2019
DOI: 10.1007/jhep11(2019)008
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Kinematical superspaces

Abstract: A. We classify N=1 d = 4 kinematical and aristotelian Lie superalgebras with spatial isotropy, but not necessarily parity nor time-reversal invariance. Employing a quaternionic formalism which makes rotational covariance manifest and simplifies many of the calculations, we find a list of 43 isomorphism classes of Lie superalgebras, some with parameters, whose (nontrivial) central extensions are also determined. We then classify their corresponding simply-connected homogeneous (4|4)-dimensional superspaces, res… Show more

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Cited by 8 publications
(7 citation statements)
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“…[49] for a review, or ref. [50] for a more concise description) that the type of spinors one obtains for SOfalse(p,qfalse)$SO_{(p, q)}$ in the real case is governed by the signature false(pqfalse)0.33emmod0.33em8$(p-q)\ {\rm mod}\ 8$. Among even signatures, signature 0 gives a real representation, signature 4 a quaternionic representation, while signatures 2 and 6 give complex representations.…”
Section: Weyl and Majorana Spinorsmentioning
confidence: 99%
“…[49] for a review, or ref. [50] for a more concise description) that the type of spinors one obtains for SOfalse(p,qfalse)$SO_{(p, q)}$ in the real case is governed by the signature false(pqfalse)0.33emmod0.33em8$(p-q)\ {\rm mod}\ 8$. Among even signatures, signature 0 gives a real representation, signature 4 a quaternionic representation, while signatures 2 and 6 give complex representations.…”
Section: Weyl and Majorana Spinorsmentioning
confidence: 99%
“…They typically result of a limiting process or appear as the geometry induced on a null hypersurface. Applications include Hamiltonian analysis [4], Carrollian particles [5,6], ultra-relativistic fluid mechanics [7][8][9][10][11][12][13], cosmology [14], Carrollian [15][16][17][18][19] and conformally Carrollian [20][21][22][23] field theories, higher-spin [24][25][26], super-symmetric [27][28][29][30][31][32] and non-commutative [33] extensions, null hypersurfaces and isolated horizons [34][35][36][37][38][39][40][41][42][43][44][45], geometry of space/time-like infinities [46][47][48] and, finally, geometry of null infinity which is the main concern of this article.…”
Section: Introduction/summarymentioning
confidence: 99%
“…They typically result of a limiting process or appear as the geometry induced on a null hypersurface. Applications include Hamiltonian analysis [4], Carrollian particles [5,6], ultra-relativistic fluid mechanics [7][8][9][10][11][12][13], cosmology [14], Carrollian [15][16][17][18][19] and conformally Carrollian [20][21][22][23] field theories, higher-spin [24,25], super-symmetric [26][27][28][29][30][31] and non-commutative [32] extensions, null hypersurfaces and isolated horizons [33][34][35][36][37][38][39][40][41][42][43][44], geometry of space/time-like infinities [45][46][47] and, finally, geometry of null infinity which is the main concern of this article. This is a well-known fact that the conformal boundary of an asymptotically flat spacetime, which we will generically refer to as "null infinity", is a (conformal) Carrollian manifold.…”
Section: Introduction/summarymentioning
confidence: 99%