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The Structure and Signals of Neutron Stars, from Birth to Death

24–28 Mar 2014
Europe/Rome timezone

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Session

Plenary session 1

24 Mar 2014, 09:00

Conveners

Plenary session 1

  • Constança Providência (University of Coimbra)

Presentation materials

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  1. 124. The Equation of State of Neutron Star Matter
    Dr Hans-Josef Schulze (INFN Sezione di Catania)
    24/03/2014, 09:10
    The main features of the EOS of neutron star matter are reviewed, comprising nucleonic, hyperonic, and quark matter contributions. The focus in on the Brueckner-Hartree-Fock theoretical method, but also other approaches will be regarded.
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  2. 136. Constraints on the Equation of State of Nuclear Matter from Heavy-Ion Collisions and from Structure
    Prof. Pawel Danielewicz (East Lansing, MSU (USA))
    24/03/2014, 09:50
    Constraints on the nuclear equation of state, following from heavy ion collisions and from structure, are reviewed. The collisions produce matter transiently reaching densities few times the normal. Isolating observables testing such densities is challenging, though, and interpretation of those observables suffers from theoretical uncertainities. Structure observables can be generally...
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  3. 130. Strangeness in Compact Stars
    Dr Juergen Schaffner-Bielich (Institut fuer Theoretische Physik, Goethe Universitaet, Frankfurt)
    24/03/2014, 10:30
    In the dense interior of compact stars the composition might change considerably. Due to weak equilibrium in neutron star matter particles carrying strangeness can appear changing the overall global properties as well as the transport properties of compact stars. The new pulsar mass limit of two solar masses gives new information on the presence of strange matter in the core of compact...
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