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33750333380
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note
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i are the initial central density and average density of the dust cloud at t=0, respectively. It is obvious that the former can be earlier than the latter for the initial data with certain central concentration.
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71
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33750336907
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note
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The similar results were obtained for linearized gravitational waves during the spherically symmetric homogeneous dust collapse [22] and for scalar waves during the neutron star collapse in the fully nonlinear spherically symmetric Einstein-fluid-Klein-Gordon system [43].
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