مؤتمر
Experimental Study of the ${^{30}}{\text {P}({\text {p}}}{,}{\gamma })^{31}\text {S}$ Reaction in Classical Novae
| العنوان: | Experimental Study of the ${^{30}}{\text {P}({\text {p}}}{,}{\gamma })^{31}\text {S}$ Reaction in Classical Novae |
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| المؤلفون: | Meyer, A., de Séréville, N., Hammache, F., Adsley, P., Parikh, A., Assié, M., Assunção, M., Bastin, B., Beaumel, D., Béroff, K., Coc, Alain, d'Agata, G., Delafosse, C., de Oliveira, F., Flavigny, F., Fox, S.P., Georgiadou, A., Gottardo, A., Grassi, L., Guillot, J., Guimaräes, V., Hubbard, N., Id Barkach, T., Kiener, J., Laird, A.M., Lara, A.L., Maccormick, M., Matea, I., Olivier, L., Oulebsir, N., Perrot, L., Portail, C., Riley, J., Sanchez Benitez, A.M., Stefan, I., Tatischeff, V. |
| المساهمون: | Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Grand Accélérateur National d'Ions Lourds (GANIL), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut des Sciences Moléculaires d'Orsay (ISMO), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM) |
| المصدر: | Springer Proc.Phys. ; 15th International Symposium on Nuclei in the Cosmos ; https://hal.science/hal-02317359Test ; 15th International Symposium on Nuclei in the Cosmos, Jun 2018, Assergi, Italy. pp.195-200, ⟨10.1007/978-3-030-13876-9_32⟩ |
| بيانات النشر: | HAL CCSD |
| سنة النشر: | 2018 |
| مصطلحات موضوعية: | [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] |
| جغرافية الموضوع: | Assergi, Italy |
| الوصف: | International audience ; The$^{30}$ P(p, $\gamma $ )$^{31}$ S reaction is one of the few remaining reactions whose rate uncertainty has a strong impact on classical novae model predictions. To reduce the nuclear uncertainties associated to this reaction, we measured the$^{31}$ P($^{3}$ He,t)$^{31}$ S reaction at the ALTO facility. Simultaneous detection of the triton and proton decays from the populated resonances will provide the proton branching ratios. The astrophysical context of this work, the current situation of the$^{30}$ P(p, $\gamma $ )$^{31}$ S reaction rate, the experimental set-up and the analysis of the single and coincidence events will be presented. |
| نوع الوثيقة: | conference object |
| اللغة: | English |
| العلاقة: | hal-02317359; https://hal.science/hal-02317359Test; INSPIRE: 1751509 |
| DOI: | 10.1007/978-3-030-13876-9_32 |
| الإتاحة: | https://doi.org/10.1007/978-3-030-13876-9_32Test https://hal.science/hal-02317359Test |
| رقم الانضمام: | edsbas.E151BF4B |
| قاعدة البيانات: | BASE |
| DOI: | 10.1007/978-3-030-13876-9_32 |
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