19.11.2014 Views

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

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

The “Flow” Is Large<br />

• Value <strong>of</strong> v 2 in<br />

dn/dφ ~ 1 + 2 v 2 cos (2 φ) + ..<br />

saturates at ~ 0.2<br />

• Hydrodynamic calculations<br />

show this collective flow is<br />

– characteristic <strong>of</strong><br />

a strongly interacting<br />

state <strong>of</strong> matter with<br />

very low viscosity<br />

10<br />

5<br />

0<br />

−5<br />

−10<br />

−10 −5 0 5 10<br />

10<br />

5<br />

10<br />

5<br />

0<br />

−5<br />

−10<br />

−10 −5 0 5 10<br />

10<br />

5<br />

– established in the<br />

earliest (geometrically<br />

asymmetric) stage<br />

<strong>of</strong> the collision<br />

– The flow is as strong as it<br />

can be<br />

0<br />

−5<br />

−10<br />

−10 −5 0 5 10<br />

0<br />

−5<br />

−10<br />

−10 −5 0 5 10<br />

<strong>Hot</strong> <strong>and</strong> <strong>Dense</strong> <strong>Nuclear</strong> matter 29

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!