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arXiv · 0708.3317

On surface tension for compact stars

R. Sharma·S. D. Maharaj
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Abstract

In an earlier treatment it was demonstrated that general relativity gives higher values of surface tension in strange stars with quark matter than neutron stars.We generate the modified Tolman-Oppenheimer-Volkoff equation to incorporate anisotropic matter and use this to show that pressure anisotropy provides for a wide range of behaviour in the surface tension than is the case with isotropic pressures. In particular it is possible that anisotropy drastically decreases the value of the surface tension.

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R. Sharma, S. D. Maharaj. 2007-08-24. On surface tension for compact stars. https://doi.org/10.1007/s12036-007-0010-x

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