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Noncommutative Electrodynamics from SO(2,3)_star Model of Noncommutative Gravity

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arxiv 1804.00608 v1 pith:5HVT4LOW submitted 2018-04-02 hep-th gr-qc

Noncommutative Electrodynamics from SO(2,3)_star Model of Noncommutative Gravity

classification hep-th gr-qc
keywords gravitymodelnoncommutativenoncommutativityactionselectrodynamicselectronfield
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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In our previous work we have constructed a model of noncommutative (NC) gravity based on $SO(2,3)_\star$ gauge symmetry. In this paper we extend the model by adding matter fields: fermions and a $U(1)$ gauge field. Using the enveloping algebra approach and the Seiberg-Witten map we construct actions for these matter fields and expand the actions up to first order in the noncommutativity (deformation) parameter. Unlike in the case of pure NC gravity, first non-vanishing NC corrections are linear in the noncommutativity parameter. In the flat space-time limit we obtain a non-standard NC Electrodynamics. Finally, we discuss effects of noncommutativity on relativistic Landau levels of an electron in a constant background magnetic field and in addition we calculate the induced NC magnetic dipole moment of the electron.

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    A first-order Seiberg–Witten twist of the bulk gauge fields lowers the critical magnetic field of 3D and 4D holographic superconductors, Bc = Bc⁰(1 − Bc⁰ k̄), mimicking a stronger applied field B_eff = B(1+Bθ).