The Equation of State of Neutron Star Matter

from to (Europe/Rome)
at Spazi Arte - Teatro Machiavelli
Piazza Università 13, Catania
Description

COMPSTAR WG2 meeting

Go to day
  • Tuesday, 7 November 2017
    • 09:00 - 09:30 Welcome and Registration 30'
    • 09:30 - 13:00 Structure and properties of the crust (chair: J. Margueron)
      • 09:30 N. CHAMEL: Latest developments in the modelling of neutron star crusts 1h0'
        Material: Slides pdf file
      • 10:30 A. FANTINA: Nuclear distribution in a Wigner-Seitz cell based model 30'
      • 11:00 COFFEE 30'
      • 11:30 X. VINAS: Crust-core transitions in neutron stars revisited 30'
        Material: Slides pdf file
      • 12:00 C. PROVIDENCIA: Crust-core transition of a neutron star 30'
        Material: Slides pdf file
      • 12:30 L. ZDUNIK: Accreted vs. catalyzed crust 30'
        Material: Slides pdf file
    • 13:00 - 14:30 LUNCH
    • 14:30 - 17:35 Transport and Cooling (chair: M. Fortin)
      • 14:30 A. SEDRAKIAN: Non-standard model cooling of neutron stars 1h0'
        Material: Slides pdf file
      • 15:30 A. RADUTA: On cooling of neutron stars with hyperons 30'
        Material: Slides pdf file
      • 16:00 COFFEE 30'
      • 16:30 U. LOMBARDO: Pairing in nuclear matter 30'
        Material: Slides pdf file
      • 17:00 S. STETINA: The photon in dense nuclear matter 30'
        Material: Slides pdf file
  • Wednesday, 8 November 2017
    • 09:00 - 13:00 EOS of the core (chair: A. Fantina)
      • 09:00 A. RIOS: EOS developments in the NewCompStar era 1h0'
        Material: Slides pdf file
      • 10:00 D. LOGOTETA: Cold and hot equation of state using microscopic interactions 30'
        Material: Slides pdf file
      • 10:30 J. MARGUERON: Predictions for neutron star properties based on an meta-modeling 30'
        Material: Slides pdf file
      • 11:00 COFFEE 30'
      • 11:30 M. FORTIN: Hyperons in neutron stars: radius and thermal evolution 30'
      • 12:00 F. PEDERIVA: Progress in the understanding of the role of hyperons in the inner core EOS 30'
        Material: Slides pdf file
      • 12:30 E. KOLOMEITSEV: Neutron star matter with hyperons, Deltas and charged rho-mesons 30'
        Material: Slides powerpoint file
    • 13:00 - 14:30 LUNCH
    • 14:30 - 18:30 EOS of the core (chair: C. Providencia)
      • 14:30 W. GUO: The high-density dependence of the symmetry energy 30'
        Material: Slides pdf file
      • 15:00 R. DE OLIVEIRA: Many-body forces in magnetic neutrons stars 30'
        Material: Slides pdf file
      • 15:30 COFFEE 30'
      • 16:00 M. BIGDELI: Magnetized neutron matter 30'
        Material: Slides pdf file
      • 16:30 G. BARNAFOLDI: Modification of compact star observables due to quantum fluctuations 30'
        Material: Slides pdf file
      • 17:00 P. FIZIEV: EOS and compact stars in minimal dilatonic gravity 30'
        Material: Slides pdf file
      • 17:30 A. BONANNO: Asymptotically safe neutron stars 30'
        Material: Slides pdf file
    • 20:00 - 00:00 DINNER
  • Thursday, 9 November 2017
    • 09:00 - 11:20 Quark Matter (chair: A. Rios)
      • 09:00 I. BOMBACI: Quark matter in neutron stars 40'
      • 09:40 M. MANNARELLI: Quark matter and color superconductivity 40'
        Material: Slides pdf file
      • 10:20 D. ZAPPALA': Hybrid star structure from the field correlator method 30'
        Material: Slides pdf file
      • 10:50 A. DRAGO: What can we learn from neutron star mergers ? 30'
    • 11:20 - 11:50 COFFEE
    • 11:50 - 12:50 P. PIZZOCHERO: Concluding Remarks and Discussion 1h0'
      Material: Slides pdf file