Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/27173
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Tamburini, Fabrizio | en_US |
dc.contributor.author | De Laurentis, Mariafelicia | en_US |
dc.contributor.author | AMATI, LORENZO | en_US |
dc.contributor.author | Thidé, Bo | en_US |
dc.date.accessioned | 2020-09-07T11:28:57Z | - |
dc.date.available | 2020-09-07T11:28:57Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 2470-0010 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27173 | - |
dc.description.abstract | We propose a new energy extraction mechanism from the rotational energy of a Kerr-Newman black hole by a gravitating massive photon field generated by electromagnetic and gravitational field coupling effects. Numerical studies show that this mechanism that depends on the black hole rotation parameter, a , shows a clear dependence on the black hole mass, M , and charge, Q , and can extract energies up to 1 0<SUP>54</SUP> erg for a black hole of the solar mass size. With this mechanism we can set a lower bound on the coupling ξ ∼10<SUP>-38</SUP> between electromagnetic and gravitational fields that might be used to explain the hypothetical extremely high energy release, >10<SUP>53</SUP> erg, suggested by the observations of some gamma-ray bursts in the controversial "energy crisis" problem if and when gamma-ray bursts seem not to show evidence for collimated emission. | en_US |
dc.language.iso | eng | en_US |
dc.title | General relativistic electromagnetic and massive vector field effects with gamma-ray burst production | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1103/PhysRevD.96.104003 | en_US |
dc.identifier.scopus | 2-s2.0-85037134827 | en_US |
dc.identifier.isi | 000414421400005 | en_US |
dc.identifier.url | https://journals.aps.org/prd/abstract/10.1103/PhysRevD.96.104003 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 96 | en_US |
dc.relation.issue | 10 | en_US |
dc.relation.firstpage | 104003 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 4 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | DEU | en_US |
dc.contributor.country | SWE | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | PHYSICAL REVIEW D | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017PhRvD..96j4003T | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering | 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 | OAS Bologna | - |
crisitem.author.orcid | 0000-0001-5355-7388 | - |
crisitem.journal.journalissn | 2470-0010 | - |
crisitem.journal.ance | E237397 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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PhysRevD.96.104003.pdf | Pdf editoriale | 184.03 kB | Adobe PDF | View/Open |
1603.01464.pdf | 231.22 kB | Adobe PDF | View/Open |
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