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Theory of the Fireball

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where Re is <strong>the</strong> outer edge <strong>of</strong> <strong>the</strong> layer. The original mass <strong>of</strong> <strong>the</strong> warm<br />

layer m is much larger than that <strong>of</strong> <strong>the</strong> iso<strong>the</strong>rmal spnere<br />

W<br />

At a later time, <strong>the</strong> mass <strong>of</strong> <strong>the</strong> warm layer is <strong>the</strong>n<br />

It does not change much.<br />

(6.24)<br />

Tne tepperature in t'ne warn layer goes from 10,000 to l;OOOo, For<br />

simplicity we assume that <strong>the</strong> density corresponds to <strong>the</strong> average temper-<br />

ature <strong>of</strong> 7O0Oo. Then, at <strong>the</strong> initial pressure used in Table VI11 Y Pa -<br />

4.1 bars, <strong>the</strong> density <strong>of</strong> <strong>the</strong> warm layer is p = 11 X<br />

W Po = 14Pa.<br />

This is much higher t'nan in Brode's calculations, Table VIII: In his<br />

calculations, <strong>the</strong> cooling wave has not reached tne iso<strong>the</strong>rmal sphere;<br />

with our assumptions it has, The difference is due to <strong>the</strong> different<br />

opacities assumed; it has <strong>the</strong> consequence that our warm layer is geo-<br />

metrically much thinner than his (Table VIII, last column) Subsequently<br />

<strong>the</strong> density decreases with pressure, not adiabatically but iso<strong>the</strong>rmally;<br />

in accord with Gilmore *s fornula (3.131, we assume

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