Abstract
Properties and mass distribution of ultramagnetized atomic nuclei that arise in heavy-ion collisions, magnetar crusts, during Type II supernova explosions and neutron star mergers are analyzed. For magnetic field strength range 0.1–10 teratesla the Zeeman effect leads to linear nuclear magnetic response with susceptibility parameter exceeding significantly nuclear g-factor. Respectively, binding energies increase for open shell and decrease for closed shell nuclei. Noticeable enhancement in a yield of corresponding explosive nucleosynthesis products with antimagic numbers corroborate with observational results.
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.
