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Astrophysics

Title: Magnetized gravitational waves

Abstract: We investigate the influence of cosmic magnetic fields on gravitational wave perturbations, and find exact solutions on large scales. We show that a large-scale magnetic field can generate large-scale non-decaying gravitational waves. In the general case where gravitational waves are generated by other mechanisms, a large-scale magnetic field introduces a new decaying tensor mode and modifies the non-decaying mode. The direct effect of the magnetic field is to damp the gravitational waves, while an indirect magneto-curvature effect can either damp or boost the waves. A magnetic field also leads to a breaking of statistical isotropy, and the magnetic imprint on the tensor spectrum in principle provides a means of detecting a primordial field.
Comments: Minor changes. To appear in Phys. Rev. D
Subjects: Astrophysics (astro-ph); General Relativity and Quantum Cosmology (gr-qc)
Journal reference: Phys.Rev. D63 (2001) 123507
DOI: 10.1103/PhysRevD.63.123507
Cite as: arXiv:astro-ph/0101151
  (or arXiv:astro-ph/0101151v3 for this version)

Submission history

From: Christos Tsagas [view email]
[v1] Wed, 10 Jan 2001 17:04:49 GMT (8kb)
[v2] Wed, 28 Feb 2001 16:41:09 GMT (9kb)
[v3] Sat, 19 May 2001 12:55:16 GMT (9kb)