12 research outputs found

    Growing electrostatic modes in the isothermal pair plasma of the pulsar magnetosphere

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    It is shown that a strongly magnetized isothermal pair plasma near the surface of a pulsar supports low-frequency (in comparison to electron cyclotron frequency) toroidal electrostatic plasma modes in the equatorial region. Physically, the thermal pressure coupled with the magnetic pressure creates the low frequency oscillations which may grow for particular case of inhomogeneities of the equilibrium magnetic field and the pair plasma density.Comment: 8 pages, 8 figures, Accepted for publication in Astrophysics & Space Science 201

    Cold Plasma Dispersion Relations in the Vicinity of a Schwarzschild Black Hole Horizon

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    We apply the ADM 3+1 formalism to derive the general relativistic magnetohydrodynamic equations for cold plasma in spatially flat Schwarzschild metric. Respective perturbed equations are linearized for non-magnetized and magnetized plasmas both in non-rotating and rotating backgrounds. These are then Fourier analyzed and the corresponding dispersion relations are obtained. These relations are discussed for the existence of waves with positive angular frequency in the region near the horizon. Our results support the fact that no information can be extracted from the Schwarzschild black hole. It is concluded that negative phase velocity propagates in the rotating background whether the black hole is rotating or non-rotating.Comment: 27 pages, 11 figures accepted for publication in Gen. Relat. & Gravi

    DRIFT THEORY OF A CHARGED-PARTICLE MOTION IN A HIGH-FREQUENCY WAVE IN THE CASE OF THE FINITE LARMOR RADIUS

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    Electromagnetic waves in an ultrarelativistically hot and strongly magnetized electron-positron plasma

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    Consiglio Nazionale delle Ricerche (CNR). Biblioteca Centrale / CNR - Consiglio Nazionale delle RichercheSIGLEITItal
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