M. Peoviti, N. Patronis, M. Axiotis, V. Foteinou, D. Rogalla, Fotios Maragkos, S. Harissopulos
{"title":"核子天体物理学研究63Cu(α，γ)67Ga反应的第一个结果","authors":"M. Peoviti, N. Patronis, M. Axiotis, V. Foteinou, D. Rogalla, Fotios Maragkos, S. Harissopulos","doi":"10.12681/hnpsanp.5091","DOIUrl":null,"url":null,"abstract":"The 63Cu(α,γ)67Ga reaction cross-section was measured in the energy range between 5 and 9 MeV, which is relevant to p-process nucleosynthesis. The experiment was conducted at the Dynamitron Tandem Laboratory, of the Ruhr-University Bochum in Germany, by applying the 4π γ-summing method, using a 12\"×12\" NaI(Tl) single crystal scintillator. The preliminary results are compared with previous measurements and theoretical TALYS calculations as well.","PeriodicalId":262803,"journal":{"name":"HNPS Advances in Nuclear Physics","volume":"45 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2023-05-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"First results from the 63Cu(α,γ)67Ga reaction study for nuclear astrophysics purposes\",\"authors\":\"M. Peoviti, N. Patronis, M. Axiotis, V. Foteinou, D. Rogalla, Fotios Maragkos, S. Harissopulos\",\"doi\":\"10.12681/hnpsanp.5091\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The 63Cu(α,γ)67Ga reaction cross-section was measured in the energy range between 5 and 9 MeV, which is relevant to p-process nucleosynthesis. The experiment was conducted at the Dynamitron Tandem Laboratory, of the Ruhr-University Bochum in Germany, by applying the 4π γ-summing method, using a 12\\\"×12\\\" NaI(Tl) single crystal scintillator. The preliminary results are compared with previous measurements and theoretical TALYS calculations as well.\",\"PeriodicalId\":262803,\"journal\":{\"name\":\"HNPS Advances in Nuclear Physics\",\"volume\":\"45 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2023-05-05\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"HNPS Advances in Nuclear Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.12681/hnpsanp.5091\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"HNPS Advances in Nuclear Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.12681/hnpsanp.5091","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
First results from the 63Cu(α,γ)67Ga reaction study for nuclear astrophysics purposes
The 63Cu(α,γ)67Ga reaction cross-section was measured in the energy range between 5 and 9 MeV, which is relevant to p-process nucleosynthesis. The experiment was conducted at the Dynamitron Tandem Laboratory, of the Ruhr-University Bochum in Germany, by applying the 4π γ-summing method, using a 12"×12" NaI(Tl) single crystal scintillator. The preliminary results are compared with previous measurements and theoretical TALYS calculations as well.
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