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Relativistic heavy ion collisions
wan ahmad tajuddin wan abdullah jabatan fizik universiti malaya
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Hot dense nuclear matter
Quark-gluon plasma Hot dense nuclear matter
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CERN 17 GeV/ nucleon Pb LBL 1-2 GeV/ nucleon JINR 6 GeV/ nucleon BNL BNL 200 GeV/ nucleon pair Cu, Au, U CERN 2.76 TeV/ nucleon pair Pb
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why condition in first microseconds in hot Big Bang
QCD state at high temperatures Hadronization (~ confinement)
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Typical temperature range –
T = 300 MeV/k = 3.3 x 1012 K 10,000 x greater than in center of Sun Corresponding energy density – e =10 GeV/ fm3 Corresponding relativistic matter pressure – P ≈ e/3 = 0.52 x 1031 bar
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Strangeness enhancement
high temperature → strangeness enhanced Statistics: particle ratios → Tch , mB at chemical freezeout Experimental: 160 MeV < Tch < 180 MeV cf. expected QCD phase transition value ~170 MeV (lattice QCD calculations)
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Heavy quarkonium suppression
hot and deconfined medium – quarkonia (cf naked flavours) expected to “melt”
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Jet quenching images courtesy CERN
coloured particles damped in coloured media
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Elliptic flow Collective anisotropy thermalization, hydrodynamics liquid-like
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Colour glass condensate
BFKL dynamics – saturation at Q2s ~ <Npart>/2 expect nch/A ~ 1/as(Q2s)
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