The Magnetar Connection

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 magnet...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Hauptverfasser:	Chowhan, Tanmay Tushar, Konar, Sushan, Banik, Sarmistha
Format:	Artikel
Sprache:	eng
Schlagworte:	Physics - High Energy Astrophysical Phenomena
Online-Zugang:	Volltext bestellen
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

container_end_page
container_issue
container_start_page
container_title
container_volume
creator	Chowhan, Tanmay Tushar Konar, Sushan Banik, Sarmistha
description	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.
doi_str_mv	10.48550/arxiv.2201.05248
format	Article
fullrecord	<record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_2201_05248</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2201_05248</sourcerecordid><originalsourceid>FETCH-LOGICAL-a678-ca2a8765bcb3e0f95a0e20519c2cecd4985617af452f2e6bd8c9b5e1c8b67b4c3</originalsourceid><addsrcrecordid>eNotzr0OgjAUQOEuDkadjZO8ANiW3lJGQ_xLNC7s5PZ6URIFg8To2xvR6WwnnxAzJSPjAOQC21f1jLSWKpKgjRuKaX7h4IDnmjtsg6ypa6auauqxGJR4ffDk35HI16s824b742aXLfch2sSFhBpdYsGTj1mWKaBkLUGlpInpZFIHViVYGtClZutPjlIPrMh5m3hD8UjMf9teVtzb6obtu_gKi14YfwBBnTT2</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>The Magnetar Connection</title><source>arXiv.org</source><creator>Chowhan, Tanmay Tushar ; Konar, Sushan ; Banik, Sarmistha</creator><creatorcontrib>Chowhan, Tanmay Tushar ; Konar, Sushan ; Banik, Sarmistha</creatorcontrib><description>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.</description><identifier>DOI: 10.48550/arxiv.2201.05248</identifier><language>eng</language><subject>Physics - High Energy Astrophysical Phenomena</subject><creationdate>2022-01</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2201.05248$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2201.05248$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Chowhan, Tanmay Tushar</creatorcontrib><creatorcontrib>Konar, Sushan</creatorcontrib><creatorcontrib>Banik, Sarmistha</creatorcontrib><title>The Magnetar Connection</title><description>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.</description><subject>Physics - High Energy Astrophysical Phenomena</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotzr0OgjAUQOEuDkadjZO8ANiW3lJGQ_xLNC7s5PZ6URIFg8To2xvR6WwnnxAzJSPjAOQC21f1jLSWKpKgjRuKaX7h4IDnmjtsg6ypa6auauqxGJR4ffDk35HI16s824b742aXLfch2sSFhBpdYsGTj1mWKaBkLUGlpInpZFIHViVYGtClZutPjlIPrMh5m3hD8UjMf9teVtzb6obtu_gKi14YfwBBnTT2</recordid><startdate>20220107</startdate><enddate>20220107</enddate><creator>Chowhan, Tanmay Tushar</creator><creator>Konar, Sushan</creator><creator>Banik, Sarmistha</creator><scope>GOX</scope></search><sort><creationdate>20220107</creationdate><title>The Magnetar Connection</title><author>Chowhan, Tanmay Tushar ; Konar, Sushan ; Banik, Sarmistha</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a678-ca2a8765bcb3e0f95a0e20519c2cecd4985617af452f2e6bd8c9b5e1c8b67b4c3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Physics - High Energy Astrophysical Phenomena</topic><toplevel>online_resources</toplevel><creatorcontrib>Chowhan, Tanmay Tushar</creatorcontrib><creatorcontrib>Konar, Sushan</creatorcontrib><creatorcontrib>Banik, Sarmistha</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Chowhan, Tanmay Tushar</au><au>Konar, Sushan</au><au>Banik, Sarmistha</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Magnetar Connection</atitle><date>2022-01-07</date><risdate>2022</risdate><abstract>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.</abstract><doi>10.48550/arxiv.2201.05248</doi><oa>free_for_read</oa></addata></record>
fulltext	fulltext_linktorsrc
identifier	DOI: 10.48550/arxiv.2201.05248
ispartof
issn
language	eng
recordid	cdi_arxiv_primary_2201_05248
source	arXiv.org
subjects	Physics - High Energy Astrophysical Phenomena
title	The Magnetar Connection
url	https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-26T02%3A25%3A04IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-arxiv_GOX&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20Magnetar%20Connection&rft.au=Chowhan,%20Tanmay%20Tushar&rft.date=2022-01-07&rft_id=info:doi/10.48550/arxiv.2201.05248&rft_dat=%3Carxiv_GOX%3E2201_05248%3C/arxiv_GOX%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true