M. Hall, D. Bardayan, S. Ahn, J. Allen, J. T. Anderson, A. D. Ayangeakaa, T. Baugher, J. Blackmon, D. Blankstein, S. Burcher, M. Carpenter, S. Cha, K. Chae, K. Chipps, J. Cizewski, M. Febbraro, B. Frentz, O. Hall, S. Henderson, J. Hu, C. Jiang, K. Jones, E. J. Lee, A. Lepailleur, D. S. Monteiro, P. O’Malley, S. Ota, S. Pain, B. Rasco, A. Ratkiewicz, J. Riggins, D. Santiago-Gonzalez, D. Seweryniak, A. Simon, H. Sims, Karl Smith, W. Tan, P. Thompson, C. Thornsberry, R. Torres-Isea, B. V. Kolk, R. Varner, D. Walter, G. Wilson, S. Zhu
{"title":"使用19F(3He,t)19Ne*(γ)来研究18F+p阈值附近的天体物理重要水平","authors":"M. Hall, D. Bardayan, S. Ahn, J. Allen, J. T. Anderson, A. D. Ayangeakaa, T. Baugher, J. Blackmon, D. Blankstein, S. Burcher, M. Carpenter, S. Cha, K. Chae, K. Chipps, J. Cizewski, M. Febbraro, B. Frentz, O. Hall, S. Henderson, J. Hu, C. Jiang, K. Jones, E. J. Lee, A. Lepailleur, D. S. Monteiro, P. O’Malley, S. Ota, S. Pain, B. Rasco, A. Ratkiewicz, J. Riggins, D. Santiago-Gonzalez, D. Seweryniak, A. Simon, H. Sims, Karl Smith, W. Tan, P. Thompson, C. Thornsberry, R. Torres-Isea, B. V. Kolk, R. Varner, D. Walter, G. Wilson, S. Zhu","doi":"10.1063/1.5127732","DOIUrl":null,"url":null,"abstract":"A direct test of nova explosion models comes from the observation of γ rays created in the decay of radioactive isotopes produced in the nova. One such isotope, 18F, is believed to be the main source of observable γ rays at and below 511 keV. The main destruction mechanism of 18F is thought to be the 18F(p,α)15O reaction, and uncertainties in the reaction rate arise from uncertainties in the energies, spins, and parities of the nuclear levels in 19Ne above the 18F+p threshold. To measure the properties of these levels, the 19F(3He,t)19Ne∗(γ) reaction was studied at Argonne National Laboratory and the Nuclear Science Laboratory at the University of Notre Dame.A direct test of nova explosion models comes from the observation of γ rays created in the decay of radioactive isotopes produced in the nova. One such isotope, 18F, is believed to be the main source of observable γ rays at and below 511 keV. The main destruction mechanism of 18F is thought to be the 18F(p,α)15O reaction, and uncertainties in the reaction rate arise from uncertainties in the energies, spins, and parities of the nuclear levels in 19Ne above the 18F+p threshold. To measure the properties of these levels, the 19F(3He,t)19Ne∗(γ) reaction was studied at Argonne National Laboratory and the Nuclear Science Laboratory at the University of Notre Dame.","PeriodicalId":141750,"journal":{"name":"25TH INTERNATIONAL CONFERENCE ON THE APPLICATION OF ACCELERATORS IN RESEARCH AND INDUSTRY","volume":"418 ","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2019-10-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"Using 19F(3He,t)19Ne*(γ) to study astrophysically important levels near the 18F+p threshold\",\"authors\":\"M. Hall, D. Bardayan, S. Ahn, J. Allen, J. T. Anderson, A. D. Ayangeakaa, T. Baugher, J. Blackmon, D. Blankstein, S. Burcher, M. Carpenter, S. Cha, K. Chae, K. Chipps, J. Cizewski, M. Febbraro, B. Frentz, O. Hall, S. Henderson, J. Hu, C. Jiang, K. Jones, E. J. Lee, A. Lepailleur, D. S. Monteiro, P. O’Malley, S. Ota, S. Pain, B. Rasco, A. Ratkiewicz, J. Riggins, D. Santiago-Gonzalez, D. Seweryniak, A. Simon, H. Sims, Karl Smith, W. Tan, P. Thompson, C. Thornsberry, R. Torres-Isea, B. V. Kolk, R. Varner, D. Walter, G. Wilson, S. Zhu\",\"doi\":\"10.1063/1.5127732\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"A direct test of nova explosion models comes from the observation of γ rays created in the decay of radioactive isotopes produced in the nova. One such isotope, 18F, is believed to be the main source of observable γ rays at and below 511 keV. The main destruction mechanism of 18F is thought to be the 18F(p,α)15O reaction, and uncertainties in the reaction rate arise from uncertainties in the energies, spins, and parities of the nuclear levels in 19Ne above the 18F+p threshold. 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Using 19F(3He,t)19Ne*(γ) to study astrophysically important levels near the 18F+p threshold
A direct test of nova explosion models comes from the observation of γ rays created in the decay of radioactive isotopes produced in the nova. One such isotope, 18F, is believed to be the main source of observable γ rays at and below 511 keV. The main destruction mechanism of 18F is thought to be the 18F(p,α)15O reaction, and uncertainties in the reaction rate arise from uncertainties in the energies, spins, and parities of the nuclear levels in 19Ne above the 18F+p threshold. To measure the properties of these levels, the 19F(3He,t)19Ne∗(γ) reaction was studied at Argonne National Laboratory and the Nuclear Science Laboratory at the University of Notre Dame.A direct test of nova explosion models comes from the observation of γ rays created in the decay of radioactive isotopes produced in the nova. One such isotope, 18F, is believed to be the main source of observable γ rays at and below 511 keV. The main destruction mechanism of 18F is thought to be the 18F(p,α)15O reaction, and uncertainties in the reaction rate arise from uncertainties in the energies, spins, and parities of the nuclear levels in 19Ne above the 18F+p threshold. To measure the properties of these levels, the 19F(3He,t)19Ne∗(γ) reaction was studied at Argonne National Laboratory and the Nuclear Science Laboratory at the University of Notre Dame.
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