The Upper Limit of Magnetic Field Strength in Dense Stellar Hadronic Matter

Details The Upper Limit of Magnetic Field Strength in Dense Stellar Hadronic Matter The Upper Limit of Magnetic Field Strength in Dense Stellar Hadronic Matter

2006-06-22

arxiv.org/abs/astro-ph/0606549v1

Astrophys.SpaceSci.310:195-199,2007

Astronomy and Astrophysics

Astrophysics

6 pages Revtex, 2 .eps figures, fig.(1) is not included

Scientific paper

10.1007/s10509-007-9500-1

It is shown that in strongly magnetized neutron stars, there exist upper limits of magnetic field strength, beyond which the self energies for both neutron and proton components of neutron star matter become complex in nature. As a consequence they decay within the strong interaction time scale. However, in the ultra-strong magnetic field case, when the zeroth Landau level is only occupied by protons, the system again becomes stable against strong decay.

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