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Please use this identifier to cite or link to this item: http://repository.iitr.ac.in/handle/123456789/4054
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dc.contributor.authorOswal M.-
dc.contributor.authorKumar S.-
dc.contributor.authorSingh U.-
dc.contributor.authorSingh G.-
dc.contributor.authorSingh K.P.-
dc.contributor.authorMehta D.-
dc.contributor.authorMitnik D.-
dc.contributor.authorMontanari C.C.-
dc.contributor.authorNandi T.-
dc.date.accessioned2020-10-06T14:31:07Z-
dc.date.available2020-10-06T14:31:07Z-
dc.date.issued2018-
dc.identifier.citationNuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and Atoms (2018), 416(): 110-118-
dc.identifier.issn0168583X-
dc.identifier.urihttps://doi.org/10.1016/j.nimb.2017.11.025-
dc.identifier.urihttp://repository.iitr.ac.in/handle/123456789/4054-
dc.description.abstractTotal L x-ray production cross sections have been measured in 74W, 79Au, 82Pb, and 83Bi by impact of 3–5 MeV/u 28Si ions, with different charge states q = 8+ up to 12+. We find that the measured cross sections do not differ with the charge state of the projectile ions, but they vary with the beam energies. The experimental data has been compared with three theoretical results, ECUSAR, ECPSSR and SLPA by using the multiple-hole fluorescence and Coster-Kronig yields. The comparison has showed the best agreement with the ECUSAR. The SLPA results also describe the experiments quite well for 74W, 79Au and 83Bi, but certain differences are observed for 82Pb, while the ECPSSR values underestimate by up to a factor two. Surprisingly, the theoretical-experimental agreement is better at low beam energies than in the high beam energy side. © 2017 Elsevier B.V.-
dc.language.isoen_US-
dc.publisherElsevier B.V.-
dc.relation.ispartofNuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and Atoms-
dc.subjectHeavy ions-
dc.subjectIonization-
dc.subjectL-shell x-rays-
dc.subjectMultiple-ionization-
dc.titleL x-ray production cross sections in high-Z atoms by 3–5 MeV/u silicon ions-
dc.typeArticle-
dc.scopusid55261958000-
dc.scopusid57202529168-
dc.scopusid57203181883-
dc.scopusid57206930935-
dc.scopusid55450559700-
dc.scopusid7202822333-
dc.scopusid7004231502-
dc.scopusid57196989609-
dc.scopusid6603709853-
dc.affiliationOswal, M., Department of Physics, Dev Samaj College, Sec 45-B, Chandigarh, 160047, India, Department of Physics, Panjab University, Chandigarh, 160014, India-
dc.affiliationKumar, S., Department of Applied Sciences, Chitkara University, Himachal Pradesh, 174103, India-
dc.affiliationSingh, U., Department of Applied Sciences, Chitkara University, Himachal Pradesh, 174103, India, The Marian Smoluchowski Institute of Physics, Jagiellonian University, Lojasiewicza 11, Krakow, 30-348, Poland-
dc.affiliationSingh, G., Department of Physics, Punjabi University, Patiala, Punjab 147002, India-
dc.affiliationSingh, K.P., Department of Physics, Panjab University, Chandigarh, 160014, India-
dc.affiliationMehta, D., Department of Physics, Panjab University, Chandigarh, 160014, India-
dc.affiliationMitnik, D., Instituto de Astronomía y Física del Espacio, CONICET and Universidad de Buenos Aires, Buenos Aires, Argentina-
dc.affiliationMontanari, C.C., Instituto de Astronomía y Física del Espacio, CONICET and Universidad de Buenos Aires, Buenos Aires, Argentina-
dc.affiliationNandi, T., Inter-University Accelerator Centre, JNU New Campus, New Delhi, 110067, India-
dc.description.fundingAuthors acknowledge gratefully G. Lapicki for providing the ECUSAR data. Financial support to Mumtaz Oswal as a research fellow under a research project (KPS) from Department of Science and Technology (DST), New Delhi is highly acknowledged. Another financial support from DST to Sunil Kumar in terms of Young Scientist scheme and a Grant from IUAC, New Delhi in terms of the UF-UP-43302 project are gratefully acknowledged. Authors from Argentina acknowledge the support from CONICET, Agencia Nacional de Promoción Científica y Tecnológica, and Universidad de Buenos Aires. Authors also thank for the service of Pelletron staff for smooth operation of the machine.-
dc.description.correspondingauthorNandi, T.; Inter-University Accelerator Centre, JNU New Campus, India; email: nanditapan@gmail.com-
Appears in Collections:Journal Publications [CY]

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