| Low-discrepancy Sequence |
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Information AboutLow-discrepancy Sequence |
| CATEGORIES ABOUT LOW-DISCREPANCY SEQUENCE | |
| numerical analysis | |
| quasirandomness | |
| diophantine approximation | |
| sequences | |
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In Mathematics , a low-discrepancy sequence is a Sequence with the property that for all ''N'', the subsequence ''x''1, ..., ''x''''N'' is almost uniformly distributed (in a sense to be made precise), and ''x''1, ..., ''x''''N''+1 is almost uniformly distributed as well. The reader may wish to consider this Illustration Of A Low-discrepancy Sequence . Low-discrepancy sequences are also called quasi-random or '''sub-random''' sequences, due to their use in situations similar to those when Pseudorandom or Random Number s are used instead. The "quasi" modifier is used to denote more clearly that the numbers are not random (and to differentiate them from pseudorandomness, which uses different assumptions), but have useful properties similar to Randomness in certain applications such as the Quasi-Monte Carlo Method . The notion of ''uniformity'' is made precise as the discrepancy defined below. Roughly speaking, the discrepancy of a sequence is low if the number of points falling into a set ''B'' is close to the number one would expect from the measure of ''B''. At least three methods of Numerical Integration can be phrased as follows. Given a set ''x''1, ..., ''x''''N'' in the interval : If the points are chosen as ''x''''i'' = ''i''/''N'', this is the '' Rectangle Rule ''. If the points are chosen to be randomly (or Pseudorandom ly) distributed, this is the '' Monte Carlo Method ''. If the points are chosen as elements of a low-discrepancy sequence, this is the '' Quasi-Monte Carlo Method ''. A remarkable result, the Koksma-Hlawka inequality, shows that the error of such a method can be bounded by the product of two terms, one of which depends only on ''f'', and another which is the discrepancy of the set ''x''1, ..., ''x''''N''. The Koksma-Hlawka inequality is stated below. It is convenient to construct the set ''x''1, ..., ''x''''N'' in such a way that if a set with ''N''+1 elements is constructed, the previous ''N'' elements need not be recomputed. The rectangle rule uses points set which have low discrepancy, but in general the elements must be recomputed if ''N'' is increased. Elements need not be recomputed in the Monte Carlo method if ''N'' is increased, but the point sets do not have minimal discrepancy. By using low-discrepancy sequences, the quasi-Monte Carlo method has the desirable features of the other two methods. DEFINITION OF DISCREPANCY The Star-Discrepancy is defined as follows, using Niederreiter's notation.
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D^ N(P) |
\{
m disc}\_\infty |
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: <math> \left Rac{1}{N} \sum {i |
1}^N f(x_i) |
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\left Rac{1}{N} \sum {i |
1}^N f(x_i) |
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