Quark Deconfinement Under the Influence of Strong Magnetic Fields

Details Quark Deconfinement Under the Influence of Strong Magnetic Fields Quark Deconfinement Under the Influence of Strong Magnetic Fields

2011-08-23

arxiv.org/abs/1108.4479v2

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

Revised version with updated references

Scientific paper

We study the effect of high magnetic fields on the particle population of neutron stars using an extended hadronic and quark SU(3) non-linear realization of the sigma model. In this model the degrees of freedom change naturally from hadrons to quarks as the density and/or temperature increases. The effects of high magnetic fields and anomalous magnetic moment (AMM) are visible in the macroscopic properties of the star, such as mass, adiabatic index, moment of inertia, and cooling curves.

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