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RADIATION PROTECTION - ILEA

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Historical Prologue 5<br />

science of radioactive substances and the radiations they emit. Thus, by<br />

1900, scientists had begun to discover and experiment with high-energy<br />

radiations of the kind that had dominated the universe during its early<br />

history.<br />

At about the same time, the work of Planck in 1900 and Einstein in<br />

1905 showed that many kinds of radiation, including heat radiation, visible<br />

light, ultraviolet light, and radiowaves, which had previously appeared<br />

to be transmitted as continuous waves of energy, were actually emitted as<br />

discrete bundles of energy called photons, and that differences among<br />

these types of radiation could be characterized in terms of the different energies<br />

of the photons. In time, it was learned that gamma radiation, emitted<br />

from the nuclei of atoms, and x rays, produced by the acceleration of<br />

electrons (outside the nucleus), were also made up of photons of electromagnetic<br />

radiation, but of much higher energies.<br />

The discovery of the new particles and rays led to intense experimentation<br />

on their properties and their interactions with matter. The energetic<br />

alpha particles (actually helium nuclei) emitted by radioactive materials<br />

were directed by Rutherford against thin gold foils. Through analysis of<br />

the scattering pattern, he deduced in 1911 that the atom was composed of<br />

a tiny central core, or nucleus, containing all the positive charge and almost<br />

all the mass of the atom, and a nearly empty surrounding region containing<br />

the light, negatively charged electrons, in sufficient number to balance<br />

out the inner positive charge. The nucleus of the hydrogen atom,<br />

consisting of a single particle with a charge equal in magnitude and opposite<br />

in sign to that of the electron, was recognized as a fundamental building<br />

block of the nuclei of all complex atoms. It was named the proton<br />

(from the Greek protos, which means “first”). With the development of the<br />

theory of the atomic nucleus composed of protons and other elementary<br />

particles, it was possible to visualize how certain types of nuclei could disintegrate<br />

and emit particles.<br />

The emitted particles had very high energies, and the source of the energies<br />

was a puzzle until the formulation by Einstein in 1905 of the massenergy<br />

equation. This equation expressed in quantitative terms his conclusion<br />

that matter could be converted into energy according to the relationship<br />

E = mc 2 , where E was the energy, m the mass, and c the velocity of<br />

light. If m was expressed in kilograms and c was expressed in meters per<br />

second, the equivalent energy E was given in a unit of energy known as the<br />

joule. When it later became possible to determine the masses of individual<br />

particles in an instrument known as the mass spectrograph, the relationship<br />

between mass and energy was verified experimentally. Whenever a<br />

particle was emitted from a nucleus with high energy, it was found that the<br />

mass of the nucleus decreased not only by the rest mass of the particles

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