2018
DOI: 10.1016/j.physletb.2018.05.046
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Dual actions for massless, partially-massless and massive gravitons in (A)dS

Abstract: We provide a unified treatment of electric-magnetic duality, at the action level and with manifest Lorentz invariance, for massive, massless as well as partially-massless gravitons propagating in maximally symmetric spacetimes of any dimension n > 3 . For massive and massless fields, we complete previous analyses that use parent-action techniques by giving dual descriptions that enable direct counting of physical degrees of freedom in the flat and massless limit. The same treatment is extended to the partially… Show more

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Cited by 19 publications
(27 citation statements)
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“…One then uses (3.31) and the trace of (3.9), taking into account that, on shell, the traces of the four curvatures K a[n−2]|b , K C a[n−2]|bc , Q ab|cd and K ab|c vanish. We obtain Both together, they propagate the correct degrees of freedom for a partially massless spin-2 field in the flat limit, as was found and discussed in section 4.3 of [7]. The flat limit of (3.36) gives…”
Section: Partially-massless Twisted Dualitysupporting
confidence: 64%
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“…One then uses (3.31) and the trace of (3.9), taking into account that, on shell, the traces of the four curvatures K a[n−2]|b , K C a[n−2]|bc , Q ab|cd and K ab|c vanish. We obtain Both together, they propagate the correct degrees of freedom for a partially massless spin-2 field in the flat limit, as was found and discussed in section 4.3 of [7]. The flat limit of (3.36) gives…”
Section: Partially-massless Twisted Dualitysupporting
confidence: 64%
“…The equations of motion for the dual gauge fields C a[n−3]|b and T a[n−2]|b derived from the Lagrangian L 0 (C, T ) -obtained by substituting (2.18) in (2.9) and given in Eq. (23) of [7] -can be written in terms of the traces of the gauge-invariant curvatures K C a[n−2]|b [2] and K T a[n−1]|b [2] . Explicitly, one has 28) and the gauge invariant tensors X and V can be expressed as…”
Section: Dual Formulationmentioning
confidence: 99%
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“…Actually, PM fields can be defined around D-dimensional Anti-de Sitter (AdS D ) spacetime where they are classically non-unitary. This can be seen explicitly by writing the action, which is real for both signs of the cosmological constant, in the Stueckelberg formulation[11].…”
mentioning
confidence: 99%