On color confinement
On color confinement
复制标题
关于色彩的限制
DOI:
10.29172/87ca58a8a3164438a43036d3d0a0f6b6
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发表时间:
2006
期刊:
影响因子:
--
通讯作者:
A. Giacomo
中科院分区:
文献类型:
--
作者:
A. Giacomo
Quarks can be detected by use of electroweak probes at short distances. They have never been observed as free particles. The experimental upper limits to the existence of free quarks can be found in Particle Data Group reports[1]. The upper limit to the ratio of the quark abundance in nature nq to that of the nucleons np is nq np ≤ 10 to be compared with the expected value in the Standard Cosmological Model 10. The inclusive cross section σp to produce a quark or an antiquark has upper limit 10cm to be compared with the value expected in the absence of confinement ≈ 10cm. A suppression factor of 10 can only have as a natural explanation that nq = 0 and σq = 0 due to some symmetry. This phenomenon is called color confinement : asymptotic particle in QCD are only colorless. The obvious question is then: does QCD imply color confinement, and, if so, by what mechanism? What is the symmetry which produces confinement? For the first time it was conjectured in ref[2] that the Hagedorn limiting temperature [3] could in fact correspond to a deconfining phase transition from hadrons to a gas of quarks and gluons (the so called Quark Gluon Plasma). Experiments colliding heavy ions have been set up at CERN and at Brookhaven to detect such transition. It is not clear what would be the smoking-gun signal for that transition and no clear statement can be done up to now. Virtual experiments, i.e. numerical simulations of the theory on the lattice have instead demonstrated the existence of a deconfining transition. Lattice Montecarlo techniques produce a discretized approximant to the functional Feynman integral which defines QCD . If the lattice spacing a is small compared to hadronic scale λ and λ is in turn much smaller than the lattice size La the numerical estimate can be a good approximation to the functional integral. Also QCD at finite temperature can be simulated by similar techniques. The partition function Tr[e H T ] is equal to the Feynman integral compactified from 0 to 1 T in the time direction, with periodic boundary conditions in time for bosonic fields, antiperiodic for fermions. In formulae