Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24572
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Pili, A. G. | en_US |
dc.contributor.author | BUCCIANTINI, NICCOLO' | en_US |
dc.contributor.author | Drago, A. | en_US |
dc.contributor.author | Pagliara, G. | en_US |
dc.contributor.author | Del Zanna, L. | en_US |
dc.date.accessioned | 2020-05-07T07:48:09Z | - |
dc.date.available | 2020-05-07T07:48:09Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 1745-3925 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24572 | - |
dc.description.abstract | We investigate the possible implications of quark deconfinement on the phenomenology of long gamma-ray bursts focusing, in particular, on the possibility to describe multiple prompt emission phases in the context of the proto-magnetar model. Starting from numerical models of rotating Hadron Stars and Quark Stars in full general relativity we track the electromagnetic spin-down evolution in both the hadronic and quark phase, linking the two families through conservation of baryon number and angular momentum. We give estimates of the time-scales and the energetics involved in the spin-down process deriving, in the relevant spin range, the relation between the initial and the final masses and rotational energies, whenever hadron-quark conversion is possible. We show how the results can be used in relevant astrophysical cases such as the double burst GRB 110709B. | en_US |
dc.language.iso | eng | en_US |
dc.title | Quark deconfinement in the proto-magnetar model of long gamma-ray bursts | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnrasl/slw115 | en_US |
dc.identifier.scopus | 2-s2.0-84988660380 | en_US |
dc.identifier.isi | 000383516700006 | en_US |
dc.identifier.url | http://arxiv.org/abs/1606.02075v1 | en_US |
dc.identifier.url | https://academic.oup.com/mnrasl/article/462/1/L26/2589556 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 462 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | L26 | en_US |
dc.relation.lastpage | L30 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 5 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. LETTERS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2016MNRAS.462L..26P | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_11 Relativistic astrophysics | 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. Arcetri | - |
crisitem.author.orcid | 0000-0002-8848-1392 | - |
crisitem.journal.journalissn | 1745-3925 | - |
crisitem.journal.ance | E205843 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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slw115.pdf | PDF editoriale | 871.63 kB | Adobe PDF | View/Open |
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