A mathematical theory of gravitational collapse

Mathematics – Mathematical Physics

Scientific paper

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Scientific paper

We study the asymptotic behaviour, as the retarded time u tends to infinity, of the solutions of Einstein's equations in the spherically symmetric case with a massless scalar field as the material model. We prove that when the final Bondi mass M 1 is different from zero, as u → ∞, a black hole forms of mass M 1 surrounded by vacuum. We find the rate of decay of the metric functions and the behaviour of the scalar field on the horizon.

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