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Critical Point and Onset of Deconfinement 2016

30 May 2016 to 4 June 2016
University of Wrocław
Europe/Warsaw timezone

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Session

COST Action MP1304 "NewCompStar" WG2 Meeting

31 May 2016, 14:00
Oratorium Marianum (University of Wrocław)

Oratorium Marianum

University of Wrocław

Main Building, plac Uniwersytecki 1

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  1. 38. Recent Results on Equation of States from NewCompStar
    Gergely Barnafoldi (Wigner RCP Hungarian Academy of Sciences)
    31/05/2016, 14:00
    Talk

    A biref summary on the recent result on compact star equation of state will be presented. I summarize the directions and activities of the NewCompStar working group on the physics of the strong interaction in cold dense nuclear and QCD medium exists in compact stars.

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  2. 108. Quark matter in neutron stars
    Gordon Baym (University of Illinois)
    31/05/2016, 14:30
    Talk

    This talk will describe the continuing development of a consistent
    picture of the liquid interiors of neutron stars, driven by three
    recent advances: observations of heavy neutron stars with masses ~2.0
    solar masses; determinations of masses and radii simultaneously for an
    increasing number of neutron stars; and an emerging understanding in
    QCD of how nuclear matter can turn into deconfined...

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  3. 118. QCD in stars
    Toru Kojo (University of Illinois, Urbana-Champaign)
    31/05/2016, 15:00
    Talk

    We delineate properties of cold, dense QCD matter through equations of state supposed from observational constraints on neutron stars.

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  4. 71. Inhomogeneous chiral condensates in the QCD phase diagram
    Michael Buballa (T)
    31/05/2016, 16:00
    Talk
  5. 72. Consequences of simultaneous chiral symmetry restoration and deconfinement for the QCD phase diagram
    Thomas Klaehn (University of Wroclaw)
    31/05/2016, 16:30
    Talk
  6. 25. Bayesian analysis of new class of realistic hybrid EoS models based on M-R data
    Alexander Ayriyan (JINR)
    31/05/2016, 17:00
    Talk

    We performed a Bayesian analysis of a new class realistic models of two-phase equations of state (EoS) for hybrid stars and demonstrated that the observation of such a pair of high-mass twin stars would have a sufficient discriminating power to favor hybrid EoS with a strong first order phase transition over alternative EoS.
    The new class of two-phase EoS is characterized by three main...

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  7. 73. Cooling of neutron stars with stiff stellar matter
    Hovik Grigorian (Joint Institute for Nuclear Research)
    31/05/2016, 17:30
    Talk
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