We describe one of the so-called low magnetic field magnetars SGR 0418+5729,
as a massive fast rotating highly magnetized white dwarf following Malheiro et.
al. 2012. We give bounds for the mass, radius, moment of inertia, and magnetic
field for these sources, by requesting the stability of realistic general
relativistic uniformly rotating configurations. Based on these parameters, we
improve the theoretical prediction of the lower limit of the spin-down rate of
SGR 0418+5729. In addition, we compute the electron cyclotron frequencies
corresponding to the predicted surface magnetic fields.
%0 Journal Article
%1 citeulike:13549889
%A Boshkayev, Kuantay
%A Rueda, Jorge A.
%A Ruffini, Remo
%B The Thirteenth Marcel Grossmann Meeting
%D 2015
%I WORLD SCIENTIFIC
%K imported
%P 2295--2300
%R 10.1142/9789814623995\_0424
%T SGRs and AXPs as massive fast rotating highly magnetized white dwarfs: the case of SGR 0418+5729
%U http://dx.doi.org/10.1142/9789814623995\_0424
%X We describe one of the so-called low magnetic field magnetars SGR 0418+5729,
as a massive fast rotating highly magnetized white dwarf following Malheiro et.
al. 2012. We give bounds for the mass, radius, moment of inertia, and magnetic
field for these sources, by requesting the stability of realistic general
relativistic uniformly rotating configurations. Based on these parameters, we
improve the theoretical prediction of the lower limit of the spin-down rate of
SGR 0418+5729. In addition, we compute the electron cyclotron frequencies
corresponding to the predicted surface magnetic fields.
%@ 978-981-4612-14-2
@article{citeulike:13549889,
abstract = {{We describe one of the so-called low magnetic field magnetars SGR 0418+5729,
as a massive fast rotating highly magnetized white dwarf following Malheiro et.
al. 2012. We give bounds for the mass, radius, moment of inertia, and magnetic
field for these sources, by requesting the stability of realistic general
relativistic uniformly rotating configurations. Based on these parameters, we
improve the theoretical prediction of the lower limit of the spin-down rate of
SGR 0418+5729. In addition, we compute the electron cyclotron frequencies
corresponding to the predicted surface magnetic fields.}},
added-at = {2019-03-25T08:20:55.000+0100},
archiveprefix = {arXiv},
author = {Boshkayev, Kuantay and Rueda, Jorge A. and Ruffini, Remo},
biburl = {https://www.bibsonomy.org/bibtex/265a985c8a4fcfa43187a16b215168dd2/ericblackman},
booktitle = {The Thirteenth Marcel Grossmann Meeting},
citeulike-article-id = {13549889},
citeulike-linkout-0 = {http://arxiv.org/abs/1503.04176},
citeulike-linkout-1 = {http://arxiv.org/pdf/1503.04176},
citeulike-linkout-2 = {http://dx.doi.org/10.1142/9789814623995\_0424},
day = 13,
doi = {10.1142/9789814623995\_0424},
eprint = {1503.04176},
interhash = {2bf6fb59c83e55ba4d11ef547b9c1911},
intrahash = {65a985c8a4fcfa43187a16b215168dd2},
isbn = {978-981-4612-14-2},
keywords = {imported},
location = {Stockholm University, Sweden},
month = mar,
pages = {2295--2300},
posted-at = {2015-03-16 08:09:06},
priority = {2},
publisher = {WORLD SCIENTIFIC},
timestamp = {2019-03-25T08:20:55.000+0100},
title = {{SGRs and AXPs as massive fast rotating highly magnetized white dwarfs: the case of SGR 0418+5729}},
url = {http://dx.doi.org/10.1142/9789814623995\_0424},
year = 2015
}