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7. Probability and Statistics Soviet Essays - Sheynin, Oscar

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nlimk = 1P(| k (n) – m k (n) | > H n ) = 0 as n (1.2.3)for any > 0 is necessary <strong>and</strong> sufficient forF(t) = (1/t2 π ) −∞exp[– (t – a) 2 /2 2 ] dt.Feller was the first to publish the necessary <strong>and</strong> sufficient conditions themselves in anexplicit form for attraction to the Gauss law under restriction (1.2.2). They can be expressedin the following way: For the existence of constants C n <strong>and</strong> H n > 0 such that conditions(1.2.1) <strong>and</strong> (1.2.2) are satisfied, it is necessary <strong>and</strong> sufficient that such constants K n exist forwhichlim inf P(| n – m n | > K n ) > 0 as n , (1.2.4a)nlimk = 1P(| k (n) – m k (n) | > K n ) = 0 as n . (1.2.4b)The former relation concerns properties of the sums rather than that of separate terms <strong>and</strong> itcan be written down in an equivalent formnlim inf K n2k = 1K( n)( ξk−2 ( n)n( ξkmξ− m( n)2k)( n)2ξk)> 0 as n , (1.2.4a)free, as (1.2.4b) also is, from the indicated shortcomings but somewhat less obvious.Bernstein [13; 40] originated a similar investigation of the conditions for the attraction ofsums of independent vectors to n-dimensional Gauss laws. In the <strong>Soviet</strong> Union, Khinchin,Romanovsky <strong>and</strong> Gnedenko followed up this direction; the last-mentioned author offered themost polished formulation [25].1.3. Specifying the Classical Limit Theorem. Even now, normal attractionlim F n (t) = (t) as n ,F n (t) = P[( n – A n )/Bn< t], (t) = (1/t2 π ) −∞exp[– (t 2 /2) dt,remains the most important case of attraction to the Gauss law. The desire to estimate asprecisely as possible the difference F n (t) – (t) is natural, both theoretically <strong>and</strong> practically.If this difference is not sufficiently small, it is also natural to add to (t) some correctionterms expressed simply enough through the distributions of the terms k (n) so that F n (t) willthen be estimated sufficiently precisely.In 1911, Bernstein discovered the most effective method of precisely estimating F n (t) forthe particular instance of the Laplace limit theorem; later he [39] somewhat strengthened hisfindings. The foundation of most of the subsequent investigations of the general case isChebyshev’s method. It approximately represents F n (t) as a series of the type of(t) + C 3 (n) (3) (t) + … + C s (n) (s) (t) + …

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