# Hot magnetized nuclear matter: Thermodynamic and Saturation Properties

**Authors:** Z. Rezaei, G. H. Bordbar

arXiv: 1702.04765 · 2017-03-02

## TL;DR

This paper investigates how magnetic fields and temperature influence the thermodynamic and saturation properties of nuclear matter using a realistic potential and variational approach, revealing effects on phase transitions and critical points.

## Contribution

It introduces a detailed analysis of hot magnetized nuclear matter's properties using AV18 potential and LOCV method, focusing on magnetic field effects on saturation and phase transition behaviors.

## Key findings

- Magnetic field decreases the flashing temperature of nuclear matter.
- Magnetic field influences the liquid-gas phase transition and critical point properties.
- Equation of state varies with temperature and magnetic field.

## Abstract

We have used a realistic nuclear potential, AV18, and a many body technique, the lowest order constraint variational (LOCV) approach, to calculate the properties of hot magnetized nuclear matter. By investigating the free energy, spin polarization parameter, and symmetry energy, we have studied the temperature and magnetic field dependence of the saturation properties of magnetized nuclear matter. In addition, we have calculated the equation of state of magnetized nuclear matter at different temperatures and magnetic fields. It was found that the flashing temperature of nuclear matter decreases by increasing the magnetic field. In addition, we have studied the effect of the magnetic field on liquid gas phase transition of nuclear matter. The liquid gas coexistence curves, the order parameter of the liquid gas phase transition, and the properties of critical point at different magnetic fields have been calculated.

## Full text

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## Figures

13 figures with captions in the complete paper: https://tomesphere.com/paper/1702.04765/full.md

## References

58 references — full list in the complete paper: https://tomesphere.com/paper/1702.04765/full.md

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Source: https://tomesphere.com/paper/1702.04765