The Meaning of Relativity: Four lectures delivered at Princeton University, May, 1921Einstein, Albert
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The Meaning of Relativity: Four lectures delivered at Princeton University, May, 1921
Einstein, Albert
Relativity (Physics)
Observing that the field equation (96) may be written in the
form
we get from (96) the equations,
From this follows
If the universe is quasi-Euclidean, and its radius of curvature
therefore infinite, then σ would vanish. But it is improbable that
[Pg 113]
the mean density of matter in the universe is actually zero; this
is our third argument against the assumption that the universe
is quasi-Euclidean. Nor does it seem possible that our hypothetical
pressure can vanish; the physical nature of this pressure can
be appreciated only after we have a better theoretical knowledge
of the electromagnetic field. According to the second of equations
(123) the radius, , of the universe is determined in terms
of the total mass, , of matter, by the equation
The complete dependence of the geometrical upon the physical
properties becomes clearly apparent by means of this equation.
Thus we may present the following arguments against the
conception of a space-infinite, and for the conception of a space-bounded,
universe:—
1. From the standpoint of the theory of relativity, the condition
for a closed surface is very much simpler than the corresponding
boundary condition at infinity of the quasi-Euclidean
structure of the universe.
2. The idea that Mach expressed, that inertia depends upon
the mutual action of bodies, is contained, to a first approximation,
in the equations of the theory of relativity; it follows
from these equations that inertia depends, at least in part, upon
mutual actions between masses. As it is an unsatisfactory assumption
to make that inertia depends in part upon mutual
actions, and in part upon an independent property of space,
Mach's idea gains in probability. But this idea of Mach's corresponds
only to a finite universe, bounded in space, and not to a
quasi-Euclidean, infinite universe. From the standpoint of epistemology
[Pg 114]
it is more satisfying to have the mechanical properties
of space completely determined by matter, and this is the case
only in a space-bounded universe.
3. An infinite universe is possible only if the mean density of
matter in the universe vanishes. Although such an assumption
is logically possible, it is less probable than the assumption that
there is a finite mean density of matter in the universe.
[Pg 115]
INDEX
A
Accelerated masses, inductive
action of, 108
Addition and subtraction of
tensors, 14
—theorem of velocities, 38
B
Biot-Savart force, 44
C
Centrifugal force, 64
Clocks, moving, 38
Compressible viscous fluid, 22
Concept of space, 3
—time, 28
Conditions of orthogonality, 7
Congruence, theorems of, 3
Conservation principles, 54
Continuum, four-dimensional, 31
Contraction of tensors, 14
Contra-variant vectors, 69
—tensors, 71
Co-ordinates, preferred systems
of, 8
Co-variance of equation of
continuity, 21
Co-variant, 12 et seq.
—vector, 68
Criticism of principle of inertia, 62
Criticisms of theory of
relativity, 29
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