Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/25153
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Vaidya, B. | en_US |
dc.contributor.author | Mignone, A. | en_US |
dc.contributor.author | BODO, Gianluigi | en_US |
dc.contributor.author | MASSAGLIA, SILVANO | en_US |
dc.date.accessioned | 2020-05-25T14:48:23Z | - |
dc.date.available | 2020-05-25T14:48:23Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 1742-6588 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/25153 | - |
dc.description.abstract | We present an implementation of a fully parallel hybrid framework for the evolution of Lagrangian particles coupled to a MHD fluid for the PLUTO code. For the applications of interest, particles represent ensembles of electrons whose spectral energy distribution is governed by a kinetic transport equation that takes into account different physical processes such as diffusive shock acceleration, synchrotron emission and adiabatic expansion. An application to model non-thermal emission from extragalactic jets shows the effectiveness and strength of the approach in describing not only the dynamics but also the radiation properties of jets and, in general, of high-energy astrophysical plasma environments. | en_US |
dc.language.iso | eng | en_US |
dc.title | A fluid-particle hybrid framework for the PLUTO code: applications to non-thermal emission in jets | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1088/1742-6596/719/1/012023 | en_US |
dc.identifier.scopus | 2-s2.0-84978044102 | en_US |
dc.identifier.isi | 000386617200023 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.1088/1742-6596/719/1/012023 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 719 | en_US |
dc.relation.issue | 1 | en |
dc.relation.firstpage | 012023 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | no | en_US |
dc.publisher.name | IOP | en_US |
dc.relation.conferencename | 10th International Conference on Numerical Modeling of Space Plasma Flows: ASTRONUM-2015 | en_US |
dc.relation.conferenceplace | Avignon, France | en_US |
dc.relation.conferencedate | 8 - 12 June 2015 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | JOURNAL OF PHYSICS. CONFERENCE SERIES | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2016JPhCS.719a2023V | 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.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 | O.A. Torino | - |
crisitem.author.orcid | 0000-0002-9265-4081 | - |
crisitem.journal.journalissn | 1742-6588 | - |
crisitem.journal.ance | E187130 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Vaidya_2016_J._Phys.__Conf._Ser._719_012023.pdf | 2.72 MB | Adobe PDF | View/Open |
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