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Abstract:
Bulk viscosity of interacting strange quark matter is calculated in the light of ms dependent reaction rate of u+s←→d+u, and the extra terms come from the interaction between quarks and theomodynamic consistency are included. We find that the results were larger than previously assumed. The application to the damping time of the interacting strange quark matter shows that although the bulk viscosity becomes larger, the previous conclusion about the observation of the existence of strange stars is unchanged.
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[1] |
Guo Hua
. In-medium QMC Model Parameters and Quark Condensation in Nuclear Matter. Chinese Physics C,
1999, 23(5): 459-468. |
[2] |
Chen Zhongqiu
, Shao Changgui
, Ma Weichuan
. Calculation of Wilson Loop Functionals for Classical and Quantum Gravities. Chinese Physics C,
1998, 22(3): 217-224. |
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