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• W2087824184 abstract "We utilize the bulk viscosity of interacting strange quark matter to reevaluate the damping time scale. The presence of medium effect of bulk viscosity leads to a stronger damping of r-modes, which can be over an order of magnitude for realistic parameters. We find that the r-mode instability window is narrowed due to the medium effect, and hence when a pulsar reaches the instability window it will only slow down by gravitational wave emission to a period of 1.78msec instead of 2.5msec given by early estimate. As a theoretical upper rotation limit of pulsars, the period of 1.78msec is very close to the two most rapidly spinning pulsars known, with periods of about 1.6msec." @default.
• W2087824184 created "2016-06-24" @default.
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• W2087824184 date "2003-03-10" @default.
• W2087824184 modified "2023-09-26" @default.
• W2087824184 title "The Critical Rotation of Strange Stars and Rapidly Rotating Pulsars" @default.
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• W2087824184 doi "https://doi.org/10.1086/374370" @default.
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