Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006a%26a...445..627z&link_type=abstract
Astronomy and Astrophysics, Volume 445, Issue 2, January II 2006, pp.627-631
Astronomy and Astrophysics
Astrophysics
8
Dense Matter, Stars: Neutron, Stars: Magnetic Fields
Scientific paper
We made a detailed study of the properties of the electron layer near the quark surface of strange stars with strong (˜1014{-}1017 G) magnetic fields. The electrostatic potential and the electric field at the quark surface were calculated as functions of the magnetic field intensity of bare strange stars. Using an ultrastrong (B≥ 2.5×1016 G) magnetic field, we found that the distribution of electrons becomes an exponential function of radial distance, which is quite different in a magnetic field-free case. We also calculated the variation in gap width between the strange core and the normal nuclear crust for strange stars, which is due to magnetic field effect.
Yu Yun-Wei
Zheng Xiao-Ping
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