A Treatise on the Theory of Screws

Forfatter: Sir Robert Stawell Ball

År: 1900

Forlag: The University Press

Sted: Cambride

Sider: 544

UDK: 531.1

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410] THE THEORY OF SCREWS IN NON-EUCLIDIAN SPACE. 449 (VII) The departure between two ranges cannot be zero unless the ranges are coincident, or unless the departure between every pair of ranges in that star is also zero. (VIII) Of the ranges in a star, two (distinct or coincident) are at infinity, i.e. have each an infinite departure from all the remainder. (IX) An infinite range has an infinite departure, not only with every range in its star, but with every range in the extent. (X) If the several ranges in one star correspond one to one with the several ranges in another, and if the two infinite ranges in one star have as their correspondents the infinite ranges in the other; then the departure between any two ranges in one star is equal to that between the two corre- sponding ranges in the other. 409. The Form of the Departure Function. The analogy of these several axioms to those which have guided us to the discovery of the intervene, shows that the investigation for the function of departure will be conducted precisely as that of the intervene has been; accordingly, we need not repeat the several steps of the investigation, but enunciate the general result, as follows :— Let xlt x2, and ylt y2 be the co-ordinates of any two ranges in a star, and let Xi, Xs, and g2 be iAe co-ordinates of the two infinite ranges in that star. Then the departure between (xlt x2) and (ylt y2) is (yig2 — y-ipi) (.yih^ — y2h-i) — x2ffi) 410. On the Arrangement of the Infinite Ranges. Every star in the extent will have two infinite ranges, and we have now to see how these several infinite ranges in the extent can be compendiously organized into a whole. To aid in this we have assumed Axiom IX., the effect of which is to render the following statement true. Let several objects on a range, 0, be the vertices of a corresponding number of stars. If 0 be an infinite range in any one of the stars, then it is so in every one. Let alt a2, as be any three ranges in an extent. Then every range in the same extent can be expressed by ÆqCl'l ^2^2 ‘^•3^3 j where xlt x2, xs are the three co-ordinates of the range. It is required to determine the relation between xlt x2, x3 if this range be infinite. B. 29