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期刊论文
Bulk viscosity of strange quark matter in density-dependent quark mass model and dissipation of r-modes in strange stars
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We study the bulk viscosity of strange quark matter (SQM) in density dependent quark mass model(DDQM) under the background of self-consistent thermodynamics. The correct formulae, with which the viscosity can be evaluated, are derived. We also find that the viscosity in DDQM can be higher by 2 to 3 orders of magnitude than MIT bag model. We calculate the damping time scales due to viscosity coupled to r-modes. The numerical results show the time scale can't be shorter than 10-1s.
【免责声明】以下全部内容由[郑小平]上传于[2009年03月20日 09时20分59秒],版权归原创者所有。本文仅代表作者本人观点,与本网站无关。本网站对文中陈述、观点判断保持中立,不对所包含内容的准确性、可靠性或完整性提供任何明示或暗示的保证。请读者仅作参考,并请自行承担全部责任。
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