作者: V. V. Usov , K. S. Cheng , T. Harko
DOI: 10.1086/427074
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摘要: We consider a thin (~102-103 fm) layer of electrons (the electrosphere) at the quark surface bare strange star, taking into account effects boundary with vacuum. The holds electron by an extremely strong electric field, generated in electrosphere to prevent from escaping infinity counterbalancing degeneracy and thermal pressure. Because tension depletion s quarks very (a few charged forms star. formation this modifies structure significantly changing field density electrons, comparison case which are ignored. Some consequences modification on properties stars briefly discussed.