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Chiral density waves in quark matter within the Nambu--Jona-Lasinio model in an external magnetic field

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arxiv 1007.2984 v3 pith:6YCXJGDI submitted 2010-07-18 hep-ph

I. E. Frolov , V. Ch. Zhukovsky , K. G. Klimenko This is my paper · ORCID
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keywords fieldmagneticdensityexternalformationmattermodelnambu--jona-lasinio
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A possibility of formation of static dual scalar and pseudoscalar density wave condensates in dense quark matter is considered for the Nambu--Jona-Lasinio model in an external magnetic field. Within a mean-field approximation, the effective potential of the theory is obtained and its minima are numerically studied; a phase diagram of the system is constructed. It is shown that the presence of a magnetic field favors the formation of spatially inhomogeneous condensate configurations at low temperatures and arbitrary non-zero values of the chemical potential.

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Cited by 1 Pith paper

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  1. How neutron star properties disfavor a nuclear chiral density wave

    nucl-th 2024-11 conditional novelty 6.0 of 10

    Within this nucleon-meson model, a chiral density wave in neutron star cores is only stable for equations of state too soft to support observed two-solar-mass pulsars, predicting isotropic cores.

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