A New Study of the Transition to Uniform Nuclear Matter in Neutron Stars and Supernovae

Details A New Study of the Transition to Uniform Nuclear Matter in Neutron Stars and Supernovae A New Study of the Transition to Uniform Nuclear Matter in Neutron Stars and Supernovae

2007-08-23

arxiv.org/abs/0708.3212v1

Phys.Part.Nucl.39:1173-1175,2008

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures. Participant Contribution at the ``Dense Matter in Heavy Ion Collisions and Astrophysics" Summer School, JI

Scientific paper

10.1134/S1063779608070356

A comprehensive microscopic study of the properties of bulk matter at densities just below nuclear saturation $\rho_s = 2.5 \sim 10^{14}$ g cm$^{-3}$, zero and finite temperature and high neutron fraction, is outlined, and preliminary results presented. Such matter is expected to exist in the inner crust of neutron stars and during the core collapse of massive stars with $M \gtrsim 8M_{\odot}

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