Az Eszterházy Károly Tanárképző Főiskola Tudományos Közleményei. 2001. Sectio Mathematicae (Acta Academiae Paedagogicae Agriensis : Nova series ; Tom. 28)

MÁTYÁS, F., Linea r recurrences and rootfinding methods

Linear recurrences and rootfinding methods 29 i. e. the sequence tends to the root a d of the polynomial (5) /(A) = A 2 - (a d + ß d)\ + cx dß d = A 2 - V dX + B d . Recently, many authors have studied the connection between recurrences and iterative transformations. The main idea is to consider such sequence transfor­mations T of the convergent sequence {A n}^_ 0 into the sequence {T n , where {T n}^l 0 converges more quickly to the same limit X. Thus, one can investigate the properties of these transformations or the accelerations of the convergence. We say that {T nconverges more quickly to X than {X nif T n — X = o(X n — X), i. e. if lim ((T N - X) / {X n - X)) = 0. n—+oo The most known four sequence transformations to accelerate the convergence of a sequence are the secant S(X n,X m), Newton-Raphson N(X n), Halley H(X n) and Aitken transformation A(X n , X m, Xt), namely if {A' n - { R^h \ and L 'J n=0 X = a d (i. e. the root of /(A) = Ü in (5)), then (6) S(X n,X m)= , A n + A m - Vd (7) N(X n) = A 2 - B c 2X r V d (8) H(X n) A3 - 3 B dX n + V dB> 3A' 2 - ZV dX, + K 2 Bd (9) A(X n,X m,X t) = y X n'\ l Y , A n — ZA m -t Af where we assume that division by zero does not occur. (The formulae (6)-(9) can be obtained from (5) using the known forms of the transformations S, N, H and A, or they can be found in [4] p. 366 and p. 369.) Some results from the recent past: G. M. Phillips [5] proved that if r n = ^J^­then A(r n_ t,r n,r n+ t) = r 2 n. J. H. McCabe and G. M. Phillips [3] generalized this for r n = , and they also proved that 5' (^r n,r mj = r n+ m and N(r n) = r 2 n. M. J. Jamieson [1] investigated the case r n = 1 for d > 1. J. B. Muskat [4], using the notations r n = l and R n — Vy + d (d > 1), proved that (a) S(r n, r m) — r n_f. m, ,b (R n, Rm) — ? > n-j. m, (10) (6) N(r n) = r 2 n, N(R n) = r 2 n,

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