Critical Behavior of Black Hole Formation in a Scalar Wave Collapse

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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DPNU-94-04 (multicol.sty was added.)

Scientific paper

10.1143/PTP.91.1265

We present a self-similar model of spherically symmetric collapse of a
massless scalar field with a parameter $p$. The black hole formation is
explicitly shown to occur only in the strong-field implosion of $p >1$. The
field evolution in the critical limit $ p \rightarrow 1 $ is compared with
numerical results found by Choptuik.

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