M. Guttormsen, A. Larsen, J. E. Midtbø, L. C. Campo, A. Görgen, V. W. Ingeberg, T. Renstrøm, S. Siem, G. Tveten, F. Zeiser, L. Kirsch
{"title":"核准连续体的伽马宽度,寿命和波动","authors":"M. Guttormsen, A. Larsen, J. E. Midtbø, L. C. Campo, A. Görgen, V. W. Ingeberg, T. Renstrøm, S. Siem, G. Tveten, F. Zeiser, L. Kirsch","doi":"10.1051/epjconf/201817806001","DOIUrl":null,"url":null,"abstract":"Statistical $\\gamma$-decay from highly excited states is determined by the nuclear level density (NLD) and the $\\gamma$-ray strength function ($\\gamma$SF). These average quantities have been measured for several nuclei using the Oslo method. For the first time, we exploit the NLD and $\\gamma$SF to evaluate the $\\gamma$-width in the energy region below the neutron binding energy, often called the quasi-continuum region. The lifetimes of states in the quasi-continuum are important benchmarks for a theoretical description of nuclear structure and dynamics at high temperature. The lifetimes may also have impact on reaction rates for the rapid neutron-capture process, now demonstrated to take place in neutron star mergers.","PeriodicalId":8464,"journal":{"name":"arXiv: Nuclear Experiment","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2018-04-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Gamma-widths, lifetimes and fluctuations in the nuclear quasi-continuum\",\"authors\":\"M. Guttormsen, A. Larsen, J. E. Midtbø, L. C. Campo, A. Görgen, V. W. Ingeberg, T. Renstrøm, S. Siem, G. Tveten, F. Zeiser, L. Kirsch\",\"doi\":\"10.1051/epjconf/201817806001\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Statistical $\\\\gamma$-decay from highly excited states is determined by the nuclear level density (NLD) and the $\\\\gamma$-ray strength function ($\\\\gamma$SF). These average quantities have been measured for several nuclei using the Oslo method. For the first time, we exploit the NLD and $\\\\gamma$SF to evaluate the $\\\\gamma$-width in the energy region below the neutron binding energy, often called the quasi-continuum region. The lifetimes of states in the quasi-continuum are important benchmarks for a theoretical description of nuclear structure and dynamics at high temperature. The lifetimes may also have impact on reaction rates for the rapid neutron-capture process, now demonstrated to take place in neutron star mergers.\",\"PeriodicalId\":8464,\"journal\":{\"name\":\"arXiv: Nuclear Experiment\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2018-04-03\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv: Nuclear Experiment\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1051/epjconf/201817806001\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv: Nuclear Experiment","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1051/epjconf/201817806001","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Gamma-widths, lifetimes and fluctuations in the nuclear quasi-continuum
Statistical $\gamma$-decay from highly excited states is determined by the nuclear level density (NLD) and the $\gamma$-ray strength function ($\gamma$SF). These average quantities have been measured for several nuclei using the Oslo method. For the first time, we exploit the NLD and $\gamma$SF to evaluate the $\gamma$-width in the energy region below the neutron binding energy, often called the quasi-continuum region. The lifetimes of states in the quasi-continuum are important benchmarks for a theoretical description of nuclear structure and dynamics at high temperature. The lifetimes may also have impact on reaction rates for the rapid neutron-capture process, now demonstrated to take place in neutron star mergers.