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Theory of the Fireball

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The W beyond 3.5 ev will be strongly absorbed at 4 0'. Thus <strong>the</strong> layers<br />

<strong>of</strong> air at intermediate temperatures get additional heat which counteracts<br />

and may even exceed <strong>the</strong> adiabatic cooling. This will tend to increase<br />

<strong>the</strong> thickness <strong>of</strong> <strong>the</strong> medium-temperature layer. This in turn will (mod-<br />

erately) lower <strong>the</strong> radiating temperature, but three-dimensional effects<br />

act <strong>the</strong> opposite way (Sec. 6) .<br />

a . <strong>Theory</strong> <strong>of</strong> Zel 'dovich et al.<br />

Zelsdovich, Kompaneets, and Raizer lo (quoted as Z) have considered<br />

<strong>the</strong> loss <strong>of</strong> radiation by hot material when <strong>the</strong> absorption coefficient<br />

for <strong>the</strong> radiation increases monotonically with temperature. They have<br />

shown that in this case a cooling wave proceeds into <strong>the</strong> hot material<br />

from <strong>the</strong> outside. Tnis is to say, <strong>the</strong> cool temperature outside gradually<br />

eats its way into <strong>the</strong> hot material, while <strong>the</strong> material in <strong>the</strong> center<br />

remains unaffected and merely expands adiabatically.<br />

For simplicity, ZelPdovich et al. consider a one-dimensional case.<br />

They fur<strong>the</strong>r as,sume that <strong>the</strong> specific heat is constant and express <strong>the</strong>ir<br />

<strong>the</strong>ory in terms <strong>of</strong> <strong>the</strong> temperature. This is not necessary; we shall<br />

merely assume that both <strong>the</strong> enthalpy H and <strong>the</strong> absorption coefficient<br />

for radiation are arbitrary but monotonically increasing functions <strong>of</strong> <strong>the</strong><br />

temperature. Like 2, we shall assume, in this subsection only, that <strong>the</strong><br />

radiation transport can be described by an opacity (Rosseland mean) ra<strong>the</strong>r<br />

than considering each wave length separately.<br />

44

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