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Black holes: from event horizons to trapping horizons - LUTH ...

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Angular momentum and area evolution laws<br />

Angular momentum flux law<br />

Under the supplementary hypothesis that ϕ is transported along the evolution<br />

vec<strong>to</strong>r h : Lh ϕ = 0, the generalized Damour-Navier-S<strong>to</strong>kes equation leads <strong>to</strong><br />

<br />

d<br />

J(ϕ) = − T (m, ϕ)<br />

dt S ɛ − 1<br />

<br />

σ<br />

16π<br />

(m) : Lϕ q − 2θ (k) <br />

ϕ · DC<br />

Sɛ<br />

St<br />

St<br />

[EG, PRD 72, 104007 (2005)]<br />

Eric Gourgoulhon (<strong>LUTH</strong>) <strong>Black</strong> <strong>holes</strong>: <strong>trapping</strong> <strong>horizons</strong> CERN, 17 March 2010 33 / 38

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