Key experimental M subshell line x-ray production cross sections for slow light ions on high atomic number targets compared with the ECUSAR theory

Simple item page
dc.contributor.authorCohen, DDen_AU
dc.contributor.authorStelcer, Een_AU
dc.contributor.authorCrawford, Jen_AU
dc.contributor.authorAtanacio, AJen_AU
dc.contributor.authorDoherty, Gen_AU
dc.contributor.authorLapicki, Ken_AU
dc.date.accessioned2015-11-16T05:00:21Zen_AU
dc.date.available2015-11-16T05:00:21Zen_AU
dc.date.issued2013-07-01en_AU
dc.date.statistics2015-11-16en_AU
dc.description.abstractThe x-ray production cross sections for dominant lines in each of the five M subshells have been measured for slow proton and helium ion impact on selected high atomic number targets from tungsten to uranium. Proton energies between 0.5 and 3 MeV and helium ion energies between 0.5 and 2 MeV were used providing M subshell cross sections for 0.3 < x < 3, where x = v /(q v ), as defined by Brandt and Mi s 1 s 2s Lapicki 1979, distinguishes between slow (x < 1) and fast (x > 1) collision regimes. s s Ion energies and targets over these ranges cover the commonly used PIXE range for M subshell x-ray production on heavy targets across the x-ray energy range 1.3-6 keV, which has a strong overlap with key common K shell elements from Al to Fe. Hence it is important for frequently used PIXE analysis programs like GUPIX and GEOPIXE to have a consistent set of M subshell cross sections together with subshell parameters, like fluorescence yields and Coster-Kronig transition rates, which will precisely and accurately predict M shell line intensities over this low energy X-ray region of interest.en_AU
dc.identifier.booktitle13th International Conference on Particle Induced Emission "PIXE 2013", Gramado, Brazil, March 3-8, 2016, Book of Abstracts.en_AU
dc.identifier.citationCohen, D., Stelcer, E., Crawford, J., Atanacio, A., Doherty, G., & Lapicki, K. (2013). Key Experimental M subshell line X-ray production cross sections for slow light ions on high atomic number targets compared with the ECUSAR theory. Presentation to the 13th International Conference on Particle Induced Emission, Gramado, Brazil, 3-8 March 2013. R. C. Fadanelli, F. M. Lúcia Yoneama, J. F. Dias & L. Amaral (Eds), 13th International Conference on Particle Induced Emission "PIXE 2013", Gramado, Brazil, March 3-8, 2016, Book of Abstracts.en_AU
dc.identifier.conferenceenddate8 March 2013en_AU
dc.identifier.conferencename13th International Conference on Particle Induced Emissionen_AU
dc.identifier.conferenceplaceGramado, Brazilen_AU
dc.identifier.conferencestartdate3 March 2013en_AU
dc.identifier.editorsR. C. Fadanelli, F. M. Lúcia Yoneama, J. F. Dias & L. Amaralen_AU
dc.identifier.govdoc6290en_AU
dc.identifier.urihttp://apo.ansto.gov.au/dspace/handle/10238/6419en_AU
dc.language.isoenen_AU
dc.publisherFederal University of Rio Grande do Sul (UFRGS)en_AU
dc.subjectProtonsen_AU
dc.subjectHelium ionsen_AU
dc.subjectAtomic numberen_AU
dc.subjectTungstenen_AU
dc.subjectUraniumen_AU
dc.subjectEnergy rangeen_AU
dc.titleKey experimental M subshell line x-ray production cross sections for slow light ions on high atomic number targets compared with the ECUSAR theoryen_AU
dc.typeConference Abstracten_AU
Files
Original bundle
Now showing 1 - 2 of 2
Thumbnail Image
Name:
Current_Trends_IBA_Techniques_Abstracts.pdf
Size:
2.32 MB
Format:
Adobe Portable Document Format
Description:
Download
Thumbnail Image
Name:
48014565(1).pdf
Size:
735.27 KB
Format:
Adobe Portable Document Format
Description:
Download
License bundle
Now showing 1 - 1 of 1
Thumbnail Image
Name:
license.txt
Size:
1.71 KB
Format:
Item-specific license agreed upon to submission
Description:
Download
Collections
Conference Publications