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We study fluctuations of survival probability in an open quantum system classically described by a map with a mixed phase space. Our results provide the first numerical support to theoretical predictions that such fluctuations have a fractal structure, quantitatively related to the algebraic decay of the classical survival probability.

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... that Q , Q max, t . It is easy to see from (15) that at 1 ø Q ø Q max, t the distribution F t ͑ Q ͒ displays the same decay exponent as P ͑ t ͒ and G ͑ Q f ͒ . It follows that the value of g to be used in (14) is g ෇ 1.323 ͑ 9 ͒ , as obtained from survival probability decays in Fig. 2 in agreement with known results [8,9]. So (14) predicts fractal dimension ഠ 1.33 . According to the above discussion, at a given time t this fractal structure should be observable on scales .df min ϳ 1 ͞ Q max, t ϳ 1 ͑͞ t ln r ͒ . Furthermore, as the validity of the theory is restricted to times less than the Heisenberg time t H ϳ r , at no time can formula (14) be expected to hold on scales smaller than ϳ 1 ͑͞ r ln r ͒ (which in our case is of order e 2 8 ). To check this prediction, we have computed fl uctuation patterns at four different times (two examples are given in Fig. 3), from which we have extracted fractal graph dimensions D and the exponents g C of correlation functions [formula (13)]. The inset of Fig. 4 shows such correlations. Fractal dimensions have been computed by means of the modi fi ed box counting algorithm used in [6]: results are shown in Fig. 4. We tested the algorithm, by computing fractal dimensions of curves generated ...
Context 2
... that Q , Q max, t . It is easy to see from (15) that at 1 ø Q ø Q max, t the distribution F t ͑ Q ͒ displays the same decay exponent as P ͑ t ͒ and G ͑ Q f ͒ . It follows that the value of g to be used in (14) is g ෇ 1.323 ͑ 9 ͒ , as obtained from survival probability decays in Fig. 2 in agreement with known results [8,9]. So (14) predicts fractal dimension ഠ 1.33 . According to the above discussion, at a given time t this fractal structure should be observable on scales .df min ϳ 1 ͞ Q max, t ϳ 1 ͑͞ t ln r ͒ . Furthermore, as the validity of the theory is restricted to times less than the Heisenberg time t H ϳ r , at no time can formula (14) be expected to hold on scales smaller than ϳ 1 ͑͞ r ln r ͒ (which in our case is of order e 2 8 ). To check this prediction, we have computed fl uctuation patterns at four different times (two examples are given in Fig. 3), from which we have extracted fractal graph dimensions D and the exponents g C of correlation functions [formula (13)]. The inset of Fig. 4 shows such correlations. Fractal dimensions have been computed by means of the modi fi ed box counting algorithm used in [6]: results are shown in Fig. 4. We tested the algorithm, by computing fractal dimensions of curves generated ...

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