SIMBAD references

2012MNRAS.425.1558D - Mon. Not. R. Astron. Soc., 425, 1558-1566 (2012/September-2)

Magnetars from magnetized cores.

DASS N.D.H. and SONI V.

Abstract (from CDS):

We consider a model in which magnetars arise from a high baryon density, magnetized core which forms when they are born. In this framework, magnetars are distinguished from pulsars by their higher masses and central density. In this model for magnetars, as core densities exceed a threshold, the strong interaction can induce a phase transition to a ground state that aligns nucleon magnetic moments. The core magnetic field is initially shielded by the ambient high-conductivity plasma. With time the shielding currents dissipate transporting the core field out, first to the crust and then breaking through the crust to the surface of the star. Recent observations provide support for this model which accounts for several properties of magnetars and also enables us to identify new magnetars.

Abstract Copyright: 2012 The Authors Monthly Notices of the Royal Astronomical Society 2012 RAS

Journal keyword(s): equation of state - magnetic fields - stars: neutron

CDS comments: In Table 1 PSR 0154-61 is a misprint for PSR 0154+61.

Simbad objects: 11

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2020.02.17-10:23:24

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