Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/26110
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | AMATI, LORENZO | en_US |
dc.contributor.author | DELLA VALLE, Massimo | en_US |
dc.date.accessioned | 2020-06-17T14:40:42Z | - |
dc.date.available | 2020-06-17T14:40:42Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.isbn | 978-981-4612-14-2 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26110 | - |
dc.description.abstract | Gamma-Ray Bursts (GRB) emit in a few dozen of seconds up to ~10<SUP>54</SUP> erg, in terms of isotropic equivalent radiated energy E<SUB>iso</SUB>, therefore they can be observed up to z ~ 10 and appear very promising tools to describe the expansion rate history of the Universe. In this paper we review the use of the E<SUB>p,i</SUB>-E<SUB>iso</SUB> correlation of Gamma-Ray Bursts to measure Ω<SUB>M</SUB>. We show that the present data set of GRBs, coupled with the assumption that we live in a flat universe, can provide indipendent evidence, from other probes, that Ω<SUB>M</SUB>~0.3. We show that current (e.g., Swift, Fermi/GBM, Konus-WIND) and next GRB experiments (e.g., CALET/GBM, SVOM, Lomonosov/UFFO, LOFT/WFM) will allow us, within a few years, to constrain Ω<SUB>M</SUB> and the evolution of dark energy with time, with an accuracy comparable to that currently exhibited by SNe-Ia. | en_US |
dc.language.iso | eng | en_US |
dc.title | Measuring Cosmological Parameters with Gamma-Ray Bursts | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1142/9789814623995_0038 | en_US |
dc.identifier.scopus | 2-s2.0-85045384951 | en_US |
dc.identifier.url | https://www.worldscientific.com/doi/abs/10.1142/9789814623995_0038 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.firstpage | 769 | en_US |
dc.relation.lastpage | 780 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.alleditors | Rosquist, Kjell;Jantzen, Robert T.; Ruffini, Remo | en_US |
dc.relation.ispartofbook | Thirteenth Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories | en_US |
dc.type.invited | sì | en_US |
dc.relation.conferencename | Thirteenth Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories | en_US |
dc.relation.conferenceplace | Stockholm, Sweden | en_US |
dc.relation.conferencedate | 1 – 7 July, 2012 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2015mgm..conf..769A | 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 | Conference paper | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.orcid | 0000-0001-5355-7388 | - |
crisitem.author.orcid | 0000-0003-3142-5020 | - |
È visualizzato nelle collezioni: | 3.01 Contributi in Atti di convegno |
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Amati_DellaValle_GrossmannMeeting.pdf | 469.88 kB | Adobe PDF | Visualizza/apri |
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