The exploration of strongly interacting matter
André Mischke
Utrecht University
Inaugural presentation – Physics and Engineering Section, Academia Europaea – 3 September 2017
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The exploration of strongly interacting matter Andr Mischk e Utrecht University Inaugural presentation Physics and Engineering Section, Academia Europaea 3 September 2017 Outline About myself Structure of matter The
Inaugural presentation – Physics and Engineering Section, Academia Europaea – 3 September 2017
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Mechanism (Nobel Prize 2013)
couple of properties that are not well understood.
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Protons and neutrons are colour neutral states.
gluon quark
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Heat and pressure Phase transition to QGP
T ≈ 1012 K ≈ 105x sun’s core
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sun
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Quark-hadron phase transition
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Heat and pressure Phase transition to QGP
T ≈ 1012 K ≈ 105x sun’s core
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particle accelerator in the world
cutting edge
technology and computing
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helium at 1.9K (~120 tons)
5.5 TeV lead-lead collisions
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Size: 16 x 26 meters Weight: 10.000 tons 18 Sub-detectors Dipole magnet B=0.5 T
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bang
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“Run-2 data taking” from 2015-2018
Charm quark à D meson bound state
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beauty
proton proton heavy quark heavy quark
Reference measurement
after collision
Quark-Gluon Plasma
Collision of heavy atomic nuclei
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) c (GeV/
T
p
5 10 15 20 25 30 35 40
Nuclear modification factor
0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2
+
, D*
+
, D Average D ALICE
|<0.5 y = 2.76 TeV, |
NN
s Pb-Pb, 0-10%
T
p with pp 30-50% <0.04
cms
y = 5.02 TeV, -0.96 <
NN
s p-Pb,
ALICE
ALI−PUB−99591
Transverse momentum ß No plasma ß With plasma
André Mischke (Utrecht University)
RAA( pT ) = YieldAA( pT ) Nbin
AA Yieldpp( pT )
Nuclear modification factor
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between quarks and gluons in the plasma phase?
energy loss and dissipation in the plasma
Particle accelerator: collision of heavy atomic nuclei
Quark-Gluon Plasma Big Bang
Quark-Gluon-Plasma is a new form of strongly interacting matter
Evolution of the universe Atomic nuclei
One of the central questions in the NuPECC LRP report
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