On the Electrodynamical Properties of Nuclear Matter in Bulk

Details On the Electrodynamical Properties of Nuclear Matter in Bulk On the Electrodynamical Properties of Nuclear Matter in Bulk

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..966..147r&link_type=abstract

RELATIVISTIC ASTROPHYSICS: 4th Italian-Sino Workshop. AIP Conference Proceedings, Volume 966, pp. 147-152 (2008).

Astronomy and Astrophysics

Astrophysics

1

Nuclear Matter Aspects Of Neutron Stars, Degenerate Fermi Gases, Statistical Model Calculations, Nuclear Matter

Scientific paper

We analyze the properties of solutions of the relativistic Thomas-Fermi equation for globally neutral cores with radius of the order of R~10 Km, at constant densities around the nuclear density. By using numerical tecniques as well as well tested analytic procedures developed in the study of heavy ions, we confirm the existence of an electric field close to the critical value Ec = me2c3/eℏ in a shell ΔR~l04ℏ/mπc near the core surface. For a core of ~10 Km the difference in binding energy reaches 1049 ergs. These results can be of interest for the understanding of very heavy nuclei as well as physics of neutron stars, their formation processes and further gravitational collapse to a black hole.

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