Anisotropic pressure in strange quark matter in the presence of a strong magnetic field

被引:50
作者
Isayev, A. A. [1 ,2 ]
Yang, J. [3 ,4 ]
机构
[1] Kharkov Phys & Technol Inst, UA-61108 Kharkov, Ukraine
[2] Kharkov Natl Univ, UA-61022 Kharkov, Ukraine
[3] Ewha Womans Univ, Dept Phys, Seoul 120750, South Korea
[4] Ewha Womans Univ, Inst Early Universe, Seoul 120750, South Korea
关键词
NEUTRON MATTER; MODEL; STAR; RAY;
D O I
10.1088/0954-3899/40/3/035105
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
The thermodynamic properties of strange quark matter in strong magnetic fields H up to 10(20) G are considered within the MIT bag model at zero temperature implying the constraints of total baryon number conservation, charge neutrality and chemical equilibrium. The pressure anisotropy, exhibited in the difference between the pressures along and perpendicular to the field direction, becomes essential at H > H-th, with the estimate 10(17) < H-th less than or similar to 10(18) G. The longitudinal pressure vanishes at the critical field H-c, which can be somewhat smaller or larger than 10(18) G depending on the total baryon number density and bag pressure. As a result, longitudinal instability occurs in strange quark matter, which precludes: (1) a significant drop in the content of s quarks, which, otherwise could happen at H similar to 10(20) G; (2) the appearance of positrons in weak processes in a narrow interval near H similar to 2 x 10(19) G (replacing electrons). The occurrence of the longitudinal instability leaves the possibility only for electrons to reach a fully polarized state, while for all quark flavors the polarization remains mild even for fields near H-c. The anisotropic equation of state is determined under the conditions relevant to the interiors of magnetars.
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页数:16
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