13–19 May 2018
Venice, Italy
Europe/Zurich timezone
The organisers warmly thank all participants for such a lively QM2018! See you in China in 2019!

Session

QCD at high temperature

15 May 2018, 09:00
Sala Volpi, 1st Floor (Palazzo del Casinò)

Sala Volpi, 1st Floor

Palazzo del Casinò

Conveners

QCD at high temperature: I

  • Chihiro Sasaki

QCD at high temperature: II

  • Massimo D'Elia (University of Pisa)

Presentation materials

There are no materials yet.

  1. Alexei Bazavov (Michigan State University)
    15/05/2018, 09:00
    QCD at high temperature
    Parallel Talk

    The equation of state (EoS) in $2+1$ flavor QCD has recently been established in the continuum limit at the physical quark masses in ab initio lattice QCD calculations. The HotQCD collaboration result provides the EoS in the temperature range from $130$ to $400$ MeV. We extend the HotQCD equation of state to higher temperatures. We utilize the Highly Improved Staggered Quarks (HISQ) action. We...

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  2. Christian Rohrhofer (Karl-Franzens Universität Graz)
    15/05/2018, 09:20
    QCD at high temperature
    Parallel Talk

    We study spatial isovector meson correlators in $n_f=2$ QCD with dynamical domain-wall fermions on $32^3\times 8$ lattices at temperatures $T=220-380$ MeV. We measure the correlators of all spin-one ($J=1$) isovector operators. We observe an approximate degeneracy of all considered correlators with increasing temperature. This approximate degeneracy suggests emergent $SU(2)_{CS}$ and...

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  3. Anirban Lahiri (Bielefeld University)
    15/05/2018, 09:40
    QCD at high temperature
    Parallel Talk

    Understanding the properties of strong interaction matter with its physical
    spectrum of light and strange quarks near the pseudo-critical temperature
    of (2+1)-flavor QCD is one of the central goals of high energy nuclear
    physics. It generally is expected that the analytic crossover transition in
    QCD is sensitive to properties of the true chiral PHASE transition at
    vanishing quark masses [1,2]....

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  4. Jacopo Ghiglieri (CERN)
    15/05/2018, 10:00
    QCD at high temperature
    Parallel Talk

    In this talk we will study the relaxation coefficients $\tau_\pi$ and $\tau_J$ of the shear stress tensor $\pi^{\mu\nu}$ and the light quark current $J$ respectively. These are second-order transport coefficients which can be determined in perturbation theory. After reviewing the perturbative kinetic theory framework that has been recently used to determine their respective first-order...

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  5. Shuai Liu (Texas A&M University)
    15/05/2018, 10:20
    QCD at high temperature
    Parallel Talk

    Understanding the microscopic properties of the hot and dense QCD matter produced at RHIC and the LHC is a critical task for heavy-ion physics. Toward this end, we have developed a non-perturbative microscopic approach to study the bulk, transport and spectral properties of the quark-gluon plasma (QGP) [1-2], treating light, heavy and static partons in a unified framework. Starting from a...

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  6. Chihiro Sasaki
    16/05/2018, 11:10
    QCD at high temperature
    Parallel Talk

    Motivated by the recent lattice study by the FASTSUM collaboration [1],
    thermal masses of the baryon parity-doublers are explored for
    various pion masses [2]. A general trend of the octet and decuplet
    parity-doublers is consistent to the results in [1], whereas their
    hyperon masses are modified to a large extent for the physical pion mass.

    We further investigate the fluctuations and...

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  7. Chris Allton (Swansea University)
    16/05/2018, 11:30
    QCD at high temperature
    Parallel Talk

    The behaviour of strange baryons in the hadronic gas and the quark-gluon plasma gives essential insight into chiral symmetry restoration and parity doubling, and has direct consequences for phenomenology, e.g. via the hadron resonance gas. We present results obtained using nonperturbative lattice simulations, employing the FASTSUM anisotropic Nf=2+1 ensembles.

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  8. Szabolcs Borsanyi (University of Wuppertal)
    16/05/2018, 11:50
    QCD at high temperature
    Parallel Talk

    A new precision lattice simulation set is analyzed for the equation of state
    to sixth order. We discuss the role of strangeness neturality and the
    range of validity of the extrapolation strategy. We calculate the pressure,
    trace anomaly, energy and entropy densitiy and the baryon number in the range
    up to mu/T < 2. We achieve improved precision by combining the technique of
    analitcal...

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  9. Mauricio Martinez Guerrero (North Caroline State University)
    16/05/2018, 12:10
    QCD at high temperature
    Parallel Talk

    In this work we discuss the phenomenological applications of non-equilibrium hydrodynamical attractors to transport phenomena in fluid dynamics. We study the late-time behaviour of a relativistic fluid undergoing Bjorken flow whose microscopic description is given in terms of the Boltzmann equation with a time-dependent relaxation time. The mathematical problem of solving the Boltzmann...

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  10. Prof. Kenji Fukushima (The University of Tokyo)
    16/05/2018, 12:30
    QCD at high temperature
    Parallel Talk

    This talk is based on 1711.01472 in which the longitudinal electric conductivity of hot and dense magnetized quark matter has been computed with full Landau level resummation which requires several nontrivial theoretical techniques. In contrast to the lowest Landau level approximation, there is no singularity in the massless limit, and we find that the resultant electric conductivity is...

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  11. Prof. Bikash Sinha (Variable Energy Cyclotron Centre)
    16/05/2018, 12:50
    QCD at high temperature
    Parallel Talk

    There are at least three sources of cosmic quarks in the universe. One, the quark
    nuggets which may survive beyond a certain baryon number during the phase
    transition from quarks to hadrons microseconds after the big bang. These quark
    nuggets can very well be candidate of cold dark matter and these nuggets consist of
    strange quarks.
    Second, the interior of the neutron star may well be made of...

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