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The Magnetar Connection

Published online by Cambridge University Press:  27 February 2023

Tanmay Tushar Chowhan Open the ORCID record for Tanmay Tushar Chowhan [Opens in a new window] ,
Sushan Konar  and
Sarmistha Banik
Tanmay Tushar Chowhan
Affiliation:
Dept. of Physics, BITS Pilani, Hyderabad Campus, Shameerpet Mandal, Hyderabad-500078, India.
Sushan Konar
Affiliation:
NCRA-TIFR, Pune 411007, India
Sarmistha Banik
Affiliation:
Dept. of Physics, BITS Pilani, Hyderabad Campus, Shameerpet Mandal, Hyderabad-500078, India.
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Abstract

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We investigate the combined evolution of the dipolar surface magnetic field (Bs) and the spin-period (Ps) of known Magnetars and high magnetic field ($${{\rm{B}}_s} \mathbin{\lower.3ex\hbox{$\buildrel>\over {\smash{\scriptstyle\sim}\vphantom{_x}}$}} {10^{13}}{\rm{G}}$$) 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 Ps-Bs 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.

Keywords

stars: neutronpulsars: magnetic fieldspulsars: evolution
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 16 , Symposium S363: Neutron Star Astrophysics at the Crossroads: Magnetars and the Multimessenger Revolution , June 2020 , pp. 322 - 323
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

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