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arxiv: 0901.3168 · v2 · pith:7CPGRW6Bnew · submitted 2009-01-20 · 🌀 gr-qc

Formation of a Kerr black hole from two stringy NUT objects

classification 🌀 gr-qc
keywords blackholekerrobjectsappropriatearisingaxiscounter-rotating
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In this paper we show that an isolated Kerr black hole can be interpreted as arising from a pair of identical counter-rotating NUT objects placed on the symmetry axis at an appropriate distance from each other.

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