Hot and Dense Nuclear Matter - Department of Physics and Astronomy
Hot and Dense Nuclear Matter - Department of Physics and Astronomy
Hot and Dense Nuclear Matter - Department of Physics and Astronomy
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Collective Flow<br />
Preequilibrium<br />
Therma-<br />
Lization<br />
QGP<br />
phase?<br />
Mixed<br />
Phase<br />
Hadronization<br />
Expansion<br />
T =<br />
0.1 fm/c<br />
~ 1 fm/c<br />
3-4 fm/c<br />
8–10 fm/c<br />
10 – 20 fm/c<br />
Collective flow due to<br />
very early pressure<br />
gradients<br />
Recombination <strong>of</strong><br />
quarks into hadrons<br />
(hadronization)<br />
<strong>Hot</strong> <strong>and</strong> <strong>Dense</strong> <strong>Nuclear</strong> matter 27
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