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)
[13]It has been attempted to remedy this lack of knowledge by considering
the charged particles as proper singularities. But in my opinion this means
giving up a real understanding of the structure of matter. It seems to me
much better to give in to our present inability rather than to be satisfied
by a solution that is only apparent.
[Pg 53]
General Expressions for the Conservation Principles. We
can hardly avoid making the assumption that in all other cases,
also, the space distribution of energy is given by a symmetrical
tensor, , and that this complete energy tensor everywhere
satisfies the relation (47c). At any rate we shall see that by
means of this assumption we obtain the correct expression for
the integral energy principle.
Let us consider a spatially bounded, closed system, which,
four-dimensionally, we may represent as a strip, outside of which
the vanish. Integrate equation (47c) over a space section.
Since the integrals of
,
and
vanish because
the vanish at the limits of integration, we obtain
Inside the parentheses are the expressions for the momentum of
the whole system, multiplied by , together with the negative
energy of the system, so that (49) expresses the conservation
principles in their integral form. That this gives the right conception
of energy and the conservation principles will be seen
from the following considerations.
PHENOMENOLOGICAL REPRESENTATION OF THE
ENERGY TENSOR OF MATTER.
Hydrodynamical Equations. We know that matter is built
up of electrically charged particles, but we do not know the laws
which govern the constitution of these particles. In treating mechanical
problems, we are therefore obliged to make use of an
[Pg 54]
inexact description of matter, which corresponds to that of classical
mechanics. The density , of a material substance and the
hydrodynamical pressures are the fundamental concepts upon
which such a description is based.
FIG. 3.
Let be the density of matter at a place, estimated with
reference to a system of co-ordinates moving with the matter.
Then , the density at rest, is an invariant. If we think of the
matter in arbitrary motion and neglect the pressures (particles
of dust in vacuo, neglecting the size of the particles and the
temperature), then the energy tensor will depend only upon the
[Pg 55]
velocity components, and . We secure the tensor character
of by putting
in which the , in the three-dimensional representation, are
given by (41). In fact, it follows from (50) that for ,
(equal to the negative energy per unit volume), as it should,
according to the theorem of the equivalence of mass and energy,
and according to the physical interpretation of the energy tensor
given above. If an external force (four-dimensional vector, )
acts upon the matter, by the principles of momentum and energy
the equation
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