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arxiv: 1512.06993 · v1 · pith:HIBIFLUPnew · submitted 2015-12-22 · ⚛️ nucl-th · astro-ph.SR

Calculation of nuclear matter in the presence of strong magnetic field using LOCV technique

classification ⚛️ nucl-th astro-ph.SR
keywords magneticenergyfieldnuclearmatterparameterpolarizationspin
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In the present work, we are interested in the properties of nuclear matter at zero temperature in the presence of strong magnetic fields using the lowest order constraint variational (LOCV) method employing $AV_{18}$ nuclear potential. Our results indicate that in the absence of a magnetic field, the energy per particle is a symmetric function of the spin polarization parameter. This shows that for the nuclear matter, the spontaneous phase transition to a ferromagnetic state does not occur. However, we have found that for the magnetic fields $ B\gtrsim 10 ^ {18}\ G$, the symmetry of energy is broken and the energy has a minimum at a positive value of the spin polarization parameter. We have also found that the effect of magnetic field on the value of energy is more significant at the low densities. Our calculations show that at lower densities, the spin polarization parameter is more sensitive to the magnetic field.

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