2020
DOI: 10.1103/physrevd.102.083508
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New class of Proca interactions

Abstract: We propose a new class of Proca interactions that enjoy a nontrivial constraint and hence propagates the correct number of degrees of freedom for a healthy massive spin-1 field. We show that the scattering amplitudes always differ from those of the Generalized Proca. This implies that the new class of interactions proposed here are genuinely different from the Generalized Proca and there can be no local field redefinitions between the two. In curved spacetime, massive gravity is the natural covariantization, b… Show more

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Cited by 38 publications
(39 citation statements)
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“…It would be intriguing to explore whether this hypothesis might be dropped in order for the Proca and DHOST constraints to be realized in a way that would mix the canonical momenta associated with the vector and scalar fields. We remark that a related generalization of the Proca constraint has been studied recently in [56] in the context of pure vector-tensor theories. We plan to revisit these questions in future work.…”
Section: Discussionmentioning
confidence: 94%
“…It would be intriguing to explore whether this hypothesis might be dropped in order for the Proca and DHOST constraints to be realized in a way that would mix the canonical momenta associated with the vector and scalar fields. We remark that a related generalization of the Proca constraint has been studied recently in [56] in the context of pure vector-tensor theories. We plan to revisit these questions in future work.…”
Section: Discussionmentioning
confidence: 94%
“…It would be intriguing to explore if this hypothesis might be dropped in order for the Proca and DHOST constraints to be realized in a way that would mix the canonical momenta associated to the vector and scalar fields. We remark that a related generalization of the Proca constraint has been studied recently in [59] in the context of pure vector-tensor theories. We plan to revisit these questions in future work.…”
Section: Discussionmentioning
confidence: 94%
“…Irrespectively of their precise origin, from a gravitational four-dimensional perspective, these extra degrees of freedom can most of the time be associated with additional helicity-0, -1 or -2 modes. The effect of the helicity-1 modes can often be associated with a generalized Proca model (see for instance [57][58][59][60][61][62][63][64][65][66][67]), although since all such Lorentz-invariant effective field theories also carry a helicity-0 mode, to start with we shall focus on the effect on a helicity-0 degrees of freedom. Taking an effective field theory point of view, one can construct the most general theories that involve a helicity-0 mode besides the standard helicity-2 ones that appear in GR.…”
Section: Introductionmentioning
confidence: 99%