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100 Years of Relativity Space-Time Structure: Einstein and Beyond ...

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Gravitational Billiards, Dualities <strong>and</strong> Hidden Symmetries 51For this frame field we adopt the so-called Iwasawa decompositionθ a = e −βa N a idx i (33)by splitting <strong>of</strong>f the (logarithmic) scale factors β a from the <strong>of</strong>f-diagonal frame(<strong>and</strong> metric) degrees <strong>of</strong> freedom N a i, which are represented by an uppertriangular matrix with 1’s on the diagonal. The spatial metric then becomesg ij =d∑e −2βa N a i N a j (34)a=1The main advantage <strong>of</strong> the Iwasawa decomposition is that it matches preciselywith the triangular decomposition (48) below, which is valid for anyKac Moody algebra. Furthermore, it turns out that, in the limit t → 0 allthe interesting action takes place in the scale factors β a , whereas the N aswell as the matter degrees <strong>of</strong> freedom asymptotically ‘come to rest’ in thislimit. Similarly, the metric <strong>and</strong> other degrees <strong>of</strong> freedom at different spatialpoints should decouple in this limit, as the spatial distance between themexceeds their horizon e . The basic hypothesis underlying the BKL analysisis therefore that spatial gradients should become less <strong>and</strong> less important incomparison with time derivatives as t → 0, such that the resulting theoryshould be effectively describable in terms <strong>of</strong> a one dimensional reduction,in which the complicated partial differential equations <strong>of</strong> <strong>Einstein</strong>’s theoryare effectively replaced by a continuous infinity <strong>of</strong> ordinary differentialequations.To spell out this idea in more detail, let us insert the above metric ansatzinto the <strong>Einstein</strong>-Hilbert action, <strong>and</strong> drop all spatial derivatives (gradients),so that this action is approximated by a continuous superposition <strong>of</strong> onedimensionalsystems. One then obtains (still in d spatial dimensions)S[g ij ] = 1 4∫∫d d xdx 0 Ñ −1 [( tr (g −1 ġ) 2 − (tr g −1 ġ) 2)] (35)in a matrix notation where g(t) ∈ GL(d, R) st<strong>and</strong>s for the matrix (g ij )representing the spatial components <strong>of</strong> the metric at each spatial point,<strong>and</strong> Ñ ≡ N√ g is a rescaled lapse function. Neglecting the <strong>of</strong>f-diagonale One might even view this decoupling as a direct consequence <strong>of</strong> the spacelike nature <strong>of</strong>the singularity.

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