2019
DOI: 10.1103/physrevd.100.105013
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Equivalent dual theories for 3D N=2 supergravity

Abstract: N =2 three dimensional Supergravity with internal R−symmetry generators can be understood as a two dimensional chiral Wess-Zumino-Witten model. In this paper, we present the reduced phase space description of the theory, which turns out to be flat limit of a generalised Liouville theory, up to zero modes. The reduced phase space description can also be explained as a gauged chiral Wess-Zumino-Witten model. We show that both these descriptions possess identical gauge and global (quantum N =2 superBMS 3 ) symmet… Show more

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Cited by 11 publications
(11 citation statements)
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“…Generalizations of the present work to the supersymmetric case are also of interest. The reduction of the boundary of N = 1 flat space supergravity was already performed in [86] and N = 2 BMS 3 invariant WZW-models were considered recently in [120,121], however the relation to the geometric action on the coadjoint orbits of supersymmetric extensions of the BMS 3 group was not yet exposed. It seems that the techniques and methods discussed here can straightforwardly be applied to the supersymmetric extensions of the BMS 3 algebra and flat space supergravities of [122][123][124].…”
Section: Discussionmentioning
confidence: 99%
“…Generalizations of the present work to the supersymmetric case are also of interest. The reduction of the boundary of N = 1 flat space supergravity was already performed in [86] and N = 2 BMS 3 invariant WZW-models were considered recently in [120,121], however the relation to the geometric action on the coadjoint orbits of supersymmetric extensions of the BMS 3 group was not yet exposed. It seems that the techniques and methods discussed here can straightforwardly be applied to the supersymmetric extensions of the BMS 3 algebra and flat space supergravities of [122][123][124].…”
Section: Discussionmentioning
confidence: 99%
“…In principle there is no compelling reason for this choice. However, we will see that this choice with small |n| can lead to consistent results which may justify this specific choice among other possible choices [32]. Thus, one can writė…”
Section: Interacting Holographic Dark Energy Model For Future Evementioning
confidence: 63%
“…Therefore, our system of equations is not closed and we still have freedom to choose one field in terms of another one. At this point, we may assume that Brans-Dicke scalar field can be described as a power law of the scale factor as φ = a n [32]. In principle there is no compelling reason for this choice.…”
Section: Interacting Holographic Dark Energy Model For Future Evementioning
confidence: 99%
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“…There are another modified gravity formalism which are completely different with f (R) model of gravity. The various aspect of f (R) models of gravity is investigated in [4][5][6][7][8][9][10][11][12][13][14][15][16][17][18]. The unification of dark energy and early time inflation with late time acceleration from f (R) theory to all Lorentz non-invariant theories is discussed by Nojiri and Odintsov [19].…”
Section: Introductionmentioning
confidence: 99%