On surface tension for compact stars

Details On surface tension for compact stars On surface tension for compact stars

2007-08-24

arxiv.org/abs/0708.3317v1

J. Astrophys. Astron. 28 (2007) 133-138

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8 pages, To appear in J. Astrophys. Astron

Scientific paper

10.1007/s12036-007-0010-x

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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