Abstract
A relativistic mean-field model is used to study the properties of neutron matter at high densities. It is found that a transition to an electrically polarized phase occurs at a density in the range of stable neutron stars. For a rotating neutron star this electric polarization can give rise to a magnetic field comparable to current estimates of the pulsar magnetic field.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
