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EMMI workshop: Neutron Matter in Astrophysics: From Neutron Stars to the r-Process

Jul 15 – 18, 2010
GSI
Europe/Berlin timezone

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Session

Session 7: Neutron stars, properties and EoS II

Jul 17, 2010, 9:00 AM
GSI

GSI

Planckstr. 1 64291 Darmstadt

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  1. 4. Modeling Hybrid Stars
    Prof. Verônica Dexheimer (Gettysburg College)
    7/17/10, 9:00 AM
    We extend the hadronic SU(3) non-linear sigma model to include quark degrees of freedom. The choice of potential for the deconfinement order parameter as a function of temperature and chemical potential allows us to construct a realistic phase diagram from the analysis of the order parameters of the system. These parameters are the chiral condensate, for the chiral symmetry restoration, and...
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  2. 16. High density behavior of the nuclear EoS and properties of massive neutron stars
    Dr Partha Roy Chowdhury (Department of Physics, University of Calcutta)
    7/17/10, 9:30 AM
    Modern constraints from the mass and mass-radius-relation measurements require stiff EoS at high densities, whereas flow data from heavy-ion collisions seem to disfavour too stiff behavior of the EoS. Our aim is to present a nuclear EoS at supernuclear densities which satisfies both the constraints from neutron star (NS) and the heavy ion collision phenomenology. The data from massive NSs and...
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  3. 10. Neutron star matter
    Dr David Blaschke
    7/17/10, 10:00 AM
    Replaced by D. Blaschke
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