Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26882
DC Field | Value | Language |
---|---|---|
dc.contributor.author | GHISELLINI, Gabriele | en_US |
dc.date.accessioned | 2020-08-27T12:51:04Z | - |
dc.date.available | 2020-08-27T12:51:04Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26882 | - |
dc.description.abstract | Fast radio bursts, with a typical duration of 1 ms and 1 Jy flux density at gigahertz frequencies, have brightness temperatures exceeding 10<SUP>33</SUP> K, requiring a coherent emission process. This can be achieved by bunching particles in volumes smaller than the typical wavelength, but this may be challenging. Maser emission is a possibility. Under certain conditions, the synchrotron-stimulated emission process can be more important than true absorption, and a synchrotron maser can be created. This occurs when the emitting electrons have a very narrow distribution of pitch angles and energies. This process overcomes the difficulties of having extremely dense bunches of particles and relaxes the light-crossing time limits, since there is no simple relation between the actual size of the source and the observed variability time-scale. | en_US |
dc.language.iso | eng | en_US |
dc.title | Synchrotron masers and fast radio bursts | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnrasl/slw202 | en_US |
dc.identifier.scopus | 2-s2.0-85010081700 | en_US |
dc.identifier.isi | 000403083900007 | en_US |
dc.identifier.url | https://academic.oup.com/mnrasl/article/465/1/L30/2404603 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 465 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | L30 | 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 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017MNRAS.465L..30G | 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 | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.grantfulltext | open | - |
item.cerifentitytype | Publications | - |
item.openairetype | Article | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.orcid | 0000-0002-0037-1974 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
syncrotron-radio-bursts2017.pdf | PDF editoriale | 292.73 kB | Adobe PDF | View/Open |
maser1609.04815.pdf | preprint | 144.44 kB | Adobe PDF | View/Open |
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