Warm nuclear and neutron star matter and the pasta phase

Details Warm nuclear and neutron star matter and the pasta phase Warm nuclear and neutron star matter and the pasta phase

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1296..207a&link_type=abstract

XI HADRON PHYSICS. AIP Conference Proceedings, Volume 1296, pp. 207-212 (2010).

Physics

Neutron Stars, Antiferromagnetic Materials, Thermal Conductivity, Surface Energy, Neutron Stars, Antiferromagnetics, Electrical And Thermal Conduction In Crystalline Metals And Alloys, Surface Thermodynamics, Surface Energies

Scientific paper

The possibility of exotic structures, i. e., the ``pasta'' phase to be
formed in the low density region of nuclear and stellar matter is
investigated. The effects of the presence of α-particles are
considered in the context of relativistic nuclear models.

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