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arxiv: astro-ph/9703034 · v1 · submitted 1997-03-06 · 🌌 astro-ph · nucl-th

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Dense nuclear matter in a strong magnetic field

Somenath Chakrabarty (University of Kalyani , India) , Debades Bandyopadhyay , Subrata Pal (Saha Institute of Nuclear Physics , Calcutta
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classification 🌌 astro-ph nucl-th
keywords matterfieldnuclearmagneticbetaequilibriumstrongabove
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We investigate in a relativistic Hartree theory the gross properties of cold symmetric nuclear matter and nuclear matter in beta equilibrium under the influence of strong magnetic fields. If the field strengths are above the critical values for electrons and protons, the respective phase spaces are strongly modified. This results in additional binding of the systems with distinctively softer equations of state compared to the field free cases. For magnetic field $\sim 10^{20}$ Gauss and beyond, the nuclear matter in beta equilibrium practically converts into a stable proton rich matter.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Dense Matter and Compact Stars in Strong Magnetic Fields

    astro-ph.HE 2026-04 unverdicted novelty 2.0

    Strong magnetic fields in compact stars induce Landau quantization and magnetic-moment couplings that change the equation of state and allow additional degrees of freedom such as hyperons, Delta resonances, and quark matter.