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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

References

Abhishek et al., 2022, submitted to JApA, arXiv:2201.00295Google Scholar
Chen, K., Ruderman, M., 1993, ApJ, 402, 264 CrossRefGoogle Scholar
Ertan, U & Alpar, M. A., 2021, MNRAS, 505, L112 CrossRefGoogle Scholar
Jackson, J. D., 1975, Classical Electrodynamics, Wiley Google Scholar
Jawor, J. A., & Tauris, T. M., 2022, MNRAS, 509, 634 CrossRefGoogle Scholar
Igoshev, A. P., Popov, S. B., 2015, AN, 336, 831 Google Scholar
Kaspi, V. M., 2011, ApJ, 741, L13A Google Scholar
Konar, S., 1997, PhD Thesis, Indian Institute of Science, BangaloreGoogle Scholar
Konar, S., 2017, JApA, 38, 47 Google Scholar
Pons, J. A., Vigano, D., 2019, LRCA, 5, 3 Google Scholar