Abstract
Coexistence of core superfluids with pion condensates in neutron star interior is studied for the neutral (π 0 ), charged (π c ) and coexistent (π 0 p c ) pion condensations, for which we adopt the simple model only with the π-N P-wave interaction described in Chapter III. Main points of the results obtained are: (1) Under the π 0 condensation, the neutron 3 P 2 -type superfluidity and the proton 1 S 0 -type one can exist with energy gaps of the same order of magnitude as those realized from the normal phase, (2) under the π c condensation, the quasi-neutron 3 P 2 superfluidity persists although considerable attenuation occurs, and (3) under the π 0 p c condensation, the quasi-neutron 3 P 2 -dominant superfluidity can exist without substantial reduction of energy gaps
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.
