Relativity : the Special and General Theory eBook

This eBook from the Gutenberg Project consists of approximately 117 pages of information about Relativity .

Relativity : the Special and General Theory eBook

This eBook from the Gutenberg Project consists of approximately 117 pages of information about Relativity .

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) 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 to real numbers lying between 1 and 2. fig. 04 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 P1 on the surface then correspond to the co-ordinates

P:  u,v

P1:  u + du, v + dv,

where du and dv signify very small numbers.  In a similar manner we may indicate the distance (line-interval) between P and P1, as measured with a little rod, by means of the very small number ds.  Then according to Gauss we have

ds2 = g[11]du2 + 2g[12]dudv = g[22]dv2

where g[11], g[12], g[22], are magnitudes which depend in a perfectly definite way on u and v.  The magnitudes g[11], g[12] and g[22], 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 coordinates are samply 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.”

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Relativity : the Special and General Theory from Project Gutenberg. Public domain.