Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/28831
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Santangelo, Andrea | en_US |
dc.contributor.author | Zane, Silvia | en_US |
dc.contributor.author | Feng, Hua | en_US |
dc.contributor.author | Xu, RenXin | en_US |
dc.contributor.author | Doroshenko, Victor | en_US |
dc.contributor.author | Bozzo, Enrico | en_US |
dc.contributor.author | Caiazzo, Ilaria | en_US |
dc.contributor.author | Zelati, Francesco Coti | en_US |
dc.contributor.author | ESPOSITO, PAOLO | en_US |
dc.contributor.author | González-Caniulef, Denis | en_US |
dc.contributor.author | Heyl, Jeremy | en_US |
dc.contributor.author | Huppenkothen, Daniela | en_US |
dc.contributor.author | ISRAEL, Gian Luca | en_US |
dc.contributor.author | Li, ZhaoSheng | en_US |
dc.contributor.author | Lin, Lin | en_US |
dc.contributor.author | MIGNANI, Roberto | en_US |
dc.contributor.author | Rea, Nanda | en_US |
dc.contributor.author | ORLANDINI, MAURO | en_US |
dc.contributor.author | Taverna, Roberto | en_US |
dc.contributor.author | Tong, Hao | en_US |
dc.contributor.author | Turolla, Roberto | en_US |
dc.contributor.author | Baglio, Cristina | en_US |
dc.contributor.author | BERNARDINI, Federico | en_US |
dc.contributor.author | BUCCIANTINI, NICCOLO' | en_US |
dc.contributor.author | FEROCI, MARCO | en_US |
dc.contributor.author | Fürst, Felix | en_US |
dc.contributor.author | Göğüș, Ersin | en_US |
dc.contributor.author | Güngör, Can | en_US |
dc.contributor.author | Ji, Long | en_US |
dc.contributor.author | Lu, FangJun | en_US |
dc.contributor.author | Manousakis, Antonios | en_US |
dc.contributor.author | MEREGHETTI, Sandro | en_US |
dc.contributor.author | MIKUSINCOVA, Romana | en_US |
dc.contributor.author | Paul, Biswajit | en_US |
dc.contributor.author | Prescod-Weinstein, Chanda | en_US |
dc.contributor.author | Younes, George | en_US |
dc.contributor.author | TIENGO, ANDREA | en_US |
dc.contributor.author | Xu, YuPeng | en_US |
dc.contributor.author | Watts, Anna | en_US |
dc.contributor.author | Zhang, Shu | en_US |
dc.contributor.author | Zhan, Shuang-Nan | en_US |
dc.date.accessioned | 2020-12-14T14:42:06Z | - |
dc.date.available | 2020-12-14T14:42:06Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 1674-7348 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28831 | - |
dc.description.abstract | In this paper we present the science potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies of strongly magnetized objects. We will focus on the physics and astrophysics of strongly magnetized objects, namely magnetars, accreting X-ray pulsars, and rotation powered pulsars. We also discuss the science potential of eXTP for QED studies. Developed by an international Consortium led by the Institute of High Energy Physics of the Chinese Academy of Sciences, the eXTP mission is expected to be launched in the mid 2020s. | en_US |
dc.language.iso | eng | en_US |
dc.title | Physics and astrophysics of strong magnetic field systems with eXTP | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1007/s11433-018-9234-3 | en_US |
dc.identifier.scopus | 2-s2.0-85052732116 | en_US |
dc.identifier.isi | 000448444300001 | en_US |
dc.identifier.url | https://link.springer.com/article/10.1007/s11433-018-9234-3 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 62 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 29505 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | DEU | en_US |
dc.contributor.country | ESP | en_US |
dc.contributor.country | CAN | en_US |
dc.contributor.country | ARE | en_US |
dc.contributor.country | IND | en_US |
dc.contributor.country | OMN | en_US |
dc.contributor.country | NLD | en_US |
dc.contributor.country | POL | en_US |
dc.contributor.country | CHN | en_US |
dc.contributor.country | CHE | en_US |
dc.contributor.country | TUR | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | SCIENCE CHINA. PHYSICS, MECHANICS & ASTRONOMY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2019SCPMA..6229505S | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | 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. Roma | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.orcid | 0000-0001-5480-6438 | - |
crisitem.author.orcid | 0000-0002-8685-583x | - |
crisitem.author.orcid | 0000-0003-0946-3151 | - |
crisitem.author.orcid | 0000-0002-8848-1392 | - |
crisitem.author.orcid | 0000-0002-7617-3421 | - |
crisitem.author.orcid | 0000-0003-3259-7801 | - |
crisitem.journal.journalissn | 1674-7348 | - |
crisitem.journal.ance | E214811 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
eXTP.pdf | postprint | 4.37 MB | Adobe PDF | View/Open |
Santangelo2018_Article_PhysicsAndAstrophysicsOfStrong.pdf | [Administrators only] | 2.08 MB | Adobe PDF |
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