Spinodal instabilities and the distillation effect in nuclear matter under strong magnetic fields
arXiv:0810.3395 · doi:10.1103/PhysRevC.79.015804
Abstract
We study the effect of strong magnetic fields, of the order of - G, on the instability region of nuclear matter at subsaturation densities. Relativistic nuclear models both with constant couplings and with density dependent parameters are considered. It is shown that a strong magnetic field can have large effects on the instability regions giving rise to bands of instability and wider unstable regions. As a consequence we predict larger transition densities at the inner edge of the crust of compact stars with strong magnetic field. The direction of instability gives rise to a very strong distillation effect if the last Landau level is only partially filled. However, for almost completed Landau levels an anti-distillation effect may occur.
16 pages, 13 figures, 3 tables, revised version submitted to Phys. Rev. C
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- Neutron matter under strong magnetic fields: a comparison of models
- Strong magnetic fields and pasta phases revisited
- Crust-core transition of a neutron star: effect of the temperature under strong magnetic fields
- Pasta phases in neutron stars under strong magnetic fields
- Stability of the neutron-proton-electron matter under strong magnetic fields: the covariant Vlasov approach
- Coexistence of phases in asymmetric nuclear matter under strong magnetic fields
- Vacuum effects on the properties of nuclear matter under an external magnetic field
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- Spinodal instabilities of spin polarized asymmetric nuclear matter