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http://hdl.handle.net/11452/25223
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DC Field | Value | Language |
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dc.date.accessioned | 2022-03-21T10:51:02Z | - |
dc.date.available | 2022-03-21T10:51:02Z | - |
dc.date.issued | 2004-08 | - |
dc.identifier.citation | Cengiz, A. ve Almaz, E. (2004). “Internal bremsstrahlung spectra of beta(-) particle emitters using the Monte Carlo method”. Radiation Physics and Chemistry, 70(6), 661-668. | en_US |
dc.identifier.issn | 0969-806X | - |
dc.identifier.uri | https://doi.org/10.1016/j.radphyschem.2004.03.008 | - |
dc.identifier.uri | http://hdl.handle.net/11452/25223 | - |
dc.description.abstract | A Monte Carlo code has been developed which obtains internal bremsstrahlung (IB) spectra accompanying beta(-) particles of beta(-) particle emitters. For the IB spectra of beta(-) particle emitters, a simple formula has been also proposed by using the theory of Knipp, Uhlenbeck and Bloch (KUB). The IB spectra of P-32(15), Rb-86(37), Sr-89(38), Sr-90(38), Y-90(39), Tc-99(43) Tm-170(69) and W-185(74) obtained by using this code and the KUB theory were compared with experiments. | en_US |
dc.language.iso | en | en_US |
dc.publisher | Pergamon-Elsevier Science | en_US |
dc.rights | info:eu-repo/semantics/closedAccess | en_US |
dc.subject | Chemistry | en_US |
dc.subject | Nuclear science and technology | en_US |
dc.subject | Physics | en_US |
dc.subject | Elementary particles | en_US |
dc.subject | Internal bremsstrahlung spectrum | en_US |
dc.subject | Beta(-) particle spectrum | en_US |
dc.subject | Monte Carlo method | en_US |
dc.subject | Beta-decay | en_US |
dc.subject | SR-89 | en_US |
dc.subject | Region | en_US |
dc.subject | Range | en_US |
dc.subject | S-35 | en_US |
dc.subject | Monte Carlo methods | en_US |
dc.subject | Phosphorus | en_US |
dc.subject | Rubidium | en_US |
dc.subject | Spectrum analysis | en_US |
dc.subject | Strontium | en_US |
dc.subject | Internal bremsstrahlung (IB) spectra | en_US |
dc.subject | Particle emitters | en_US |
dc.title | Internal bremsstrahlung spectra of beta(-) particle emitters using the Monte Carlo method | en_US |
dc.type | Article | en_US |
dc.identifier.wos | 000221898800001 | tr_TR |
dc.identifier.scopus | 2-s2.0-2442591781 | tr_TR |
dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi | tr_TR |
dc.contributor.department | Uludağ Üniversitesi/Fen-Edebiyat Fakültesi/Fizik Bölümü. | tr_TR |
dc.contributor.orcid | 0000-0002-8708-2189 | tr_TR |
dc.identifier.startpage | 661 | tr_TR |
dc.identifier.endpage | 668 | tr_TR |
dc.identifier.volume | 70 | tr_TR |
dc.identifier.issue | 6 | tr_TR |
dc.relation.journal | Radiation Physics and Chemistry | en_US |
dc.contributor.buuauthor | Cengiz, Ahmet | - |
dc.contributor.buuauthor | Almaz, Ekrem | - |
dc.contributor.researcherid | AAH-7446-2021 | tr_TR |
dc.contributor.researcherid | C-3437-2019 | tr_TR |
dc.subject.wos | Chemistry, physical | en_US |
dc.subject.wos | Nuclear science and technology | en_US |
dc.subject.wos | Physics, atomic, molecular and chemical | en_US |
dc.indexed.wos | SCIE | en_US |
dc.indexed.scopus | Scopus | en_US |
dc.wos.quartile | Q3 (Chemistry, physical) | en_US |
dc.wos.quartile | Q2 (Nuclear science & technology) | en_US |
dc.wos.quartile | Q4 Physics, atomic, molecular & chemical) | en_US |
dc.contributor.scopusid | 18534116600 | tr_TR |
dc.contributor.scopusid | 18533626200 | tr_TR |
dc.subject.emtree | Phosphorus 32 | en_US |
dc.subject.emtree | Radioisotope | en_US |
dc.subject.emtree | Rubidium 86 | en_US |
dc.subject.emtree | Strontium 89 | en_US |
dc.subject.emtree | Technetium 99m | en_US |
dc.subject.emtree | Thulium | en_US |
dc.subject.emtree | Yttrium 90 | en_US |
dc.subject.emtree | Article | en_US |
dc.subject.emtree | Brems radiation | en_US |
dc.subject.emtree | Electron | en_US |
dc.subject.emtree | Mathematical computing | en_US |
dc.subject.emtree | Monte Carlo method | en_US |
dc.subject.emtree | Radiation physics | en_US |
dc.subject.emtree | Theoretical model | en_US |
Appears in Collections: | Scopus Web of Science |
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