The atom and the Bohr theory of its structure : $b an elementary presentationHolst, Helge
Science
The atom and the Bohr theory of its structure : $b an elementary presentation
Holst, Helge
Atomic theory
In actual practice no body is absolutely black. Even a body coated
with lampblack reflects about 10 per cent. of the light waves incident
on it. The Danish physicist Christiansen remarked long ago that a
real black body could be produced only if an arrangement could be
made whereby the incident waves could be reflected several times
in succession before finally being emitted. To take the case of
lampblack, three such reflections would reduce the re-emission from
the lampblacked body to only ⁴/₁₀₀₀ of the radiation initially falling
on it. This type of black body was finally realized by making a cavity
in an oven having as its only opening a very small peep-hole, and
keeping the temperature of the wall of the oven uniform. If a ray is
sent into the cavity through the peep-hole, it will become, so to
speak, captured, because, when once inside it will suffer countless
reflections from the walls of the cavity, having more and more of its
energy absorbed at each reflection. Very little of the radiation thus
entering will ever get out again, and consequently such a body will
act very much like a “perfect black body” according to the theoretical
definition above. Accordingly, the radiation which is emitted from such
a glowing cavity through the peep-hole will be black or practically
black radiation.
The cavity itself will be criss-crossed in all directions by radiation
emitted from one part of the inner surface of the cavity and absorbed
by (and partially reflected from) other parts of the surface. When
the walls of the cavity are kept at a fixed and uniform temperature
there will automatically be produced a state of equilibrium in which
every cubic centimetre of the cavity will contain a definite quantity
of radiation energy, dependent only on the temperature of the walls.
Further, in the equilibrium state the radiation energy will be
distributed in a perfectly definite way (dependent as before on the
temperature only) among the various types of radiation corresponding to
different wave-lengths and frequencies. If there is too much radiation
of one kind and too little of another, the walls of the cavity will
absorb more of the first kind than they emit, and emit more of the
second kind than they absorb, and so the state will vary until the
right proportion for equilibrium is attained.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account