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More on quantum chiral higher spin gravity

Evgeny Skvortsov, Tung Tran, Mirian Tsulaia

2020Physical review. D/Physical review. D.88 citationsDOIOpen Access PDF

Abstract

Chiral higher spin gravity is unique in being the smallest higher spin extension of gravity and in having a simple local action both in flat and (anti-)de Sitter spaces. It must be a closed subsector of any other higher spin theory in four dimensions, which makes it an important building block and benchmark. Using the flat space version for simplicity, we perform a thorough study of quantum corrections in chiral theory, which strengthens our earlier results [E. Skvortsov, T. Tran, and M. Tsulaia, Phys. Rev. Lett. 121, 031601 (2018)]. Even though the interactions are naively nonrenormalizable, we show that there are no UV divergences in two-, three-, and four-point amplitudes at one loop thanks to the higher spin symmetry. We also give arguments that the AdS chiral theory should exhibit similar properties. It is shown that chiral theory admits Yang-Mills gaugings with $U(N)$, $SO(N)$, and $USp(N)$ groups, which is reminiscent of the Chan-Paton symmetry in string theory.

Topics & Concepts

PhysicsSpin foamQuantum gravitySpin (aerodynamics)QuantumImmirzi parameterTheoretical physicsLoop quantum gravityQuantum mechanicsCondensed matter physicsThermodynamicsBlack Holes and Theoretical PhysicsNoncommutative and Quantum Gravity TheoriesCosmology and Gravitation Theories
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