Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/23624
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Blasi, P. | en_US |
dc.contributor.author | AMATO, Elena | en_US |
dc.contributor.author | D'Angelo, M. | en_US |
dc.date.accessioned | 2020-03-27T08:02:26Z | - |
dc.date.available | 2020-03-27T08:02:26Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.issn | 1824-8039 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/23624 | - |
dc.description.abstract | Most models of the origin of ultra high energy cosmic rays rely on the existence of luminous extragalactic sources. Cosmic rays escaping the galaxy where the source is located produce a suf- ficiently large electric current to justify the investigation of plasma instabilities induced by such current. Most interesting is the excitation of modes that lead to production of magnetic perturba- tions that may scatter particles thereby hindering their escape, or at least changing the propagation mode of escaping cosmic rays. We argue that self-generation of waves may force cosmic rays to be confined in the source proximity for energies $E<10^7\ L_{44}^{23}$ GeV for low background magnetic fields ($B_0 \ll$ nG). For larger values of $B_0$, cosmic rays are confined close to their sources for energies $E < 2 \times 10^8\ \lambda_{10}\ L_{44}^{1/4} B_{-10}^{1/2}$ GeV, where $B_{-10}$ is the field in units of 0.1 nG, $\lambda_{10}$ is its coherence length in units of 10 Mpc and $L_{44}$ is the source luminosity in units of $10^{44}$ erg/s. | en_US |
dc.language.iso | eng | en_US |
dc.title | Cosmic ray self-confinement close to extragalactic sources | en_US |
dc.type | Conference paper | - |
dc.identifier.url | https://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=236 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 34 | en_US |
dc.relation.firstpage | 505 | en_US |
dc.type.referee | REF_4 | en_US |
dc.description.numberofauthors | 3 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.ispartofbook | 34th International Cosmic Ray Conference (ICRC2015) | en_US |
dc.type.invited | no | en_US |
dc.relation.conferencename | 34th International Cosmic Ray Conference (ICRC2015) | en_US |
dc.relation.conferenceplace | The Hague, The Netherlands | en_US |
dc.relation.conferencedate | 30 July - 6 August, 2015 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | POS PROCEEDINGS OF SCIENCE | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2015ICRC...34..505B | en_US |
dc.relation.ercsector | Scienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_10 High energy and particle astronomy – X-rays, cosmic rays, gamma rays, neutrinos | 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.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Conference paper | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 1824-8039 | - |
crisitem.journal.ance | E188909 | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0002-9881-8112 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
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15_ICRC_Blasi.pdf | PDF editoriale | 115.13 kB | Adobe PDF | View/Open |
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