Nonlinear evolution of the r-modes in neutron stars.
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Cites background or methods from "Nonlinear evolution of the r-modes ..."
...(4) The discrete Fourier transform of the gravitational wave signal from our rescaling of the simulation of Lindblom et al (2001a) is shown in figure 4....
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...We direct those readers who might be interested in the wider range of subjects covered in the talk to the recent review by Lindblom (2001), and the recent papers by Lindblom et al (2001b) and by Lindblom and Owen (2002)....
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...Fortunately, tests have shown (Lindblom et al 2001b) that the maximum amplitude which the r-mode achieves (and hence the maximum value of J22) is relatively insensitive to the strength of the GRR force....
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...These lead to large surface waves which break and shock (Lindblom et al 2001a, 2001b)....
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...2. r-mode evolution model We base our estimates of the GR produced by the non-linear evolution of an unstable r-mode on the numerical simulations by Lindblom et al (2001a, 2001b)....
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28 citations
28 citations
Cites background from "Nonlinear evolution of the r-modes ..."
...On the other hand, differential rotation, first suggested by Rezzolla et al. (2000, 2001a, 2001b), is an unavoidable feature of nonlinear r-modes (Stergioulas & Font 2001; Lindblom et al. 2001; Sá 2004)....
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28 citations
27 citations