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eing that 'qu<strong>an</strong>tum' is a more, inclusive term, which c<strong>an</strong> be<br />

applied to other things as well<br />

as light - for inst<strong>an</strong>ce - to<br />

the vibration <strong>of</strong> whole atoms <strong>an</strong>d molecules.<br />

T8P - Text number 8 - Physics<br />

THE QUANTUM THEORY OF RADIATION (Part two)<br />

The qu<strong>an</strong>tum <strong>of</strong> radi<strong>an</strong>t energy differs from<br />

the<br />

qu<strong>an</strong>tum <strong>of</strong> electricity, the electron, in a very import<strong>an</strong>t way.<br />

The amount <strong>of</strong> charge is the same on all electrons: there<br />

is<br />

but one unit. The magnitude <strong>of</strong> this unit <strong>of</strong> radi<strong>an</strong>t<br />

energy,<br />

however, is different for every different wave-length <strong>of</strong><br />

radiation. It is, in fact, proportional to the frequency, so<br />

that the qu<strong>an</strong>tum <strong>of</strong> energy <strong>of</strong> extreme visible red radiation is<br />

only half that <strong>of</strong> the extreme visible violet radiation,<br />

which,<br />

as we have said before, hîs double the frequency. The qu<strong>an</strong>tum<br />

<strong>of</strong> <strong>an</strong> X-radiation<br />

is very much greater th<strong>an</strong> the qu<strong>an</strong>tum <strong>of</strong> <strong>an</strong>y<br />

visible<br />

radiation.<br />

The qu<strong>an</strong>tum <strong>of</strong> energy corresponding<br />

to a given<br />

species <strong>of</strong> radiation is found, then, <strong>by</strong> multiplying the frequency<br />

<strong>by</strong> a certain fixed number, which is called Pl<strong>an</strong>ck's universal<br />

const<strong>an</strong>t, <strong>an</strong>d always indicated <strong>by</strong> Ih. Pl<strong>an</strong>ck's const<strong>an</strong>t enters<br />

into every aspect <strong>of</strong> modern atomic physics <strong>an</strong>d its<br />

numerical<br />

value has been found <strong>by</strong> at least ten different methods,<br />

involving<br />

such things as X-ray properties, the distribution<br />

<strong>of</strong> energy in<br />

black-body radiation, the frequencies <strong>of</strong> spectral lines, <strong>an</strong>d so<br />

on. All the methods give values agreeing to within a few parts<br />

in ten<br />

thous<strong>an</strong>d.<br />

Light, then, or radiation<br />

in general, has a packet

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