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Three-dimensional non-relativistic Hietarinta supergravity

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arxiv 2409.01298 v2 pith:DMRNRHAW submitted 2024-09-02 hep-th gr-qc

Three-dimensional non-relativistic Hietarinta supergravity

classification hep-th gr-qc
keywords non-relativistichietarintagravitysupersupergravitytheoryactionaddressing
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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In this work we present the non-relativistic regime of the Hietarinta gravity theory and its extension to supergravity. At the bosonic level, we derive the non-relativistic version of the Hietarinta model by employing a contraction process and addressing the non-degeneracy of the invariant metric. To incorporate supersymmetry, we apply the Lie algebra expansion method to obtain the non-relativistic formulation of $\mathcal{N}=2$ Hietarinta supergravity. Our results reveal that the non-relativistic Hietarinta theory encompasses the extended Bargmann (super)gravity as a special case, yet it differs significantly from other existing non-relativistic (super)gravity models. Furthermore, we generalize our analysis to include a cosmological constant term in the non-relativistic Hietarinta (super)gravity action and examine its effects on the torsion structure.

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Cited by 1 Pith paper

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  1. Non-Relativistic Chern-Simons Supergravity with Torsion

    hep-th 2026-04 unverdicted novelty 7.0

    A parameterized family of non-relativistic supergravity theories with torsion is obtained in three dimensions from the semigroup expansion of an N=2 supersymmetric Mielke-Baekler algebra.