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Using the isomorphism $mathfrak{o}(3;mathbb{C})simeqmathfrak{sl}(2;mathbb{C})$ we develop a new simple algebraic technique for complete classification of quantum deformations (the classical $r$-matrices) for real forms $mathfrak{o}(3)$ and $mathfrak{o}(2,1)$ of the complex Lie algebra $mathfrak{o}(3;mathbb{C})$ in terms of real forms of $mathfrak{sl}(2;mathbb{C})$: $mathfrak{su}(2)$, $mathfrak{su}(1,1)$ and $mathfrak{sl}(2;mathbb{R})$. We prove that the $D=3$ Lorentz symmetry $mathfrak{o}(2,1)simeqmathfrak{su}(1,1)simeqmathfrak{sl}(2;mathbb{R})$ has three different Hopf-algebraic quantum deformations which are expressed in the simplest way by two standard $mathfrak{su}(1,1)$ and $mathfrak{sl}(2;mathbb{R})$ $q$-analogs and by simple Jordanian $mathfrak{sl}(2;mathbb{R})$ twist deformations. These quantizations are presented in terms of the quantum Cartan-Weyl generators for the quantized algebras $mathfrak{su}(1,1)$ and $mathfrak{sl}(2;mathbb{R})$ as well as in terms of quantum Cartesian generators for the quantized algebra $mathfrak{o}(2,1)$. Finaly, some applications of the deformed $D=3$ Lorentz symmetry are mentioned.
We use the decomposition of o(3,1)=sl(2;C)_1oplus sl(2;C)_2 in order to describe nonstandard quantum deformation of o(3,1) linked with Jordanian deformation of sl(2;C}. Using twist quantization technique we obtain the deformed coproducts and antipode
We construct firstly the complete list of five quantum deformations of $D=4$ complex homogeneous orthogonal Lie algebra $mathfrak{o}(4;mathbb{C})cong mathfrak{o}(3;mathbb{C})oplus mathfrak{o}(3;mathbb{C})$, describing quantum rotational symmetry of f
We explore a nonlinear realization of the (2+1)-dimensional Lorentz symmetry with a constant vacuum expectation value of the second rank anti-symmetric tensor field. By means of the nonlinear realization, we obtain the low-energy effective action of
Motivated by the isomorphism between osp(4|6) superalgebra and D=3 N=6 superconformal algebra we consider the superstring action on the AdS_4 x CP^3 background parametrized by D=3 N=6 super-Poincare and CP^3 coordinates supplemented by the coordinate
We present a model of gravity based on spontaneous Lorentz symmetry breaking. We start from a model with spontaneously broken symmetries for a massless 2-tensor with a linear kinetic term and a nonderivative potential, which is shown to be equivalent