1986
DOI: 10.1016/0370-2693(86)90763-x
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Gauge fields of any spin and symmetry

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Cited by 127 publications
(174 citation statements)
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“…Here we emphasize a crucial -though not completely uncontroversial -standpoint, namely that the string tension is a background dependent quantity determined by the solution, whereby tensionless limits [22,23,24,25] open windows into the Landscape which may ultimately turn out to be wider than those offered by traditional tensile strings and supergravity. Moreover, since excitations of strings and other extended objects carry general angular momenta, the unifying algebra must incorporate higher-spin symmetries [1,26,27,28,4,6,7,29] (see also [30]).…”
Section: Discussionmentioning
confidence: 95%
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“…Here we emphasize a crucial -though not completely uncontroversial -standpoint, namely that the string tension is a background dependent quantity determined by the solution, whereby tensionless limits [22,23,24,25] open windows into the Landscape which may ultimately turn out to be wider than those offered by traditional tensile strings and supergravity. Moreover, since excitations of strings and other extended objects carry general angular momenta, the unifying algebra must incorporate higher-spin symmetries [1,26,27,28,4,6,7,29] (see also [30]).…”
Section: Discussionmentioning
confidence: 95%
“…Indeed, the resemblance between the spectrum of massless fields (1.4) and the tensionless limit of the leading flat-space Regge trajectory [23,66,60,67] can be made into a more precise correspondence, which includes massive multi-singletons and higher trajectories, by using supersymmetry and holography arguments [68,69,37,40,70]. Clearly, this motivates establishing a more direct link between the phase-space approach and the tensionless limit of (bosonic) p-branes in anti-de Sitter spacetime.…”
Section: Higher-spin Gauge Theory and Singleton Stringsmentioning
confidence: 99%
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“…As we will show in this work, they provide an alternative route to the description of massless higher spins in their full generality, finding their original inspiration in the so-called TDiff-invariant spin-2 theories originally considered in [40,41] and more recently in [42] in connection with unimodular gravity and with the cosmological constant problem. Moreover, in a number of cases one can relate transverse-invariant theories to the triplet Lagrangians emerging from the tensionless limit of the free open string [34,30,35], of which they effectively provide a simplified version retaining the same particle content.…”
Section: Symmetric Tensorsmentioning
confidence: 99%
“…The BRST charge Q that results from this theory is of course precisely the one that produces an infinite tower of gauge fields with actions unified in Φ|Q|Φ [4,5,6,7] 1 .…”
Section: Constraintsmentioning
confidence: 99%