SGR 0418+5729 as an evolved Quark-Nova compact remnant
Rachid Ouyed, Denis Leahy, Brian Niebergal (Department of Physics and, Astronomy, University of Calgary, Alberta, Canada)

TL;DR
This paper proposes that the peculiar low-magnetic-field soft gamma repeater SGR 0418+5729 can be explained as an evolved quark star with a surrounding debris ring from a Quark-Nova, reproducing its burst and decay properties.
Contribution
It introduces a novel model where low-magnetic-field quark stars with debris rings explain magnetar-like activity, challenging the neutron star magnetic field paradigm.
Findings
A 16 Myr old quark star with a specific debris ring reproduces observed properties.
Magnetic penetration of the ring causes SGR-like bursts.
Predicted observable signatures include an accretion glitch and a sub-keV proton cyclotron line.
Abstract
Soft gamma repeaters and anomalous X-ray pulsars are believed to be magnetars, i.e. neutron stars powered by extreme magnetic fields, B~10^(14)-10^(15) Gauss. The recent discovery of a soft gamma repeater with low magnetic field (< 7.5x10^(12) Gauss), SGR 0418+5729, which shows bursts similar to those of SGRs, implies that a high surface dipolar magnetic field might not be necessary for magnetar-like activity. We show that the quiescent and bursting properties of SGR 0418+5729 find natural explanations in the context of low-magnetic field Quark-Nova (detonative transition from a neutron star to a quark star) remnants, i.e. an old quark star surrounded by degenerate (iron-rich) Keplerian ring/debris ejected during the Quark-Nova explosion. We find that a 16 Myr old quark star surrounded by a ~ 10^(-10)xM_sun ring, extending in radius from ~ 30 km to 60 km, reproduces many observed…
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