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- W1989307588 abstract "A non radially oscillating star emits gravitational waves at frequencies and with damping times that depend on the equation of state of matter and on the dynamical processes that occur in the interior. In this talk we will discuss how the high density behaviour of matter affects the oscillation frequencies of neutron stars in different phases of their life." @default.
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- W1989307588 date "2005-01-01" @default.
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- W1989307588 title "Imprint of the equation of state of dense matter on gravitational waves emitted by oscillating neutron stars" @default.
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- W1989307588 doi "https://doi.org/10.1088/1742-6596/8/1/008" @default.
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