Fine structure on the surface of bare strange stars

Details Fine structure on the surface of bare strange stars Fine structure on the surface of bare strange stars

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap.....48..111h&link_type=abstract

Astrophysics, Volume 48, Issue 1, pp.111-121

Astronomy and Astrophysics

Astrophysics

Stars, Quark Matter, Surface Tension, Stars - Quark Matter - Surface Tension

Scientific paper

The surface fine structure of bare strange stars is determined. The distribution of electrons and quarks in the surface layer is determined using a phenomenological Thomas-Fermi model. For the MIT bag model, the quark density at the free surface is found to fall off continuously to zero in a layer of finite thickness. Unlike the results of other authors, here the electric field in the transition layer changes direction. The coefficient of surface tension of the quark matter is determined in terms of this model. Depending on the model parameters, it is 60-150 MeV/Fm2.

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