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dc.contributor.authorU. Tippawanen_US
dc.contributor.authorS. Pompen_US
dc.contributor.authorA. Atacen_US
dc.contributor.authorB. Bergenwallen_US
dc.contributor.authorJ. Blomgrenen_US
dc.contributor.authorS. Dangtipen_US
dc.contributor.authorA. Hildebranden_US
dc.contributor.authorC. Johanssonen_US
dc.contributor.authorJ. Klugen_US
dc.contributor.authorP. Mermoden_US
dc.contributor.authorL. Nilssonen_US
dc.contributor.authorM. Österlunden_US
dc.contributor.authorK. Elmgrenen_US
dc.contributor.authorN. Olssonen_US
dc.contributor.authorO. Jonssonen_US
dc.contributor.authorA. V. Prokofieven_US
dc.contributor.authorP. U. Renbergen_US
dc.contributor.authorP. Nadel-Turonskien_US
dc.contributor.authorV. Corcalciucen_US
dc.contributor.authorY. Watanabeen_US
dc.contributor.authorA. J. Koningen_US
dc.date.accessioned2018-09-11T09:28:14Z-
dc.date.available2018-09-11T09:28:14Z-
dc.date.issued2005-05-24en_US
dc.identifier.issn15517616en_US
dc.identifier.issn0094243Xen_US
dc.identifier.other2-s2.0-33749460501en_US
dc.identifier.other10.1063/1.1945311en_US
dc.identifier.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=33749460501&origin=inwarden_US
dc.identifier.urihttp://cmuir.cmu.ac.th/jspui/handle/6653943832/62470-
dc.description.abstractRadiation effects induced by terrestrial cosmic rays in microelectronics, on board aircrafts as well as at sea level, have recently attracted much attention. The most important particle radiation is due to spallation neutrons, created in the atmosphere by cosmic-ray protons. When, e.g., an electronic memory circuit is exposed to neutron radiation, charged particles can be produced in a nuclear reaction. The charge released by ionization can cause a flip of the memory content in a bit, which is called a single-event upset (SEU). This induces no hardware damage to the circuit, but unwanted re-programming of memories, CPUs, etc., can have consequences for the reliability, and ultimately also for the safety of the system. Data on energy and angular distributions of the secondary particles produced by neutrons in silicon nuclei are essential input for analyses and calculation of SEU rate. In this work, double-differential cross sections of inclusive light-ion (p, d, t,3He and α) production in silicon, induced by 96 MeV neutrons, are presented. Energy distributions are measured at eight laboratory angles from 20° to 160° in steps of 20°. Deduced energy-differential and production cross sections are reported as well. Experimental cross sections are compared to theoretical reaction model calculations and existing experimental data in the literature. © 2005 American Institute of Physics.en_US
dc.subjectPhysics and Astronomyen_US
dc.titleLight-ion production in the interaction of 96 MeV neutrons with siliconen_US
dc.typeConference Proceedingen_US
article.title.sourcetitleAIP Conference Proceedingsen_US
article.volume769en_US
article.stream.affiliationsUppsala Universiteten_US
article.stream.affiliationsChiang Mai Universityen_US
article.stream.affiliationsTotalforsvarets forskningsinstituten_US
article.stream.affiliationsSvedberg Laboratoryen_US
article.stream.affiliationsInstitute of Atomic Physics, Bucharesten_US
article.stream.affiliationsKyushu Universityen_US
article.stream.affiliationsThe Nuclear Research & Consultancy Groupen_US
article.stream.affiliationsGeorge Washington Universityen_US
Appears in Collections:CMUL: Journal Articles

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