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NOTES ON THE ORIGIN OF THE GENERAL THEORY OF, RELATIVITY 285<br />

. tion of masses and changes with it, the geometric structure of<br />

this space is also dependent on physical fac<strong>to</strong>rs. Thus, according<br />

<strong>to</strong> this theory space is-exactly as Riemann guessed-no<br />

longer absolute; its structure depends on physical infiuences.<br />

(Physical) geometry is no longer an isolated self-contained science<br />

like the geometry of Euclid.<br />

The problem of gravitation was thus reduced <strong>to</strong> a mathematical<br />

problem: it was required <strong>to</strong> find the simplest fundamental<br />

equations which are covariant with respect <strong>to</strong> arbitrary coordinate<br />

transformation. This was a well-defined problem that<br />

could at least be solved.<br />

I will not speak here of the experimental confinnation of this<br />

theory, but explain at once why the theory could not rest permanently<br />

satisfied with this success. Gravitation had indeed been<br />

deduced from the structure of space, but besides the gravitational<br />

field there is also the electromagnetic field. This had, <strong>to</strong><br />

begin with, <strong>to</strong> be introduced in<strong>to</strong> the theory as an entity independent<br />

of gravitation. Terms which <strong>to</strong>ok account of the<br />

existence of the electromagnetic field had <strong>to</strong> be added <strong>to</strong> the<br />

fundamental field equations. But the idea that there exist two<br />

structures of space independent of each other, the metric-gravitational<br />

and the electromagnetic, was in<strong>to</strong>lerable <strong>to</strong> the theoretical<br />

spirit. We are prompted <strong>to</strong> the belief that both·sorts of field<br />

must correspond <strong>to</strong> a unified structure of space.<br />

NOTES ON THE ORIGIN OF THE GENERAL<br />

THEORY OF RELATIVITY<br />

Mein Weltbild, Amsterdam: Querida Verlag, 1934.<br />

I gladly accede <strong>to</strong> the request that I should say something<br />

about the his<strong>to</strong>ry of my own scientific work. Not that I have<br />

an exaggerated notion of the importance of my own efforts, but<br />

<strong>to</strong> write the his<strong>to</strong>ry of other men's work demands a degree of<br />

absorption in other people's ideas which is much more in the<br />

line of the trained his<strong>to</strong>rian; <strong>to</strong> tllrow light on one's own earlier<br />

thinking appears in<strong>com</strong>parably easier. Here one has an immense<br />

advantage over everybody else, and one ought not <strong>to</strong><br />

leave the opportunity unused out of modesty.

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