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    Power law tail in the radial growth probability distribution for DLA

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    Using both analytic and numerical methods, we study the radial growth probability distribution P(r,M)P(r,M) for large scale off lattice diffusion limited aggregation (DLA) clusters. If the form of P(r,M)P(r,M) is a Gaussian, we show analytically that the width ξ(M)\xi(M) of the distribution {\it can not} scale as the radius of gyration RGR_G of the cluster. We generate about 17501750 clusters of masses MM up to 500,000500,000 particles, and calculate the distribution by sending 10610^6 further random walkers for each cluster. We give strong support that the calculated distribution has a power law tail in the interior (r0r\sim 0) of the cluster, and can be described by a scaling Ansatz P(r,M)rαξg(rr0ξ)P(r,M) \propto {r^\alpha\over\xi}\cdot g\left( {r-r_0}\over \xi \right), where g(x)g(x) denotes some scaling function which is centered around zero and has a width of order unity. The exponent α\alpha is determined to be 2\approx 2, which is now substantially smaller than values measured earlier. We show, by including the power-law tail, that the width {\it can} scale as RGR_G, if α>Df1\alpha > D_f-1.Comment: 11 pages, LaTeX, 5 figures not included, HLRZ preprint-29/9
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