Non-Linear Development of the Secular Bar-Mode Instability in Rapidly Rotating Neutron Stars
We present results from investigations of the nonlinear development of the secular bar-mode instability that is driven by gravitational radiation-reaction (GRR) forces in rotating neutron stars. Our fully three-dimensional hydrodynamical simulations have shown that, in the absence of any competing v...
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| Format: | Others |
| Language: | en |
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LSU
2004
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| Online Access: | http://etd.lsu.edu/docs/available/etd-10282004-114654/ |