The electron, its isolation and measurement and the determination of some of its propertiesMillikan, Robert Andrews
Philosophy
The electron, its isolation and measurement and the determination of some of its properties
Millikan, Robert Andrews
Electrons
But a beautiful discovery by Klein and Rosseland[187] a little
later, in Bohr’s Institute, made this conclusion unnecessary. For it
showed that there was an intermediate process, namely, a so-called
collision of the second kind, by means of which the energy
might be transferred without loss, indirectly from the
light-wave to the conduction electron, thus obviating the necessity
of a direct transfer. In other words, the Klein and Rosseland
discovery proved that the energy could be transferred from
the light-wave to the conduction electron by being absorbed first by
[Pg 256]
an atom, which would thus be changed from the normal to the excited
state, i.e., the state in which one of its electrons has been lifted
from a normal to an outer orbit. This excited atom could then return to
its normal state without radiation by a collision “of the second
kind,” which consists in transferring its whole absorbed energy
to a free or conduction electron. The reality of this phenomenon
has been experimentally checked by Franck and Cario.[188] This
important discovery then left the evidence for localized light-quanta
precisely where it was before.[189]
Within the past year, however, a young American physicist, Dr. A. H.
Compton, of the University of Chicago, has discovered another new
phenomenon which constitutes perhaps the best evidence yet found in
favor of Einstein’s hypothesis of localized light-quanta.
Compton’s procedure is as follows. Assuming, for the sake of obtaining
quantitative relations, the correctness of Einstein’s hypothesis, he
argues that when such a “light-quanta” collides with a free
electron the impact should be governed by the laws which hold for the
collision between any material bodies. These are two in number, namely:
(1) the principle of the conservation of energy; (2) the principle of
the conservation of momentum (Newton’s Third Law).
Now the energy of a light-quanta, as heretofore shown, is .
It moves with the speed of light, , and if its momentum is taken
as , it follows at once from the Einstein relativity relation
[Pg 257]
between energy and mass, namely, , that its
momentum is . This is seen by substituting in the
foregoing Einstein relation for energy. Or, if preferred, the
same expression for momentum may be deduced easily from the established
laws of light-pressure.
The qualitative results of the preceding assumptions are immediately
seen to be as follows. The light-quanta, by colliding with the free
electron necessarily transfers some of its energy to it, and therefore,
if it arrives with the energy , it must recoil from
the impact at some angle with a smaller energy ,
and therefore a lower frequency , than
that with which it impinged. In other words, light waves should be
changed from a higher frequency to a lower—from blue toward red—by
impact with a free electron.
[Pg 258]
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