Speaker
Mr
J P W Diener
(Stellenbosch University)
Description
The magnetic properties of matter under extreme conditions are of particular importance to understand the neutron star interior. One contributing factor to the neutron star’s magnetic field could be the ferromagnetic phase of nuclear matter. Using a relativistic model we calculated the ferromagnetic phase diagram for dense neutron matter.
Primary author
Mr
J P W Diener
(Stellenbosch University)
Co-author
Prof.
F G Scholtz
(Stellenbosch University/NITheP)
