Subnuclear matter in neutron stars and supernovae: nuclear pasta and beyond

Details Subnuclear matter in neutron stars and supernovae: nuclear pasta and beyond Subnuclear matter in neutron stars and supernovae: nuclear pasta and beyond

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ragt.meet..119n&link_type=abstract

In Proceedings of RAGtime 6/7: Workshops on black holes and neutron stars, Opava, 16-18/18-20 September, 2004/2005; S. Hledík an

Astronomy and Astrophysics

Astrophysics

Scientific paper

We review the current status of models of matter at subnuclear density as it appears in astrophysical contexts; namely, during core collapse of supernovae and in the inner crusts of neutron stars. We discuss the main observational probes of this regime, and present preliminary results of our own studies of the so-called nuclear pasta that appears in this density regime.

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