Zobrazeno 1 - 10
of 33
pro vyhledávání: '"Gilardy, G."'
Beyond the acceptance limit of DRAGON: the case of the $\mathrm{^6Li(\alpha,\gamma)^{10}B}$ reaction
Autor:
Psaltis, A., Chen, A. A., Connolly, D. S., Davids, B., Gilardy, G., Giri, R., Greife, U, Huang, W., Hutcheon, D. A., Karpesky, J., Lennarz, A., Liang, J., Paneru, M. Lovely. S. N., Ruiz, C., Tenkila, G., Williams, M.
Radiative capture reactions play a pivotal role for our understanding of the origin of the elements in the cosmos. Recoil separators provide an effective way to study these reactions, in inverse kinematics, and take advantage of the use of radioactiv
Externí odkaz:
http://arxiv.org/abs/2011.01225
Radiative alpha-capture, ($\alpha,\gamma$), reactions play a critical role in nucleosynthesis and nuclear energy generation in a variety of astrophysical environments. The St. George recoil separator at the University of Notre Dame's Nuclear Science
Externí odkaz:
http://arxiv.org/abs/1701.05186
Autor:
Psaltis, A., Chen, A.A., Connolly, D.S., Davids, B., Gilardy, G., Giri, R., Greife, U., Huang, W., Hutcheon, D.A., Karpesky, J., Lennarz, A., Liang, J., Lovely, M., Paneru, S.N., Ruiz, C., Tenkila, G., Williams, M.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 21 January 2021 987
Akademický článek
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Autor:
Frentz, B., Aprahamian, A., Boeltzig, A., Borgwardt, T., Clark, A. M., Deboer, R. J., Gilardy, G., Görres, J., Hanhardt, M., Henderson, S. L., Howard, K. B., Kadlecek, T., Liu, Q., Macon, K. T., Moylan, S., Reingold, C. S., Robertson, D., Seymour, C., Strauss, S. Y., Strieder, F., Vande Kolk, B., Wiescher, M.
Publikováno v:
Physical Review C 106(2022), 065803
The CNO cycle is the main energy source in massive stars during their hydrogen burning phase, and, for our sun, it contributes at the ≈1% level. As the ¹⁴N(p,γ)¹⁵O reaction is the slowest in the cycle, it determines the CNO energy production
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4577::20c491d12b04217050c3dd00d247be76
https://www.hzdr.de/publications/Publ-35974-1
https://www.hzdr.de/publications/Publ-35974-1
Autor:
Fang X., Tan W. P., Beard M., deBoer R. J., Gilardy G., Jung H., Liu Q., Lyons S., Robertson D., Setoodehnia K., Seymour C., Stech E., Vande Kolk B., Wiescher M., de Souza R., Hudan S., Singh V., Tang X. D., Uberseder E.
Publikováno v:
EPJ Web of Conferences, Vol 178, p 04008 (2018)
The total cross sections of the 12C+16O fusion have been experimentally determined at low energies to investigate the role of this reaction during late stellar evolution burning phases. A high-intensity oxygen beam was produced by the 5MV pelletron a
Externí odkaz:
https://doaj.org/article/53d5083c493e4690b3bf7b07b9007718
Autor:
Psaltis, A., Chen, A.A., Connolly, D.S., Davids, B., Gilardy, G., Giri, R., Greife, U., Huang, W., Hutcheon, D.A., Karpesky, J., Lennarz, A., Liang, J., Lovely, M., Paneru, S.N., Ruiz, C., Tenkila, G., Williams, M.
Publikováno v:
Nucl.Instrum.Meth.A
Nucl.Instrum.Meth.A, 2021, 987, pp.164828. ⟨10.1016/j.nima.2020.164828⟩
Nucl.Instrum.Meth.A, 2021, 987, pp.164828. ⟨10.1016/j.nima.2020.164828⟩
Radiative capture reactions play a pivotal role for our understanding of the origin of the elements in the cosmos. Recoil separators provide an effective way to study these reactions, in inverse kinematics, and take advantage of the use of radioactiv
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=arXiv_dedup_::935d89658f8d858b6c003dce141e68f0
https://hal.archives-ouvertes.fr/hal-03022681
https://hal.archives-ouvertes.fr/hal-03022681
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
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K zobrazení výsledku je třeba se přihlásit.
Autor:
Lyons, S., Görres, J., deBoer, R. J., Stech, E., Chen, Y., Gilardy, G., Liu, Q., Long, A. M., Moran, M., Robertson, D., Seymour, C., Vande Kolk, B., Wiescher, M., Best, A.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3730::5a75cf71181c26fb0459247c63ffc5ac
http://hdl.handle.net/11588/721088
http://hdl.handle.net/11588/721088
Autor:
Psaltis, A., Chen, A.A., Connolly, D.S., Davids, B., Esker, N., Gilardy, G., Greife, Uwe, Huang, W., Hutcheon, D.A., Karpesky, J., Lennarz, A., Liang, J., Lovely, M., Paneru, S.N., Giri, R., Ruiz, C., Tenkila, G., Wen, A., Williams, M.
Publikováno v:
Springer Proc.Phys.
15th International Symposium on Nuclei in the Cosmos
15th International Symposium on Nuclei in the Cosmos, Jun 2018, Assergi, Italy. pp.425-428, ⟨10.1007/978-3-030-13876-9_81⟩
15th International Symposium on Nuclei in the Cosmos
15th International Symposium on Nuclei in the Cosmos, Jun 2018, Assergi, Italy. pp.425-428, ⟨10.1007/978-3-030-13876-9_81⟩
International audience; The origin of the p-nuclei, has been a long-standing puzzle in nuclear astrophysics. The $\nu $ p-process is a candidate for the production of the light p-nuclei, but it presents high sensitivity to both supernova dynamics and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::3473282abdf2e5388c786ebdeddab483
https://hal.archives-ouvertes.fr/hal-02327773
https://hal.archives-ouvertes.fr/hal-02327773