Abstract
The present research work is considered as part II of the previous work entitled [Plane Symmetric Solutions to the Nonlinear Spinor Field Equations in General Relativity Theory, jmp, 2019, 10, 1222-1234]. Here, we opt for the static spherical symmetric metric. In this metric, we have obtained spherical symmetric soliton-like solutions to the spinor field equations with nonlinear terms, which are arbitrary functions of , taking into account the proper gravitational field of elementary particles. Equations with power and polynomial nonlinearities are investigated in detail. It is shown that the initial set of the Einstein and spinor field equations with a power-law nonlinearity possess regular solutions with a localized energy density of the spinor field only if we consider massless particle without losing the generality (m = 0). In this case, a soliton-like configuration has negative energy. In order to define the role of the nonlinearity and the own gravitational field of the elementary particles in this model, we have obtained exact static symmetric solutions to the above spinor field equations in the linear case by considering Dirac’s equations and in flat space-time. It is proved that soliton-like solutions are absent in the linear case. But in flat space-time soliton-like configurations exist and have positive total energy.
Highlights
The soliton as regular, localized energy density, finite total energy and stable solutions of nonlinear differential equations, is widely used in pure science
It is demonstrated that the static plane symmetric metric doesn’t convenient to obtain the soliton-like solutions with finite quantities of the total charge and the total spin
We shall analyze the general results obtained in the previous section for concrete nonlinear terms of the arbitrary function F ( IP ) in the lagrangian density
Summary
The soliton as regular, localized energy density, finite total energy and stable solutions of nonlinear differential equations, is widely used in pure science. It is demonstrated that the static plane symmetric metric doesn’t convenient to obtain the soliton-like solutions with finite quantities of the total charge and the total spin They concluded that the consideration of the own gravitational field of the elementary particles and the nonlinearity of the spinor field in the lagrangian density are not sufficient in order to describe the configuration of elementary particles. In this present study, considering the nonlinearity of the spinor field, the own gravitational field of elementary particles and changing the geometrical properties of the metric, we have extended the results initiated in [4] to exact spherical symmetric solutions
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