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arXiv · 1702.00386

A self-consistent study of magnetic field effects on hybrid stars

V. Dexheimer·B. Franzon·S. Schramm
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Abstract

It is understood that strong magnetic fields affect the structure of neutron stars. Nevertheless, many calculations for magnetized neutron stars are still being performed using symmetric solutions of Einstein's equations. In this conference proceeding, we review why this is not the correct procedure and we also discuss the effects of magnetic fields on the stellar population and temperature profiles.

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V. Dexheimer, B. Franzon, S. Schramm. 2017-02-01. A self-consistent study of magnetic field effects on hybrid stars. https://doi.org/10.1088/1742-6596/861/1/012012

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