Magnetar formation through a convective dynamo in protoneutron stars
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DOI: 10.1126/sciadv.aay2732
Abstract: Strong field dynamos can explain magnetar formation consistently with the millisecond magnetar model for extreme explosions. The release of spin-down energy by a magnetar is a promising scenario to power several classes of extreme explosive… read more here.
Keywords: magnetar formation; protoneutron; formation convective; formation ... See more keywords