Generation of Gravitational Radiation in Dusty Plasmas and Supernovae

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dc.creatorBrodin, G.
dc.creatorMarklund, M.
dc.creatorShukla, P. K.
dc.date2004-12-09
dc.date.accessioned2026-07-07T10:27:22Z
dc.date.available2026-07-07T10:27:22Z
dc.descriptionWe present a novel nonlinear mechanism for exciting a gravitational radiation pulse (or a gravitational wave) by dust magnetohydrodynamic (DMHD) waves in dusty astrophysical plasmas. We derive the relevant equations governing the dynamics of nonlinearly coupled DMHD waves and a gravitational wave (GW). The system of equations is used to investigate the generation of a GW by compressional Alfvén waves in a type II supernova. The growth rate of our nonlinear process is estimated, and the results are discussed in the context of the gravitational radiation accompanying supernova explosions.
dc.description4 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0412210
dc.identifierhttp://arxiv.org/abs/astro-ph/0412210
dc.identifierJETPLett.81:135,2005; PismaZh.Eksp.Teor.Fiz.81:169-173,2005
dc.identifierdoi:10.1134/1.1914867
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177131
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGeneration of Gravitational Radiation in Dusty Plasmas and Supernovae
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