The Meaning of Relativity: Four lectures delivered at Princeton University, May, 1921 — John Shaqi
The Meaning of Relativity: Four lectures delivered at Princeton University, May, 1921Einstein, Albert
Science
The Meaning of Relativity: Four lectures delivered at Princeton University, May, 1921
Einstein, Albert
Relativity (Physics)
The equations of motion of a material particle are
() is a vector; , and therefore also , an invariant; thus
[Pg 17]
() is a vector; in the same way it may be shown that
() is a vector. In general, the operation of differentiation
with respect to time does not alter the tensor character. Since
is an invariant (tensor of rank 0), )
is a vector, or
tensor of rank 1 (by the theorem of the multiplication of tensors).
If the force () has a vector character, the same holds for
the difference (. These equations of motion are
therefore valid in every other system of Cartesian co-ordinates
in the space of reference. In the case where the forces are conservative
we can easily recognize the vector character of ().
For a potential energy, , exists, which depends only upon the
mutual distances of the particles, and is therefore an invariant.
The vector character of the force, = ,
is then a consequence of our general theorem about the derivative of a tensor
of rank 0.
Multiplying by the velocity, a tensor of rank 1, we obtain the
tensor equation
By contraction and multiplication by the scalar we obtain the
equation of kinetic energy
[Pg 18]
If denotes the difference of the co-ordinates of the material
particle and a point fixed in space, then the have the
character of vectors. We evidently have
= , so that
the equations of motion of the particle may be written
Multiplying this equation by we obtain a tensor equation
Contracting the tensor on the left and taking the time average
we obtain the virial theorem, which we shall not consider
further. By interchanging the indices and subsequent subtraction,
we obtain, after a simple transformation, the theorem of
moments,
It is evident in this way that the moment of a vector is not a
vector but a tensor. On account of their skew-symmetrical character
there are not nine, but only three independent equations of
this system. The possibility of replacing skew-symmetrical tensors
of the second rank in space of three dimensions by vectors
depends upon the formation of the vector
[Pg 19]
If we multiply the skew-symmetrical tensor of rank 2 by the
special skew-symmetrical tensor introduced above, and contract
twice, a vector results whose components are numerically
equal to those of the tensor. These are the so-called axial vectors
which transform differently, from a right-handed system to
a left-handed system, from the . There is a gain in
picturesqueness in regarding a skew-symmetrical tensor of rank 2
as a vector in space of three dimensions, but it does not represent
the exact nature of the corresponding quantity so well as
considering it a tensor.
Public-domain text, read in full here on John Shaqi.
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