http://arxiv.org/abs/2201.05248
We investigate the combined evolution of the dipolar surface magnetic field (B$_{s}$) and the spin-period (P$_s$) of known magnetars and high magnetic field (B$_s$ $ \gtrsim 10^{13}$~G) radio pulsars. We study the long term behaviour of these objects assuming a simple ohmic dissipation of the magnetic field. Identifying the regions (in the P$_s$-B$_s$ plane) in which these neutron stars would likely move into, before crossing the death-line to enter the pulsar graveyard, we comment upon the possible connection between the magnetars and other classes of neutron stars.
T. Chowhan, S. Konar and S. Banik
Mon, 17 Jan 22
58/59
Comments: 2 pages, 1 figure, To be published in Proceedings of the International Astronomical Union (S363)
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