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XXIII.—On the Cardinal Function of Interpolation-Theory
Published online by Cambridge University Press: 15 September 2014
Extract
The function which is discussed in the greater part of this paper was introduced by Professor E. T. Whittaker in vol. xxxv (1915), pp. 181–194 of these Proceedings. A one-valued function, analytic in the finite part of the plane save possibly for poles, is taken and a table made of the values of f(x) for x = a, a + w, a — w, a + 2w, a — 2w, … The function
called the Cardinal Function, is then shown to be the simplest function satisfying the table of values so obtained, in that it is a function which, when analysed into its periodic constituents, has no rapid oscillations.
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References
page 269 note * References to this in the present paper are denoted by (I).
page 271 note * This fact was pointed out, but not discussed fully, in a paper by Brown, T. Arnold, Proc. Edin. Math. Soc., xxxiv (1915–16)Google Scholar.
page 271 note † yr is assumed to be bounded as r→∞.
page 273 note * Bromwich, Theory of Infinite Series (1908), p. 205.
page 273 note † Cf. N. Nielsen, Handbuch der Theorie der Gammafunktion (B. G. Teubner, Leipzig, 1906), p. 127. In further references this work is denoted by (II).
page 274 note * K. Ogura, Tôhoku Math. Journal, vol. xvii, p. 141, has shown that Newton's formula is also expressible as an integral, viz. -1<R(z)<0 where ϕ(t) = f 0 - tδf + t 2δ2f 1-…. The present integral is, essentially, an expression for the Gauss formula in terms of the tabulated values.
page 280 note * An Introduction to the Theory of Infinite Series (1908), p. 123.
page 280 note † Carmichael, R. D., Bull. Amer. Math. Soc. (2), vol. xxv (1918–19), p. 113Google Scholar; or T. H. Gronwall, Comptes Rendus (June 1914), vol. clviii, p. 1664.
page 281 note * I hope to publish shortly a note dealing with this point.
page 281 note † Norlünd, , Annales Sci. de l'Ecole Normale (3), vol. xxxix (1922), p 365Google Scholar.
page 281 note ‡ Dougall, , Proc. Edin. Math. Soc., vol. xviii (1900), p. 78Google Scholar, has used this theorem to obtain some useful expansions in the theory of spherical harmonics.
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