دورية أكاديمية

Measurement of the $^{140}Ce ( n , γ )$ Cross Section at n_TOF and Its Astrophysical Implications for the Chemical Evolution of the Universe

التفاصيل البيبلوغرافية
العنوان: Measurement of the $^{140}Ce ( n , γ )$ Cross Section at n_TOF and Its Astrophysical Implications for the Chemical Evolution of the Universe
المؤلفون: n_TOF Collaboration, Amaducci, S., Colonna, N., Cosentino, L., Cristallo, S., Finocchiaro, P., Krtička, M., Massimi, C., Mastromarco, M., Mazzone, A., Maugeri, E. A., Mengoni, A., Roederer, I. U., Straniero, O., Valenta, S., Vescovi, D., Aberle, O., Alcayne, V., Andrzejewski, J., Audouin, L., Babiano-Suarez, V., Bacak, M., Barbagallo, M., Bennett, S., Berthoumieux, E., Billowes, J., Bosnar, D., Brown, A., Busso, M., Caamaño, M., Caballero-Ontanaya, L., Calviño, F., Calviani, M., Cano-Ott, D., Casanovas, A., Cerutti, F., Chiaveri, E., Cortés, G., Cortés-Giraldo, M. A., Damone, L. A., Davies, P. J., Diakaki, M., Dietz, M., Domingo-Pardo, C., Dressler, R., Ducasse, Q., Dupont, E., Durán, I., Eleme, Z., Fernández-Domínguez, B., Ferrari, A., Furman, V., Göbel, K., Garg, R., Gawlik-Ramięga, A., Gilardoni, S., Gonçalves, I. F., González-Romero, E., Guerrero, C., Gunsing, F., Harada, H., Heinitz, S., Heyse, J., Jenkins, D. G., Junghans, A., Käppeler, F., Kadi, Y., Kimura, A., Knapová, I., Kokkoris, M., Kopatch, Y., Kurtulgil, D., Ladarescu, I., Lederer-Woods, C., Leeb, H., Lerendegui-Marco, J., Lonsdale, S. J., Macina, D., Manna, A., Martínez, T., Masi, A., Mastinu, P., Mendoza, E., Michalopoulou, V., Milazzo, P. M., Mingrone, F., Moreno-Soto, J., Musumarra, A., Negret, A., Nolte, R., Ogállar, F., Oprea, A., Patronis, N., Pavlik, A., Perkowski, J., Petrone, C., Piersanti, L., Pirovano, E., Porras, I., Praena, J., Quesada, J. M., Ramos-Doval, D., Rauscher, T., Reifarth, R., Rochman, D., Rubbia, C., Sabaté-Gilarte, M., Saxena, A., Schillebeeckx, P., Schumann, D., Sekhar, A., Smith, A. G., Sosnin, N. V., Sprung, P., Stamatopoulos, A., Tagliente, G., Tain, J. L., Tarifeño-Saldivia, A., Tassan-Got, L., Thomas, Th, Torres-Sánchez, P., Tsinganis, A., Ulrich, J., Urlass, S., Vannini, G., Variale, V., Vaz, P., Ventura, A., Vlachoudis, V., Vlastou, R., Wallner, A., Woods, P. J., Wright, T., Žugec, P.
المصدر: Physical Review Letters, 132 (12), Art.-Nr.: 122701 ; ISSN: 0031-9007, 1092-0145, 1079-7114
بيانات النشر: American Physical Society
سنة النشر: 2024
المجموعة: KITopen (Karlsruhe Institute of Technologie)
مصطلحات موضوعية: ddc:530, Physics, info:eu-repo/classification/ddc/530
الوصف: $^{140}Ce(n,γ)$ is a key reaction for slow neutron-capture ($s$-process) nucleosynthesis due to being a bottleneck in the reaction flow. For this reason, it was measured with high accuracy (uncertainty ≈5%) at the n_TOF facility, with an unprecedented combination of a high purity sample and low neutron-sensitivity detectors. The measured Maxwellian averaged cross section is up to 40% higher than previously accepted values. Stellar model calculations indicate a reduction around 20% of the s-process contribution to the Galactic cerium abundance and smaller sizeable differences for most of the heavier elements. No variations are found in the nucleosynthesis from massive stars.
نوع الوثيقة: article in journal/newspaper
وصف الملف: application/pdf
اللغة: English
العلاقة: info:eu-repo/semantics/altIdentifier/issn/0031-9007; info:eu-repo/semantics/altIdentifier/issn/1092-0145; info:eu-repo/semantics/altIdentifier/issn/1079-7114; https://publikationen.bibliothek.kit.edu/1000169990Test; https://publikationen.bibliothek.kit.edu/1000169990/152724774Test; https://doi.org/10.5445/IR/1000169990Test
DOI: 10.5445/IR/1000169990
الإتاحة: https://doi.org/10.5445/IR/1000169990Test
https://doi.org/10.1103/PhysRevLett.132.122701Test
https://publikationen.bibliothek.kit.edu/1000169990Test
https://publikationen.bibliothek.kit.edu/1000169990/152724774Test
حقوق: https://creativecommons.org/licenses/by/4.0/deed.deTest ; info:eu-repo/semantics/openAccess
رقم الانضمام: edsbas.61769168
قاعدة البيانات: BASE