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Hypersymmetric extensions of Maxwell-Chern-Simons gravity in 2+1 dimensions

TLDR
In this article, a consistent way of coupling three-dimensional hyper-Maxwell-Chern-Simons gravity theory with massless spin-$\frac{5}{2}$ gauge fields was presented.
Abstract
We present a consistent way of coupling three-dimensional Maxwell-Chern-Simons gravity theory with massless spin-$\frac{5}{2}$ gauge fields. We first introduce the simplest hyper-Maxwell-Chern-Simons gravity generically containing two massless spin-2 fields coupled with a massless Majorana fermion of spin $\frac{5}{2}$ whose novel underlying superalgebra is explicitly constructed. We then present three alternative hypersymmetric extensions of the Maxwell algebra which are shown to emerge from the In\"on\"u-Wigner contraction procedure of precise combinations of the $\mathfrak{o}\mathfrak{s}\mathfrak{p}(1|4)$ and the $\mathfrak{s}\mathfrak{p}(4)$ algebras. This allows us to construct distinct types of hyper-Maxwell-Chern-Simons theories that extend to include generically interacting nonpropagating spin-4 fields accompanied by one or two spin-$\frac{5}{2}$ gauge fields.

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Mapping relativistic to ultra/non-relativistic conformal symmetries in 2D and finite T T ¯ $$ \sqrt{T\overline{T}} $$ deformations

TL;DR: The conformal symmetry algebra in 2D (Diff(S1)⊕Diff (S1)) is shown to be related to its ultra/non-relativistic version (BMS3≈GCA2) through a nonlinear map of the generators, without any sort of limiting process.
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Non-relativistic and ultra-relativistic expansions of three-dimensional spin-3 gravity theories

TL;DR: In this article , a spin-3 extension of the AdS algebra was obtained by applying the expansion procedure using different semigroups, leading to spin 3 extensions of known non-relativistic and ultra-relateivistic algebras.
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Three-dimensional Maxwellian Carroll gravity theory and the cosmological constant

TL;DR: In this article, an extension of the Maxwellian Carroll symmetry is shown to be necessary in order for the invariant tensor of the ultra-relativistic Maxwellian algebra to be non-degenerate.
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Mapping relativistic to ultra/non-relativistic conformal symmetries in 2D and finite $\sqrt{T\bar{T}}$ deformations

TL;DR: The conformal symmetry algebra in 2D (Diff($S^{1}$)$\oplus$Diff$S€ 1}$)) is shown to be related to its ultra/non-relativistic version (BMS${3}$ ) through a nonlinear map of the generators, without any sort of limiting process as discussed by the authors.
Posted Content

Three-dimensional Maxwellian Carroll gravity theory and the cosmological constant

TL;DR: In this article, an extension of the Maxwellian Carroll symmetry is presented for the invariant tensor of the ultra-relativistic Maxwellian algebra to be non-degenerate.
References
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Journal ArticleDOI

N=1 supergravity and Maxwell superalgebras

TL;DR: In this paper, the authors presented the construction of the D = 4 supergravity action from the minimal Maxwell superalgebra sℳ4 by applying the abelian semigroup expansion procedure.
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A note on the Chevalley–Eilenberg cohomology for the Galilei and Poincaré algebras

TL;DR: In this paper, the complete Chevalley-Eilenberg cohomology at form degrees 2, 3 and 4 for the Galilei and Poincare groups was constructed in a systematic way.
Journal ArticleDOI

Gauged ads–maxwell algebra and gravity

TL;DR: In this article, the anti-de Sitter algebra is extended with additional generators, forming the negative cosmological constant counterpart of the Maxwell algebra. But the resulting theory is described by the Einstein-Cartan action with Holst term, and the gauge fields associated with the Maxwell generators appear only in topological terms that do not influence dynamical field equations.
Journal ArticleDOI

Maxwell superalgebras and Abelian semigroup expansion

TL;DR: In this paper, it was shown that different choices of abelian semigroups S lead to interesting D = 4 Maxwell superalgebras, which are derived alternatively as an S-expansion of osp ( 4 | N ).
Journal ArticleDOI

Hypersymmetry in D=3 of coupled gravity-massless spin-5/2 system

TL;DR: In this article, the coupled massless spin-5/2-Einstein system exhibits a new local supersymmetry parametrised by a vector-spinor rather than a spinor as in supergravity.
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