Theory of the Fireball
Theory of the Fireball
Theory of the Fireball
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shock, Eq. (3.15) . Next comes t'ne cooling wave I11 in whicn t e temper-<br />
ature falls more steeply, according to (3.8) . (At late times, region I1<br />
is wiped out and I11 follows immediately upon I . ) Region IV includes<br />
<strong>the</strong> material which has gone through tne cooling wave, and now cools adi-<br />
abatically; nence <strong>the</strong> temperature falls slowly with r (Sec . 'jd) D is<br />
<strong>the</strong> material point from whicn <strong>the</strong> cooling wave started originally; region<br />
V, outside that point, is also expanding adiabatically, but from snock<br />
conditions; thus it is <strong>the</strong> continuation <strong>of</strong> region 11. Finally region VI<br />
is <strong>the</strong> air not yet shocked. As time goes on, <strong>the</strong> cooling wave I11 moves<br />
inward, wiping out region I1 and <strong>the</strong>n eating into region I. Region IV<br />
accordingly grows toward <strong>the</strong> inside, but its outer end D stays fixed.<br />
Region V expands into VI by shock.<br />
We note once more that u is <strong>the</strong> velocity in Lagrange coordinates,<br />
2<br />
and in gm/cm sec. The problem is xnade somewhat more complicated by <strong>the</strong><br />
three dimensions and <strong>the</strong> adiabatic expansion, cf. Sec. 6, but tne prin-<br />
cipal features remain <strong>the</strong> same<br />
d. Adiabatic Expansion after Cooling. Radiating Temperature<br />
When a given material element has gone through <strong>the</strong> cooling wave, it<br />
is left at <strong>the</strong> radiating temperature T1. Thereaf'ter, it w ill expand<br />
adiabatically. Equation (3.25) shows that for adiabatic expansion<br />
or, using (3.10)<br />
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