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  The oscillation and stability of differentially rotating spherical shells: the normal-mode problem

Watts, A. L., Andersson, N., Beyer, H., & Schutz, B. F. (2003). The oscillation and stability of differentially rotating spherical shells: the normal-mode problem. Monthly Notices of the Royal Astronomical Society, 342(4), 1156-1168. doi:10.1046/j.1365-8711.2003.06612.x.

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3139.pdf (Publisher version), 3MB
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 Creators:
Watts, A. L.1, Author
Andersson, N.1, Author
Beyer, H.2, Author
Schutz, B. F.3, Author           
Affiliations:
1External Organizations, Department of Mathematics, University of Southampton, Southampton SO17 1BJ, ou_persistent22              
2MPI for Gravitational Physics, Max Planck Society, Golm, DE, ou_24007              
3Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, Golm, DE, ou_24013              

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 Abstract: An understanding of the dynamics of differentially rotating systems is key to many areas of astrophysics. We investigate the oscillations of a simple system exhibiting differential rotation, and discuss issues concerning the role of corotation points and the emergence of dynamical instabilities. This problem is of particular relevance to the emission of gravitational waves from oscillating neutron stars, which are expected to possess significant differential rotation immediately after birth or binary merger.

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 Dates: 2003-07
 Publication Status: Published online
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 Rev. Type: Peer
 Identifiers: eDoc: 3139
DOI: 10.1046/j.1365-8711.2003.06612.x
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Title: Monthly Notices of the Royal Astronomical Society
Source Genre: Journal
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Publ. Info: Oxford : Blackwell Science
Pages: - Volume / Issue: 342 (4) Sequence Number: - Start / End Page: 1156 - 1168 Identifier: ISSN: 0035-8711