Modeling a nonperturbative spinor vacuum interacting with a strong gravitational wave

The European Physical Journal C

Vladimir Dzhunushaliev¹  Vladimir Folomeev² 

[1] Department of Theoretical and Nuclear Physics, Al-Farabi Kazakh National University, 050040, Almaty, Kazakhstan;Institute of Experimental and Theoretical Physics, Al-Farabi Kazakh National University, 050040, Almaty, Kazakhstan;Institute of Physicotechnical Problems and Material Science of the NAS of the Kyrgyz Republic, 265 a, Chui Street, 720071, Bishkek, Kyrgyz Republic;

关键词: Einstein Equation;    Gravitational Wave;    Periodic Potential;    Spinor Field;    Nonvanishing Component;   

DOI  :  10.1140/epjc/s10052-015-3526-2

来源: Springer

【 摘 要 】

We consider the propagation of strong gravitational waves interacting with a nonperturbative vacuum of spinor fields. To described the latter, we suggest an approximate model. The corresponding Einstein equation has the form of the Schrödinger equation. Its gravitational-wave solution is analogous to the solution of the Schrödinger equation for an electron moving in a periodic potential. The general solution for the periodic gravitational waves is found. The analog of the Kronig–Penney model for gravitational waves is considered. It is shown that the suggested gravitational-wave model permits the existence of weak electric charge and current densities concomitant with the gravitational wave. Based on this observation, a possible experimental verification of the model is suggested.

【 授权许可】

CC BY