Indirect Visibility of Gravitational Waves in Magnetohydrodynamic Plasmas

Simple item page
dc.creatorMoortgat, Joachim
dc.creatorKuijpers, Jan
dc.date2005-03-17
dc.date.accessioned2026-07-07T03:29:28Z
dc.date.available2026-07-07T03:29:28Z
dc.descriptionWe propose a mechanism to make gravitational waves (GWs) visible in the electromagnetic domain. Gravitational waves that propagate through a strongly magnetized plasma interact with the plasma through its anisotropic stress-energy tensor and excite magnetohydrodynamic (MHD) wave modes. In catastrophic events such as the merger of a double neutron star binary, a large fraction of the total binding energy of the system is released in the form of GWs observable by LIGO, and the amount of energy transferred to the MHD waves is substantial. These modes, however, are excited at the same frequency as the GW and are not directly observable. In this paper we investigate radiation processes that operate in the presence of the gravitationally excited MHD waves and radiate in the radio regime accessible to LOFAR. We present order of magnitude estimates for the spectral flux of a merger detectable by a LOFAR.
dc.description6 pages; 8 eps figures; Proceedings of the XXII Texas Symposium on Relativistic Astrophysics, Stanford University, Palo Alto, USA, December 13-17 2004. PSN 1230
dc.identifierhttps://arxiv.org/abs/gr-qc/0503074
dc.identifierhttp://arxiv.org/abs/gr-qc/0503074
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35232
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleIndirect Visibility of Gravitational Waves in Magnetohydrodynamic Plasmas
dc.typetext

Files

Collections

arXiv