Evidence for a multipolar magnetic field in SGR J1745-2900 from X-ray light-curve analysis
Rafael C. R. de Lima, Jaziel G. Coelho, Jonas P. Pereira, Claudia V., Rodrigues, Jorge A. Rueda

TL;DR
This study analyzes 3.5-year X-ray light-curve data of SGR J1745-2900 to infer a multipolar magnetic field structure through hot spot modeling, suggesting complex magnetic topology in this highly magnetized neutron star.
Contribution
It introduces a detailed hot spot model including general relativistic effects to support the presence of multipolar magnetic fields in SGR J1745-2900.
Findings
Light-curve compatible with two or three hot spots
Large hot spots imply complex magnetic field structure
Supports multipolar magnetic field hypothesis
Abstract
SGR J1745-2900 was detected from its outburst activity in April 2013 and it was the first soft gamma repeater (SGR) detected near the center of the Galaxy (Sagittarius A). We use 3.5-year Chandra X-ray light-curve data to constrain some neutron star (NS) geometric parameters. We assume that the flux modulation comes from hot spots on the stellar surface. Our model includes the NS mass, radius, a maximum of three spots of any size, temperature and positions, and general relativistic effects. We find that the light-curve of SGR J1745-2900 could be described by either two or three hot spots. The ambiguity is due to the small amount of data, but our analysis suggests that one should not disregard the possibility of multi-spots (due to a multipolar magnetic field) in highly magnetized stars. For the case of three hot spots, we find that they should be large and have angular…
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