Neutron star equation of state and the possibility of complex self-energy in Landau theory of a Fermi liquid in the presence of a strong, quantizing magnetic field

Physics

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Nuclear Matter Aspects Of Neutron Stars, Spin Arrangements In Magnetically Ordered Materials, Neutron Stars

Scientific paper

Using the relativistic version of Landau theory of Fermi liquid with σ-ω and ρ mesons exchange, we have obtained an equation state for dense neutron star matter in the presence of a strong, quantizing magnetic field. It is found that in this scenario the self-energies of both neutron and proton components of dense neutron star matter become complex under certain physical conditions. To be more specific, it is observed that in the exchange diagrams of σ,ω and neutral ρ transfer processes and in the direct interaction diagram with ρ± transfer reactions, the nucleon self-energies become complex in nature.

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