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nydus/Relativity: The Special and General TheoryPublic

Albert Einstein provides a non-mathematical exposition of the special and general theories of relativity for readers interested in physics and philosophy. The text presents the core concepts in their original sequence and aims to explain the theories as simply as possible for those with a standard university-level education.

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Table of Contents

XXV

Gaussian Co-ordinates

According to Gauss, this combined analytical

and geometrical mode of handling the problem can be arrived at in the following way. We imagine a system of arbitrary curves (see [fig:4]Fig. 4) drawn on the surface of the table. These we designate as u-curves, and we indicate each of them by means of a number. The curves u=1, u=2 and u=3 are drawn in the diagram. Between the curves u=1 and u=2 we must imagine an infinitely large number to be drawn, all of which correspond

2in087 to real numbers lying between 1 and 2. We have then a system of u-curves, and this "infinitely dense" system covers the whole surface of the table. These u-curves must not intersect each other, and through each point of the surface one and only one curve must pass. Thus a perfectly definite value of u belongs to every point on the surface of the marble slab. In like manner we imagine a system of v-curves drawn on the surface. These satisfy the same conditions as the u-curves, they are provided with numbers

in a corresponding manner, and they may likewise be of arbitrary shape. It follows that a value of u and a value of v belong to every point on the surface of the table. We call these two numbers the co-ordinates of the surface of the table (Gaussian co-ordinates).

For example, the point P in the diagram has the Gaussian co-ordinates u=3, v=1. Two neighbouring points P and P on the surface then correspond to the co-ordinates

where du and dv signify very small numbers. In a similar manner we may indicate the distance (line-interval)

between P and P, as measured with a little rod, by means of the very small number ds. Then according to Gauss we have ds2=g11du2+2g12dudv+g22dv2, where g11, g12, g22, are magnitudes which depend in a perfectly definite way on u and v. The magnitudes g11, g12 and g22 determine the behaviour of the rods relative to the u-curves and v-curves, and thus also relative to the surface of the table. For the case in which the points of the surface considered form a Euclidean continuum

with reference to the measuring-rods, but only in this case, it is possible to draw the u-curves and v-curves and to attach numbers to them, in such a manner, that we simply have: ds2=du2+dv2. Under these conditions, the u-curves and v-curves are straight lines in the sense of Euclidean geometry, and

they are perpendicular to each other. Here the Gaussian co-ordinates are simply Cartesian ones. It is clear

that Gauss co-ordinates are nothing more than an association of two sets of numbers with the points of the surface considered, of such a nature that numerical values differing very slightly from each other are associated with neighbouring points "in space."

So far, these considerations hold for a continuum

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