Perspectives of Nuclear Physics in Europe - European Science ...
Perspectives of Nuclear Physics in Europe - European Science ...
Perspectives of Nuclear Physics in Europe - European Science ...
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an <strong>in</strong>crease at the deconf<strong>in</strong>ement temperature, albeit<br />
a much more gradual one, which is related to residual<br />
<strong>in</strong>teractions between the constituents.<br />
However, conf<strong>in</strong>ement is not the only phenomenon<br />
responsible for rapid changes <strong>in</strong> the thermodynamic<br />
state variables. The transition related to the break<strong>in</strong>g<br />
<strong>of</strong> chiral symmetry result<strong>in</strong>g <strong>in</strong> the dynamical generation<br />
<strong>of</strong> hadron masses and the appearance <strong>of</strong> pions as<br />
Goldstone bosons plays an essential role. The chiral<br />
transition is characterised by a rapid decrease <strong>of</strong> the<br />
quark-antiquark condensate with T and µ B , which <strong>in</strong> fact<br />
serves as an order parameter <strong>of</strong> strongly <strong>in</strong>teract<strong>in</strong>g matter.<br />
However, the key manifestations <strong>of</strong> chiral symmetry<br />
restoration are its observable consequences for the<br />
hadron spectrum. Chiral partners must be degenerate,<br />
imply<strong>in</strong>g significant modifications <strong>of</strong> hadronic spectral<br />
functions by the medium as the transition is approached.<br />
Schematic models and numerical studies with LQCD<br />
have been developed to quantify <strong>in</strong>-medium modification<br />
<strong>of</strong> physical observables due to the restoration <strong>of</strong><br />
chiral symmetry.<br />
The chiral condensate has been shown <strong>in</strong> LQCD to<br />
drop rapidly over the same temperature <strong>in</strong>terval where<br />
the energy density drops. This suggests that deconf<strong>in</strong>ement<br />
and the restoration <strong>of</strong> approximate chiral symmetry<br />
<strong>in</strong> QCD may be co<strong>in</strong>cidental. However, the exact relation<br />
between the deconf<strong>in</strong>ement and chiral phase transition<br />
is quantitatively far from established <strong>in</strong> LQCD.<br />
Recent LQCD calculations constra<strong>in</strong> the temperature<br />
<strong>of</strong> the chiral and deconf<strong>in</strong>ement transitions at µ B = 0 to<br />
T c ≈ 150 – 170 MeV. Methods have been developed <strong>in</strong><br />
LQCD to explore the shift <strong>of</strong> T c with µ B for µ B < 3T. Studies<br />
also <strong>in</strong>dicate the possible existence <strong>of</strong> a critical po<strong>in</strong>t<br />
(CP) <strong>in</strong> the phase diagram at f<strong>in</strong>ite µ B . They have further<br />
led to a quantification <strong>of</strong> the EoS <strong>of</strong> nuclear matter at<br />
Box 2. Broken chiral symmetry and<br />
the orig<strong>in</strong> <strong>of</strong> hadron masses<br />
The orig<strong>in</strong> <strong>of</strong> the masses <strong>of</strong> particles is one <strong>of</strong> the most<br />
fundamental questions that we may ask about nature.<br />
The visible matter <strong>in</strong> our universe ma<strong>in</strong>ly consists <strong>of</strong><br />
protons and neutrons, which have a mass <strong>of</strong> about<br />
1 GeV/c 2 each. However, with<strong>in</strong> the ‘Standard Model’,<br />
the elementary build<strong>in</strong>g blocks <strong>of</strong> protons and neutrons,<br />
the quarks and gluons, are massless. Gluons mediate<br />
the <strong>in</strong>teraction between the quarks and have, like the<br />
photons, no restmass. The quarks, on the other hand,<br />
should be massless due to a fundamental property <strong>of</strong><br />
the strong force, chiral symmetry. In laboratory experiments<br />
on Earth, however, we observe non-zero (and<br />
very different) quark masses (as shown <strong>in</strong> the figure<br />
below). In the ‘Standard Model’, quarks acquire mass<br />
through their <strong>in</strong>teraction with an elementary field fill<strong>in</strong>g<br />
all space, the so-called Higgs field. The Higgs field<br />
breaks chiral symmetry explicitly, generat<strong>in</strong>g quark<br />
masses. The search for the Higgs particle is one <strong>of</strong><br />
the ma<strong>in</strong> goals <strong>of</strong> the LHC experiments.<br />
The Higgs mechanism is able to expla<strong>in</strong> the masses<br />
<strong>of</strong> the heavy quarks (green bars <strong>in</strong> the figure). For the<br />
light quarks, which account for the mass <strong>of</strong> the matter<br />
surround<strong>in</strong>g us, the explicit symmetry break<strong>in</strong>g<br />
is very small, and the result<strong>in</strong>g small quark masses<br />
(5 – 10 MeV/c 2 ) are by far <strong>in</strong>sufficient to expla<strong>in</strong> the<br />
observed mass <strong>of</strong> hadrons (for example, the proton<br />
mass <strong>of</strong> ≈ 1 GeV/c 2 ). In order to expla<strong>in</strong> the mass <strong>of</strong> a<br />
hadron, the vacuum surround<strong>in</strong>g a quark or gluon <strong>in</strong>side<br />
the hadron must be filled with a strong field <strong>of</strong> quarkantiquark<br />
pairs, called the ‘chiral condensate’.<br />
The <strong>in</strong>teraction <strong>of</strong> the light quarks with this condensate<br />
breaks chiral symmetry spontaneously, and<br />
generates the large quark masses. Increas<strong>in</strong>g the temperature<br />
or baryon density <strong>of</strong> a system, for example<br />
through a high-energy nuclear collision, modifies the<br />
vacuum. The chiral condensate is diluted and chiral<br />
symmetry is partly restored, caus<strong>in</strong>g a modification<br />
(reduction) <strong>of</strong> the masses <strong>of</strong> hadrons. At very high<br />
density or temperature the spontaneous break<strong>in</strong>g <strong>of</strong><br />
the symmetry should completely disappear and the<br />
condensate should vanish. This transition may <strong>in</strong> fact<br />
co<strong>in</strong>cide with the deconf<strong>in</strong>ement transition. The search<br />
for signatures <strong>of</strong> chiral symmetry restoration is <strong>of</strong> fundamental<br />
importance <strong>in</strong> physics and one central objective<br />
<strong>of</strong> high-energy heavy ion collision experiments.<br />
<strong>Perspectives</strong> <strong>of</strong> <strong>Nuclear</strong> <strong>Physics</strong> <strong>in</strong> <strong>Europe</strong> – NuPECC Long Range Plan 2010 | 83