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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Jet Quenching<br />
The jet has to make its way out through the hot <strong>and</strong> dense medium<br />
Energy loss (stopping power) depends<br />
critically on type <strong>of</strong> medium:<br />
Hadronic Medium: ~ 0.2 - 0.4 GeV/fm<br />
Partonic Medium: ~ 2 – 3 GeV/fm<br />
<strong>Hot</strong> <strong>and</strong> <strong>Dense</strong> <strong>Nuclear</strong> matter 21