Results 21 to 30 of about 269,645 (307)

Unitarity Bounds in AdS_3 Higher Spin Gravity [PDF]

open access: yesJournal of High Energy Physics, 2012
We study SL(N,R) Chern-Simons gauge theories in three dimensions. The choice of the embedding of SL(2,R) in SL(N,R), together with asymptotic boundary conditions, defines a theory of higher spin gravity.
A Achucarro   +39 more
core   +2 more sources

On the spectrum of pure higher spin gravity [PDF]

open access: yesJournal of High Energy Physics, 2020
We study the spectrum of pure massless higher spin theories in AdS3. The light spectrum is given by a tower of massless particles of spin s = 2, ⋯ , N and their multi-particles states. Their contribution to the torus partition function organises into the
L. Alday   +3 more
semanticscholar   +6 more sources

Classical Aspects of Higher Spin Topologically Massive Gravity [PDF]

open access: yesClassical and Quantum Gravity, 2012
We study the classical solutions of three dimensional topologically massive gravity (TMG) and its higher spin generalization, in the first order formulation.
Chen, Bin, Long, Jiang, Zhang, Jian-dong
core   +2 more sources

Black holes in Truncated Higher Spin AdS$_3$ Gravity [PDF]

open access: yesJournal of High Energy Physics, 2012
We study the higher spin black holes in a truncated version of higher spin gravity in $AdS_3$. This theory contains only finite number of even spins s=2,4,...,2N.
Chen, Bin, Long, Jiang, Wang, Yi-nan
core   +2 more sources

How higher-spin gravity surpasses the spin two barrier: no-go theorems versus yes-go examples [PDF]

open access: yesReviews of Modern Physics, 2012
Aiming at non-experts, we explain the key mechanisms of higher-spin extensions of ordinary gravity. We first overview various no-go theorems for low-energy scattering of massless particles in flat spacetime.
Bekaert, X.   +9 more
core   +5 more sources

Boundary freedom in higher spin gravity

open access: yesPhysics Letters B
We investigate new boundary conditions in three-dimensional asymptotically Anti–de Sitter gravity coupled to higher-spin fields, allowing for arbitrary boundary degrees of freedom.
Arnaud Delfante
doaj   +3 more sources

More on Chiral Higher Spin Gravity and convex geometry [PDF]

open access: yesNuclear Physics B, 2022
Recently, a unique class of local Higher Spin Gravities with propagating massless fields in $4d$ - Chiral Higher Spin Gravity - was given a covariant formulation both in flat and $(A)dS_4$ spacetimes at the level of equations of motion. We unfold the corresponding homological perturbation theory as to explicitly obtain all interaction vertices.
A. Sharapov   +3 more
semanticscholar   +6 more sources

Geometric tool kit for higher spin gravity (part I): An introduction to the geometry of differential operators [PDF]

open access: yesInternational Journal of Modern Physics A, 2023
These notes provide an introduction to the algebra and geometry of differential operators and jet bundles. Their point of view is guided by the leitmotiv that higher-spin gravity theories call for higher-order generalisations of Lie derivatives and ...
X. Bekaert
semanticscholar   +1 more source

Asymptotic dynamics of three dimensional supergravity and higher spin gravity revisited [PDF]

open access: yesJournal of High Energy Physics, 2023
We reconsider the Hamiltonian reduction of the action for three dimensional AdS supergravity and W3 higher spin AdS gravity in the Chern-Simons formulation under asymptotically anti-de Sitter boundary conditions.
Wout Merbis, Turmoli Neogi, A. Ranjbar
semanticscholar   +1 more source

Geometric tool kit for higher spin gravity (part II): An introduction to Lie algebroids and their enveloping algebras [PDF]

open access: yesInternational Journal of Modern Physics A, 2023
These notes provide a self-contained introduction to Lie algebroids, Lie-Rinehart algebras and their universal envelopes. This review is motivated by the speculation that higher-spin gauge symmetries should admit a natural formulation as enveloping ...
X. Bekaert
semanticscholar   +1 more source

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