Exact solution of the relativistic magnetohydrodynamic equations in the background of a plane gravitational wave with combined polarization

A.A. Agathonov and Yu.G. Ignatyev1


We obtain an exact solution of the self-consistent relativistic magnetohydrodynamic equations for an anisotropic magnetoactive plasma in the background of a plane gravitational wave metric (PGW) with an arbitrary polarization. It is shown that, in the linear approximation in the gravitational wave amplitude, only the e+ polarization of the PGW interacts with a magnetoactive plasma.


  1. Yu. G. Ignat'ev, Grav. & Cosmol.1 287 (1995).
  2. Yu. G. Ignat'ev, Grav. & Cosmol. 2, 345 (1996).
  3. Yu. G. Ignat'ev and D. N. Gorokhov, Grav. & Cosmol. 3 261 (1997).
  4. J. L. Synge, Relativity: The General Theory (NHPC, Amsterdam, 1960).
  5. C. W. Misner, K. S. Thorne, and J. A. Wheeler, Gravitation (Freeman, San Francisco, 1973).
  6. Yu. G. Ignat'ev and A. B. Balakin., Sov. Phys. J. (Izv. Vuzov, Fizika) 24, No. 7, 20 (1981).
  7. L. D. Landau and E. M. Lifshitz, Field Theory (Nauka, Moscow, 1973).
  8. Yu. G. Ignat'ev and N. R. Khusnutdinov, Ukr. Fiz. Zh. No. 31, 707 (1986).
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