Investigating magnetically induced distortions of neutron stars through gamma-ray burst X-ray plateaus

The magnetic field may distort neutron stars (NSs), but its e ffect has not yet been robustly tested through gravitational-wave observations due to the absence of a fast-rotating Galactic magnetar. The investigation of parts of gamma-ray bursts (GRBs) can potentially shed light on the magnetically induced distortion since their central objects may be millisecond magnetars. In this paper we propose a method for estimating the distortions of these possible magnetars under the GRB magnetar scenario. According to the case study of GRB 070521, we find a relation between the e ffective magnetically induced ellipticity, similar to B;e ff, and the e ffective dipole magnetic field strength on NS surfaces, Be ff, namely similar to B;eff similar to 10(-3)(Beff=10(15) G)2. Furthermore, we constrain the internal magnetic field structure of the magnetar to be Be ff similar to 0:02 h Bt i and Be ff similar to 0:1 B-t, where (B-t) i is the volume-averaged internal toroidal field. This constraint can be used as the initial condition in modeling the structure of NS magnetospheres. Finally, the possibility of testing the method shown in this paper through gravitational-wave observations is discussed.

Automated summary

This paper proposes a method for estimating the distortions of magnetars in gamma-ray bursts (GRBs), and finds a relation between the effective magnetically induced ellipticity and the dipole magnetic field strength on neutron star surfaces. The paper also constrains the internal magnetic field structure of the magnetar and discusses the possibility of testing the method through gravitational-wave observations.