Abstract

We obtain optical vortices with classical orbital momentum ℓ = 1 and spin j = ±1/2 as exact solutions of a system of nonlinear Maxwell equations (NMEs). Two kinds of Kerr‐type media, namely, those with and without linear dispersion of the electric and the magnet susceptibility, are investigated. The electric and magnetic fields are represented as sums of circular and linear components. This allows us to reduce the NME to a set of nonlinear Dirac equations (NDEs). The vortex solutions in the case of media with dispersion admit finite energy, while the solutions in case of media without dispersion admit infinite energy. The amplitude equations are obtained from equations of nonstationary optical and magnetic response (dispersion). This includes also the optical pulses with time duration of order of and less than the time of relaxation of the media (femtosecond pulses). The possible generalization of NME to a higher number of optical components and a higher number of ℓ and j is discussed.

Highlights

  • Nonlinear wave processes appeared in different sections of the contemporary physics: nonlinear optics, plasma physics, hydrodynamics, and nonlinear field theory

  • We derive a set of amplitude nonlinear Maxwell equations (NMEs) for nonlinear optical media with and without dispersion of the electric and magnetic susceptibility

  • We have shown that in cases of linear and circularly polarized components of the electric and magnetic fields, the NMEs reduce to the system of Nonlinear Dirac equations (NDEs)

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Summary

OPTICAL LEPTONS

We obtain optical vortices with classical orbital momentum = 1 and spin j = ±1/2 as exact solutions of a system of nonlinear Maxwell equations (NMEs). Two kinds of Kerr-type media, namely, those with and without linear dispersion of the electric and the magnet susceptibility, are investigated. The electric and magnetic fields are represented as sums of circular and linear components. This allows us to reduce the NME to a set of nonlinear Dirac equations (NDEs). The amplitude equations are obtained from equations of nonstationary optical and magnetic response (dispersion). This includes the optical pulses with time duration of order of and less than the time of relaxation of the media (femtosecond pulses).

Introduction
We rewrite again the conditions for the spatial phase functions
11. Conclusion

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