128 research outputs found

    Sea-quark flavor asymmetry in the nucleon from a relativistic analysis of the Drell-Yan scattering off nuclei

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    It is shown that accounting for the relativistic structure of the deuteron allows to explain the ratio of the Drell-Yan pair production cross-section at the low Bjorken xx off the deuteron and the proton. Thus, the sea quark distributions in the nucleon should be studied with accounting for the effects of the relativistic structure of the deuteron. The suggested approach reduces theoretical uncertainty in extracting the ratio uˉ/dˉ\bar u/\bar d from the data and it is important for the clarification of the nature of the sea quark asymmetry in the nucleon.Comment: 4 pages, 1 figures, Chiral Symmetry in Hadron and Nuclear Physics November 13-16, 2007, Osak

    Observation of deconfinement in a cold dense quark medium

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    In this paper we study the confinement/deconfinement transition in lattice SU(2)SU(2) QCD at finite quark density and zero temperature. The simulations are performed on an 32432^4 lattice with rooted staggered fermions at a lattice spacing a=0.044 fma = 0.044 \mathrm{~fm}. This small lattice spacing allowed us to reach very large baryon density (up to quark chemical potential μq>2000 MeV\mu_q > 2000 \mathrm{~MeV}) avoiding strong lattice artifacts. In the region μq∼1000 MeV\mu_q\sim 1000 \mathrm{~MeV} we observe for the first time the confinement/deconfinement transition which manifests itself in rising of the Polyakov loop and vanishing of the string tension σ\sigma. After the deconfinement is achieved at μq>1000 MeV\mu_q > 1000 \mathrm{~MeV}, we observe a monotonous decrease of the spatial string tension σs\sigma_s which ends up with σs\sigma_s vanishing at μq>2000 MeV\mu_q > 2000 \mathrm{~MeV}. From this observation we draw the conclusion that the confinement/deconfinement transition at finite density and zero temperature is quite different from that at finite temperature and zero density. Our results indicate that in very dense matter the quark-gluon plasma is in essence a weakly interacting gas of quarks and gluons without a magnetic screening mass in the system, sharply different from a quark-gluon plasma at large temperature.Comment: 6 pages, 4 figure

    Lattice QCD thermodynamics at finite chemical potential and its comparison with Experiments

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    We compare higher moments of baryon numbers measured at the RHIC heavy ion collision experiments with those by the lattice QCD calculations. We employ the canonical approach, in which we can access the real chemical potential regions avoiding the sign problem. In the lattice QCD simulations, we study several fits of the number density in the pure imaginary chemical potential, and analyze how these fits affects behaviors at the real chemical potential. In the energy regions between sNN\sqrt{s}_{NN}=19.6 and 200 GeV, the susceptibility calculated at T/Tc=0.93T/T_c=0.93 is consistent with experimental data at 0≤μB/T<1.50 \le \mu_B/T < 1.5, while the kurtosis shows similar behavior with that of the experimental data in the small μB/T\mu_B/T regions 0≤μB/T<0.30 \le \mu_B/T < 0.3. The experimental data at sNN=\sqrt{s}_{NN}= 11.5 shows quite different behavior. The lattice result in the deconfinement region,T/Tc=1.35T/T_c=1.35, is far from experimental data

    Temperature dependence of the axial magnetic effect in two-color quenched QCD

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    The Axial Magnetic Effect is the generation of an equilibrium dissipationless energy flow of chiral fermions in the direction of the axial (chiral) magnetic field. At finite temperature the dissipationless energy transfer may be realized in the absence of any chemical potentials. We numerically study the temperature behavior of the Axial Magnetic Effect in quenched SU(2) lattice gauge theory. We show that in the confinement (hadron) phase the effect is absent. In the deconfinement transition region the conductivity quickly increases, reaching the asymptotic T2T^2 behavior in a deep deconfinement (plasma) phase. Apart from an overall proportionality factor, our results qualitatively agree with theoretical predictions for the behavior of the energy flow as a function of temperature and strength of the axial magnetic field.Comment: 5 pages, 1 figur
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