Physics
Scientific paper
Apr 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jphg...34..653t&link_type=abstract
Journal of Physics G: Nuclear and Particle Physics, Volume 34, Issue 4, pp. 653-659 (2007).
Physics
4
Scientific paper
We explore within the mean-field theory with TM1 parametrization the possibility of the π0 condensation under strong external magnetic fields in neutron star matter that includes sigma particles. At the magnetic field of B = 1018 G, π0 does not condense. At B = 6 × 1018 G, π0 condensation together with a partial stiffening of the matter equation of state occurs in the baryon number densities below 1 fm-3. It is anticipated that the average magnetic field in the stellar interior does not exceed O(1018) G in a neutron star as massive as two times a solar mass.
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