According to the general theory of relativity, the geometrical properties of space are not independent, but they are determined1 by matter. Thus we can draw conclusions about the geometrical structure of the universe only if we base our considerations on the state of the matter as being something that is known. We know from experience that, for a suitably chosen co-ordinate system, the velocities2 of the stars are small as compared with the velocity3 of transmission of light. We can thus as a rough approximation arrive at a conclusion as to the nature of the universe as a whole, if we treat the matter as being at rest.
We already know from our previous discussion that the behaviour of measuring-rods and clocks is influenced by gravitational fields, i.e. by the distribution of matter. This in itself is sufficient to exclude the possibility of the exact validity of Euclidean geometry in our universe. But it is conceivable that our universe differs only slightly from a Euclidean one, and this notion seems all the more probable, since calculations show that the metrics of surrounding space is influenced only to an exceedingly small extent by masses even of the magnitude of our sun. We might imagine that, as regards geometry, our universe behaves analogously4 to a surface which is irregularly curved in its individual parts, but which nowhere departs appreciably5 from a plane: something like the rippled6 surface of a lake. Such a universe might fittingly be called a quasi-Euclidean universe. As regards its space it would be infinite. But calculation shows that in a quasi-Euclidean universe the average density7 of matter would necessarily be nil8. Thus such a universe could not be inhabited by matter everywhere; it would present to us that unsatisfactory picture which we portrayed9 in Section XXX.
If we are to have in the universe an average density of matter which differs from zero, however small may be that difference, then the universe cannot be quasi-Euclidean. On the contrary, the results of calculation indicate that if matter be distributed uniformly, the universe would necessarily be spherical10 (or elliptical). Since in reality the detailed11 distribution of matter is not uniform, the real universe will deviate12 in individual parts from the spherical, i.e. the universe will be quasi-spherical. But it will be necessarily finite. In fact, the theory supplies us with a simple connection1 between the space-expanse of the universe and the average density of matter in it.
1 For the “radius” R of the universe we obtain the equation
upper R squared equals StartFraction 2 Over kappa rho EndFraction
The use of the C.G.S. system in this equation gives 2 slash13 kappa equals 1.08 dot 10 Superscript 27; rho is the average density of the matter and kappa is a constant connected with the Newtonian constant of gravitation.
The End
The End
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1 determined | |
adj.坚定的;有决心的 | |
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2 velocities | |
n.速度( velocity的名词复数 );高速,快速 | |
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3 velocity | |
n.速度,速率 | |
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4 analogously | |
adv.类似地,近似地 | |
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5 appreciably | |
adv.相当大地 | |
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6 rippled | |
使泛起涟漪(ripple的过去式与过去分词形式) | |
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7 density | |
n.密集,密度,浓度 | |
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8 nil | |
n.无,全无,零 | |
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9 portrayed | |
v.画像( portray的过去式和过去分词 );描述;描绘;描画 | |
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10 spherical | |
adj.球形的;球面的 | |
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11 detailed | |
adj.详细的,详尽的,极注意细节的,完全的 | |
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12 deviate | |
v.(from)背离,偏离 | |
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13 slash | |
vi.大幅度削减;vt.猛砍,尖锐抨击,大幅减少;n.猛砍,斜线,长切口,衣衩 | |
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