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85037180165
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Throughout this paper, we use (Formula presented) as the central rest mass density of equilibrium stars (initial data for our computation) and (Formula presented) as the central rest mass density of dynamically evolved stars (i.e., the latter changes during the evolution)
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Throughout this paper, we use (Formula presented) as the central rest mass density of equilibrium stars (initial data for our computation) and (Formula presented) as the central rest mass density of dynamically evolved stars (i.e., the latter changes during the evolution).
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39
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85037193405
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Note that we recompute the constraint equations whenever we modify the initial equilibrium configurations (e.g., by depleting the pressure or by modifying the initial density profile)
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Note that we recompute the constraint equations whenever we modify the initial equilibrium configurations (e.g., by depleting the pressure or by modifying the initial density profile).
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