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 |