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Generation of gravitational radiation in dusty plasmas and supernovae
Umeå University, Faculty of Science and Technology, Department of Physics.
Umeå University, Faculty of Science and Technology, Department of Physics.
Umeå University, Faculty of Science and Technology, Department of Physics.
2005 (English)In: JETP Letters: Journal of Experimental And Theoretical Physics Letters, ISSN 0021-3640, E-ISSN 1090-6487, Vol. 81, no 4, 135-139 p.Article in journal (Refereed) Published
Abstract [en]

We 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.

Place, publisher, year, edition, pages
2005. Vol. 81, no 4, 135-139 p.
Identifiers
URN: urn:nbn:se:umu:diva-12355DOI: 10.1134/1.1914867OAI: oai:DiVA.org:umu-12355DiVA: diva2:152026
Available from: 2007-04-02 Created: 2007-04-02 Last updated: 2011-01-26Bibliographically approved

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Brodin, GertMarklund, MattiasShukla, Padma K.

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