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Theory of the Fireball

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inconsistency in our apyroximations .<br />

In our one-diniensional tneoqy, tne end <strong>of</strong> Stage C I narks -<strong>the</strong> max-<br />

Snrrm. <strong>of</strong> radiation, both in temperature and total emission. In Stage C I<br />

because <strong>the</strong> material becomes more transparent. In Stage C I1 <strong>the</strong> reverse<br />

is <strong>the</strong> case, (5.39), because <strong>the</strong> material which has gone through <strong>the</strong><br />

cooling wave becomes thicker with time, (5,.32). Tnis material provides<br />

opacity for <strong>the</strong> visible light from <strong>the</strong> fireball; since it becomes more<br />

opaque, <strong>the</strong> radiation must now come from a layer <strong>of</strong> smaller absorption<br />

coefficient, (5.35), and <strong>the</strong>refore <strong>of</strong> lower temperature. As (5.36) sha~s,<br />

<strong>the</strong> increase <strong>of</strong> thickness (t 2n <strong>the</strong> denominator) is more important than<br />

<strong>the</strong> continued decrease <strong>of</strong> density (factor p 1/3 ). Tnese results will be<br />

modified in <strong>the</strong> three-dimensional <strong>the</strong>ory, Sec. 6.<br />

1<br />

The maximum temperature has been calculated as T = 0.92 or 1.08,<br />

from om two calculations; it is clearly close to 1, i.e., ~O,OOO~.<br />

This number is not too mucn out <strong>of</strong> line with observation considering<br />

tnat we have calculated a maximum. In fact, tne transition from Stage<br />

C I to C I1 cannot be sudden as we have assumed; <strong>the</strong> cooling wave must<br />

begin gradually, and tnerefore <strong>the</strong> temperature peak which we have calcu-<br />

lated will actually be cut <strong>of</strong>f (Fig. 3). The observable maximum may<br />

easily be 1000° lower than our calculation.<br />

66<br />

k

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