Study of the 12C +16 O fusion reaction in carbon burning via the Trojan Horse Method

Autor: Oliva A. A., Tumino A., Soic N., Prajapati P. M., Acosta L., Alba R., Barba F., Cherubini S., D’Agata G., Dell’Aquila D., Di Pietro A., Fernandez J.P., Figuera P., Galaviz Redondo D., Guardo L., Gulino M., Hammache F., Jelavic Malenica D., Kiliç A.I., La Cognata M., La Commara M., Lamia L., Lattuada D., Maiolino C., Manicò G., Mazzocco M., Milin M., Nanru Ma, Nurmukhanbetova A., Nurkic D., Palmerini S., Parascandolo T., Pierroutsakou D., Pizzone R.G., Popocovski R., Rapisarda G.G., Romano S., Santonocito D., Sergi M.L., Shotter A., Spartà R., Spiridon A., Trache L., Vukman N., Yamaguchi H.

Publikováno v: EPJ Web of Conferences, Vol 279, p 11015 (2023)

12C +12 C is the main reaction during core and shell carbon burning in massive stars, however, at temperatures higher than 109K when most of the carbon is depleted and its abundance is lower than 16O, the 12C +16 O fusion can also become relevant. Mo

Externí odkaz: https://doaj.org/article/5b9ac92064e548e5934bc79d9585bcb4

Validation of the $^{10}\mathrm{Be}$ Ground-State Molecular Structure Using $^{10}\mathrm{Be}(p,p\alpha)^{6}\mathrm{He}$ Triple Differential Reaction Cross-Section Measurements

Autor: Li, P. J., Beaumel, D., Lee, J., Assié, M., Chen, S., Franchoo, S., Gibelin, J., Hammache, F., Harada, T., Kanada-En'yo, Y., Kubota, Y., Leblond, S., Liang, P. F., Lokotko, T., Lyu, M., Marqués, F. M., Matsuda, Y., Ogata, K., Otsu, H., Rindel, E., Stuhl, L., Suzuki, D., Togano, Y., Tomai, T., Xu, X. X., Yoshida, K., Zenihiro, J., Achouri, N. L., Aumann, T., Baba, H., Cardella, G., Ceruti, S., Stefanescu, A. I., Corsi, A., Frotscher, A., Gao, J., Gillibert, A., Inaba, K., Isobe, T., Kawabata, T., Kitamura, N., Kobayashi, T., Kondo, Y., Kurihara, A., Liu, H. N., Miki, H., Nakamura, T., Obertelli, A., Orr, N. A., Panin, V., Sasano, M., Shimada, T., Sun, Y. L., Tanaka, J., Trache, L., Tudor, D., Uesaka, T., Wang, H., Yamada, H., Yang, Z. H., Yasuda, M.

Publikováno v: Phys. Rev. Lett. 131 (2023) 212501

The cluster structure of the neutron-rich isotope $^{10}$Be has been probed via the $(p,p\alpha)$ reaction at 150 MeV/nucleon in inverse kinematics and in quasifree conditions. The populated states of $^{6}$He residues were investigated through missi

Externí odkaz: http://arxiv.org/abs/2311.13129

The astrophysical S-factor of the direct 18O(p, γ)19F capture by the ANC method

Autor: Burjan V., Hons Z., Kroha V., Mrázek J., Piskoř Š., Mukhamedzhanov A. M., Trache L., Tribble R. E., La Cognata M., Lamia L., Pizzone G. R., Romano S., Spitaleri C., Tumino A.

Publikováno v: EPJ Web of Conferences, Vol 165, p 01007 (2017)

We attempted to determine the astrophysical S-factor of the direct part of the 18O(p, γ)19F capture by the indirect method of asymptotic normalization coefficients (ANC). We measured the differential cross section of the transfer reaction 18O(3He, d

Externí odkaz: https://doaj.org/article/e168a041f3024b198995b1e5b3d7d51f

Horizons: Nuclear Astrophysics in the 2020s and Beyond

Autor: Schatz, H., Reyes, A. D. Becerril, Best, A., Brown, E. F., Chatziioannou, K., Chipps, K. A., Deibel, C. M., Ezzeddine, R., Galloway, D. K., Hansen, C. J., Herwig, F., Ji, A. P., Lugaro, M., Meisel, Z., Norman, D., Read, J. S., Roberts, L. F., Spyrou, A., Tews, I., Timmes, F. X., Travaglio, C., Vassh, N., Abia, C., Adsley, P., Agarwal, S., Aliotta, M., Aoki, W., Arcones, A., Aryan, A., Bandyopadhyay, A., Banu, A., Bardayan, D. W., Barnes, J., Bauswein, A., Beers, T. C., Bishop, J., Boztepe, T., Côté, B., Caplan, M. E., Champagne, A. E., Clark, J. A., Couder, M., Couture, A., de Mink, S. E., Debnath, S., deBoer, R. J., Hartogh, J. den, Denissenkov, P., Dexheimer, V., Dillmann, I., Escher, J. E., Famiano, M. A., Farmer, R., Fisher, R., Fröhlich, C., Frebel, A., Fryer, C., Fuller, G., Ganguly, A. K., Ghosh, S., Gibson, B. K., Gorda, T., Gourgouliatos, K. N., Graber, V., Gupta, M., Haxton, W., Heger, A., Hix, W. R., Ho, W C. G., Holmbeck, E. M., Hood, A. A., Huth, S., Imbriani, G., Izzard, R. G., Jain, R., Jayatissa, H., Johnston, Z., Kajino, T., Kankainen, A., Kiss, G. G., Kwiatkowski, A., La Cognata, M., Laird, A. M., Lamia, L., Landry, P., Laplace, E., Launey, K. D., Leahy, D., Leckenby, G., Lennarz, A., Longfellow, B., Lovell, A. E., Lynch, W. G., Lyons, S. M., Maeda, K., Masha, E., Matei, C., Merc, J., Messer, B., Montes, F., Mukherjee, A., Mumpower, M., Neto, D., Nevins, B., Newton, W. G., Nguyen, L. Q., Nishikawa, K., Nishimura, N., Nunes, F. M., O'Connor, E., O'Shea, B. W., Ong, W-J., Pain, S. D., Pajkos, M. A., Pignatari, M., Pizzone, R. G., Placco, V. M., Plewa, T., Pritychenko, B., Psaltis, A., Puentes, D., Qian, Y-Z., Radice, D., Rapagnani, D., Rebeiro, B. M., Reifarth, R., Richard, A. L., Rijal, N., Roederer, I. U., Rojo, J. S., K, J. S, Saito, Y., Schwenk, A., Sergi, M. L., Sidhu, R. S., Simon, A., Sivarani, T., Skúladóttir, Á., Smith, M. S., Spiridon, A., Sprouse, T. M., Starrfield, S., Steiner, A. W., Strieder, F., Sultana, I., Surman, R., Szücs, T., Tawfik, A., Thielemann, F., Trache, L., Trappitsch, R., Tsang, M. B., Tumino, A., Upadhyayula, S., Martínez, J. O. Valle, Van der Swaelmen, M., Vázquez, C. Viscasillas, Watts, A., Wehmeyer, B., Wiescher, M., Wrede, C., Yoon, J., Zegers, R G. T., Zermane, M. A., Zingale, M.

Nuclear Astrophysics is a field at the intersection of nuclear physics and astrophysics, which seeks to understand the nuclear engines of astronomical objects and the origin of the chemical elements. This white paper summarizes progress and status of

Externí odkaz: http://arxiv.org/abs/2205.07996

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