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Bulk viscosity of interacting magnetized strange quark matter

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Bulk viscosity for interacting strange quark matter and r-mode instability windows for strange stars

Jian-Feng Xu et al.

Summary: The study investigates the bulk viscosity of strange quark matter within the framework of the equivparticle model, showing a significant increase compared to scenarios utilizing the bag model. This increase is primarily due to the large quark equivalent masses in the equivparticle model, which are a result of strong interquark interactions and dynamical chiral symmetry breaking. The high bulk viscosity results in a shorter predicted damping time for oscillations in a canonical 1.4 solar mass strange star, with the r-mode instability window accommodating observational frequencies and temperatures for pulsars in low-mass X-ray binaries.

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