Birkhoff's invariant and Thorne's Hoop Conjecture
arXiv:0903.1580
Abstract
I propose a sharp form of Thorne's hoop conjecture which relates Birkhoff's invariant for an outermost apparent horizon to its mass, . I prove the conjecture in the case of collapsing null shells and provide further evidence from exact rotating black hole solutions. Since is bounded below by the length of the shortest non-trivial geodesic lying in the apparent horizon, the conjecture implies . The Penrose conjecture, , and Pu's theorem imply this latter consequence for horizons admitting an antipodal isometry. Quite generally, Penrose's inequality and Berger's isembolic inequality, , where is the injectivity radius, imply , where is the convexity radius.
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