar theories [52][53][54][55][56] including the proof of the four-dimensional a-theorem [57], the electroweak EFT [58,59], and Einstein-Maxwell theory with applications to the Weak Gravity Conjecture [60][61][62][63][64]. The IR consistency program, taking a bottom-up approach to constraining EFTs, has evolved in tandem with the swamp- Figure 1: Schematic depiction of bounds derived in this work.…”
Section: Introductionmentioning
confidence: 99%
“…We have considered k = 0 vector symmetries, but scalar-vector theories with abelian shift symmetries with higher values of k will also arise from the decoupling limits of massive higher-spin theories, as discussed in Ref. [67]. For example, the massive spin-3 scalar-vector decoupling limit interactions of Ref.…”
Section: Discussionmentioning
confidence: 99%
“…[67] have a non-trivial abelian k = 1 vector shift symmetry. This should generalize to arbitrary k using the decoupling limits of massive higher-spins that interact via special potentials that generalize the pseudo-linear interactions [67][68][69]. In Appendix C we write down these scalar-vector interactions explicitly for all even values of k.…”
Section: Discussionmentioning
confidence: 99%
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“…We note that even though the question at hand-what is the one-loop contribution from massive higher-spin states-is technically well posed, the regime of validity of the perturbative expansion is narrow: the higher-spin action is itself an effective action with a cutoff, and Ref. [35] showed that a single higher-spin particle cannot be parametrically lighter than this cutoff, so that a weak coupling treatment of isolated higher-spin particles is typically not possible.…”
Section: Bsm Perspectivementioning
confidence: 99%