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EMMI Rapid Reaction Task Force: Quark Matter in Compact Stars

→ Europe/Berlin
FIAS Frankfurt

FIAS Frankfurt

Ruth-Moufang-Str.1 60438 Frankfurt am Main
Jürgen Schaffner-Bielich (Frankfurt University), Stefan Schramm (FIAS Frankfurt)
Poster
Program
  • Mo., 7. Oktober
    • 09:30 → 09:45
      Registration 15m
    • 09:45 → 10:00
      Presentation of EMMI 15m
      Sprecher: Ewerz
    • 10:00 → 11:00
      Overview: Signals of quark matter in compact stars 1 h
      Sprecher: Weber
      Slides
    • 11:00 → 12:00
      Overview: Recent estimates of neutron star masses and radii and limits on properties of quark matter EoSA 1 h
      Sprecher: Lattimer
      Slides
    • 12:00 → 14:00
      lunch 2h
    • 14:00 → 18:00
      Signals and constraints
      Sitzungsleiter: Haensel
      • 14:00
        Masses of black widow pulsars: whiy high values should not be a surprise 30m
        Sprecher: Horvath
        Slides
      • 14:30
        Signals of quark matter in core-collapse supernovae 30m
        Sprecher: Sagert
        Slides
      • 15:00
        coffee 30m
      • 15:30
        Quark matter in compact stars: Indications from x-ray and radio pulsars 30m
        Sprecher: Schwenzer
        Slides
      • 16:00
        Quark matter and cooling of compact stars 30m
        Sprecher: Negreios
        Slides
      • 16:30
        discussions 1 h 30m
  • Di., 8. Oktober
    • 09:00 → 12:00
      Quark matter
      Sitzungsleiter: Fraga
      • 09:00
        Recent advances in perturbative QCD at finite temperature and density 30m
        Sprecher: Vuorinen
        Slides
      • 09:30
        Compact-star matter from NJL models and QCD 30m
        Sprecher: Buballa
        Slides
      • 10:00
        Superlfuid propertis of quark matter 30m
        Sprecher: Schmitt
        Slides
      • 10:30
        coffee 30m
      • 11:00
        Quark matter subjects to strong magnetic fields 30m
        Sprecher: Menezes
        Slides
      • 11:30
        Inhomogeneous chiral phases in the QCD phase diagram and implications on compact stars 30m
        Sprecher: Tatsumi
        Slides
    • 12:00 → 14:00
      lunch 2h
    • 14:00 → 18:00
      Hybrid stars
      Sitzungsleiter: Schramm
      • 14:00
        Are quarks not hadron-confined in compact stars? 30m
        Sprecher: Xu
        Slides
      • 14:30
        Massive stars within self-consistent approaches 30m
        Sprecher: Dexheimer
        Slides
      • 15:00
        coffee 30m
      • 15:30
        NJL hybrid stars and the recent 2M_sun pulsars 30m
        Sprecher: Lugones
        Slides
      • 16:00
        Hadron-quark mixed phase with geometrical structure and equation of state 30m
        Sprecher: Maruyama
        Slides
      • 16:30
        discussions 1 h 30m
  • Mi., 9. Oktober
    • 09:00 → 12:00
      Phase transition in compact stars
      Sitzungsleiter: Mishustin
      • 09:00
        Conversion of neutron stars into quark stars 30m
        Sprecher: Pagliara
        Slides
      • 09:30
        Formation of hybrid stars from metastable hadronic stars 30m
        Sprecher: Providencia
        Slides
      • 10:00
        Radial oscillations in compact stars 30m
        Sprecher: Brillante
        Slides
      • 10:30
        coffee 30m
      • 11:00
        Can very compact and very masstive neutron stars both exist? 30m
        Sprecher: Drago
        Slides
      • 11:30
        Rapid cooling of Cas A as a phase transition in dense QCD 30m
        Sprecher: Sedrakian
        Slides
    • 12:00 → 14:00
      Lunch 2h
    • 14:00 → 18:00
      Failed attempts
      Sitzungsleiter: Buballa
      • 14:00
        Investigation of the existence of hybrid stars using NJL models 30m
        Sprecher: Malheiro
        Slides
      • 14:30
        Maximum mass of hybrid stars and microscopic stability of strange cores 30m
        Sprecher: Zdunik
        Slides
      • 15:00
        coffee 30m
      • 15:30
        Mass-radius constraints for compact stars and the QCD phase diagram 30m
        Sprecher: Blaschke
        Slides
      • 16:00
        Strange Cores and Neutron Star Radii 30m
        Sprecher: Haensel
        Slides
      • 16:30
        discussions 1 h 30m
  • Do., 10. Oktober
    • 10:00 → 11:00
      Initial preparation of the task force report
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