Maxwell's equations and Lorentz force in doubly special relativity

被引:1
|
作者
Takka, N. [1 ]
Bouda, A. [1 ]
机构
[1] Univ Bejaia, Lab Phys Theor, Fac Sci Exactes, Bejaia 06000, Algeria
关键词
Noncommutative geometry; kappa-Minkowski space-time; Maxwell's equations; FEYNMANS PROOF; POINCARE; MONOPOLE;
D O I
10.1007/s12648-019-01556-x
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
On the basis of all commutation relations of the kappa-deformed phase space incorporating the kappa-Minkowski space-time, we have derived in this paper an extended first approximation of both Maxwell's equations and Lorentz force in doubly (or deformed) special relativity (DSR). For this purpose, we have used our approach of the special relativistic version of Feynman's proof by which we have established the explicit formulations of electric and magnetic fields. As in Fock's nonlinear relativity (FNLR), the laws of electrodynamics depend on the particle mass which therefore constitutes a common point between the two extended forms of special relativity. As one consequence, the corresponding equation of motion contains two different types of contributions. In addition to the usual type, another one emerges as a consequence of the coexistence of mass and charge which are coupled with the kappa-deformation and electromagnetic field. This new effect completely induced by the kappa-deformed phase space is interpreted as the gravitational-type Lorentz force. Unlike FNLR, the corrective terms all depend on the electromagnetic field in DSR.
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页码:1227 / 1235
页数:9
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