Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/31875
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Amelino-Camelia, Giovanni | en_US |
dc.contributor.author | D’amico, Giacomo | en_US |
dc.contributor.author | FIORE, Fabrizio | en_US |
dc.contributor.author | Puccetti, Simonetta | en_US |
dc.contributor.author | Ronco, Michele | en_US |
dc.date.accessioned | 2022-03-24T14:10:53Z | - |
dc.date.available | 2022-03-24T14:10:53Z | - |
dc.date.issued | 2021 | en_US |
dc.identifier.issn | 2073-8994 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31875 | - |
dc.description.abstract | Some recent studies exposed preliminary but rather intriguing statistical evidence of in vacuo dispersion-like spectral lags for gamma-ray bursts (GRBs), a linear correlation between time of observation and energy of GRB particles, which is expected in some models of quantum geometry. Those results focused on testing in vacuo dispersion for the most energetic GRB particles, and in particular only included photons with energy at emission greater than 40 GeV. We here extend the window of the statistical analysis down to 5 GeV and find results that are consistent with what had been previously noticed at higher energies. | en_US |
dc.language.iso | eng | en_US |
dc.title | In vacuo dispersion-like spectral lags in gamma-ray bursts | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3390/sym13040541 | en_US |
dc.identifier.scopus | 2-s2.0-85103858290 | en_US |
dc.identifier.url | https://www.mdpi.com/2073-8994/13/4/541 | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/85103858290 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 13 | en_US |
dc.relation.issue | 4 | en_US |
dc.relation.firstpage | 541 | en_US |
dc.type.referee | REF_1 | 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 | SYMMETRY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.relation.fund | H2020 | en_US |
dc.relation.project | HERMES-SP (High Energy Rapid Modular Ensemble of Satellites, Scientific Pathfinder) | 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 | en_US |
dc.description.apc | sì | 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. Trieste | - |
crisitem.author.orcid | 0000-0002-4031-4157 | - |
crisitem.project.grantno | 821896 | - |
crisitem.journal.journalissn | 2073-8994 | - |
crisitem.journal.ance | E200475 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
symmetry-13-00541-v2.pdf | Pdf editoriale | 487.77 kB | Adobe PDF | View/Open |
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