The pasta structure in the hadron-quark phase transition and the effects on magnetized compact stars

Details The pasta structure in the hadron-quark phase transition and the effects on magnetized compact stars The pasta structure in the hadron-quark phase transition and the effects on magnetized compact stars

2009-11-20

arxiv.org/abs/0911.3968v2

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

7 pages, 3 figures, Compact stars in the QCD phase diagram II

Scientific paper

We report the effects of quark-hadron phase transition on the structures of general relativistic stars with purely toroidal magnetic field. For the mixed phase, we take into account of the finite-size effects, which lead to non-uniform "Pasta" structures. Our study is based on axisymetric and stationary formalism including purely toroidal magnetic field. For hybrid stars, we find the characteristic distribution of magnetic field, which has a discontinuity originated in the quark-hadron mixed phase. These distributions of magnetic field will change astrophysical phenomena, such as cooling processes.

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