Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/23592
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Grimani, C. | en_US |
dc.contributor.author | Fabi, M. | en_US |
dc.contributor.author | Lobo, A. | en_US |
dc.contributor.author | Mateos, I. | en_US |
dc.contributor.author | TELLONI, Daniele | en_US |
dc.date.accessioned | 2020-03-26T11:25:06Z | - |
dc.date.available | 2020-03-26T11:25:06Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.issn | 0264-9381 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/23592 | - |
dc.description.abstract | Metal free-floating test masses aboard the future interferometers devoted to gravitational wave detection in space are charged by galactic and solar cosmic rays with energies \gt 100 MeV/n. This process represents one of the main sources of noise in the lowest frequency band (\lt 10<SUP>-3</SUP> Hz) of these experiments. We study here the charging of the LISA Pathfinder (LISA-PF) gold-platinum test masses due to galactic cosmic-ray (GCR) protons and helium nuclei with the Fluka Monte Carlo toolkit. Projections of the energy spectra of GCRs during the LISA-PF operations in 2015 are considered. This work was carried out on the basis of the solar activity level and solar polarity epoch expected for LISA-PF. The effects of GCR short-term variations are evaluated here for the first time. Classical Forbush decreases, GCR variations induced by the Sun rotation, and fluctuations in the LISA-PF frequency bandwidth are discussed. | en_US |
dc.language.iso | eng | en_US |
dc.title | LISA Pathfinder test-mass charging during galactic cosmic-ray flux short-term variations | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1088/0264-9381/32/3/035001 | en_US |
dc.identifier.scopus | 2-s2.0-84921033934 | en_US |
dc.identifier.isi | 000349155600002 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.1088/0264-9381/32/3/035001 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 32 | en_US |
dc.relation.issue | 3 | en_US |
dc.relation.firstpage | 035001 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | CLASSICAL AND QUANTUM GRAVITY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2015CQGra..32c5001G | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegherò il file al passo 5-Carica) | en_US |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
crisitem.journal.journalissn | 0264-9381 | - |
crisitem.journal.ance | E037774 | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.orcid | 0000-0002-6710-8142 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
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CQG_CG_ST.pdf | postprint | 1.28 MB | Adobe PDF | Visualizza/apri |
P16_Grimani_et_al_2015.pdf | [Administrators only] | 931.08 kB | Adobe PDF |
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