Critical \(\mathcal{N} = (1, 1)\) general massive supergravity
From MaRDI portal
Publication:1641774
DOI10.1007/JHEP04(2018)105zbMath1390.83391arXiv1802.03957OpenAlexW3123263766MaRDI QIDQ1641774
George Moutsopoulos, Jan Rosseel, Nihat Sadik Deger
Publication date: 19 June 2018
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1802.03957
Two-dimensional field theories, conformal field theories, etc. in quantum mechanics (81T40) Supergravity (83E50) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Cites Work
- A dynamical theory for linearized massive superspin 3/2
- AdS\({}_3\)/LCFT\({}_2\) -- correlators in cosmological topologically massive gravity
- Critical and non-critical Einstein-Weyl supergravity
- Short-cut to new anomalies in gravity duals to logarithmic conformal field theories
- Superconformal sigma models in three dimensions
- Supersymmetric warped AdS in extended topologically massive supergravity
- Massive \( \mathcal{N} = 2\) supergravity in three dimensions
- Two-dimensional turbulence: A novel approach via logarithmic conformal field theory
- Logarithmic operators in conformal field theory
- Three-dimensional \(\mathcal{N} = 2\) (AdS) supergravity and associated supercurrents
- Higher derivative couplings and massive supergravity in three dimensions
- Supersymmetric backgrounds and black holes in \( \mathcal{N}=(1,1)\) cosmological new massive supergravity
- CHERN–SIMONS THEORIES WITH SUPERSYMMETRIES IN THREE DIMENSIONS
- Supersymmetric solutions of N = (2, 0) topologically massive supergravity
- Holographic applications of logarithmic conformal field theories
- More on massive 3D supergravity
- Logarithmic superconformal minimal models
- Massive 3D supergravity
- CONSISTENT BOUNDARY CONDITIONS FOR COSMOLOGICAL TOPOLOGICALLY MASSIVE GRAVITY AT THE CHIRAL POINT
- N⩾=2 supersymmetric Chern-Simons terms as d=3 extended conformal supergravity
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