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

## TL;DR

This paper reviews the impact of strong magnetic fields on the structure and properties of hybrid stars, emphasizing the importance of self-consistent solutions over symmetric approximations in modeling magnetized neutron stars.

## Contribution

It highlights the necessity of self-consistent modeling for magnetic fields in hybrid stars and discusses their effects on stellar population and temperature profiles.

## Key findings

- Magnetic fields significantly influence hybrid star structure.
- Symmetric solutions are inadequate for modeling magnetized neutron stars.
- Magnetic effects alter temperature profiles and stellar populations.

## 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.