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An exact one parameter () family of solutions representing scalar field collapse is shown to exhibit a type of critical behaviour which has been discussed by Choptuik. The three possible evolutions are outlined. For supercritical evolution (when black holes form) it is shown that a quantity related to the mass of the black hole exhibits a power law dependence on , for near critical evolution . The solution supports the conjecture that black hole formation initially occurs at infinitesimal mass.
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P. R. Brady (1994) studied this question.
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