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[en] The problem of plasma wave generation and propagation in the presence of strong gravitational fields is studied in the framework of general relativity theory. The coupled relativistic hydrodynamic and Maxwellian equations are solved in circumstances of the surface of the neutron star. The wave solution of the system of equation is analyzed, some limit cases are discussed in detail. The instability criteria of relativistic plasma are also found. (D.Gy.)
Source
Bakos, J.S.; Soerlei, Zsuzsa (eds.); Eoetvoes Lorand Fizikai Tarsulat, Budapest (Hungary); Hungarian Academy of Sciences, Budapest. Central Research Inst. for Physics; 539 p; ISBN 963 372 373 6; 
; Jun 1985; p. 108-110; Koezponti Fizikai Kutato Intezet; Budapest (Hungary); 17. International conference on phenomena in ionized gases; Budapest (Hungary); 8-12 Jul 1985; 5 refs.
; Jun 1985; p. 108-110; Koezponti Fizikai Kutato Intezet; Budapest (Hungary); 17. International conference on phenomena in ionized gases; Budapest (Hungary); 8-12 Jul 1985; 5 refs.