Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/23851
DC Field | Value | Language |
---|---|---|
dc.contributor.author | BUCCIANTINI, NICCOLO' | en_US |
dc.contributor.author | Pili, A. G. | en_US |
dc.contributor.author | Del Zanna, L. | en_US |
dc.date.accessioned | 2020-04-06T06:13:28Z | - |
dc.date.available | 2020-04-06T06:13:28Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/23851 | - |
dc.description.abstract | Magnetic fields play a critical role in the phenomenology of neutron stars. There is virtually no observable aspect which is not governed by them. Despite this, only recently efforts have been done to model magnetic fields in the correct general relativistic regime, characteristic of these compact objects. In this work we present, for the first time, a comprehensive and detailed parameter study, in general relativity, of the role that the currents distribution, and the related magnetic field structure, have in determining the precise structure of neutron stars. In particular, we show how the presence of localized currents can modify the field strength at the stellar surface, and we look for general trends, both in terms of energetic properties and magnetic field configurations. Here we verify that, among other things, for a large class of different current distributions the resulting magnetic configurations are always dominated by the poloidal component of the current. | en_US |
dc.language.iso | eng | en_US |
dc.title | The role of currents distribution in general relativistic equilibria of magnetized neutron stars | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stu2689 | en_US |
dc.identifier.scopus | 2-s2.0-85000995956 | en_US |
dc.identifier.isi | 000350273400024 | en_US |
dc.identifier.url | http://arxiv.org/abs/1412.5347v1 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/447/4/3278/1750392 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 447 | en_US |
dc.relation.issue | 4 | en_US |
dc.relation.firstpage | 3278 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2015MNRAS.447.3278B | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 3 – prodotto già presente in altro archivio Open Access (arXiv, REPEC…) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0002-8848-1392 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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Bucciantini-Pili 2015 "The role of currents distribution in general relativistic equilibria of magnetized" AA.pdf | PDF editoriale | 4.87 MB | Adobe PDF | View/Open |
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