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pro vyhledávání: '"Jain R"'
Autor:
Randhawa, J. S., Kanungo, R., Refsgaard, J., Mohr, P., Ahn, T., Alcorta, M., Andreoiu, C., Bhattacharjee, S. S., Davids, B., Christian, G., Chen, A. A., Coleman, R., Garrett, P., Grinyer, G. F., Fuakye, E. Gyabeng, Hackman, G., Jain, R., Kapoor, K., Kr��cken, R., Laffoley, A., Lennarz, A., Liang, J., Meisel, Z., Nikhil, N., Psaltis, A., Radich, A., Rocchini, M., Saei, N., Saxena, M., Singh, M., Svensson, C., Subramaniam, P., Talebitaher, A., Upadhyayula, S., Waterfield, C., Williams, J., Williams, M.
Reactions on the proton-rich nuclides drive the nucleosynthesis in Core-Collapse Supernovae (CCSNe) and in X-ray bursts (XRBs). CCSNe eject the nucleosynthesis products to the interstellar medium and hence are a potential inventory of p-nuclei, where
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::94bb019f842f7535d535245f03de9249
Autor:
Hamaker, A., Leistenschneider, E., Jain, R., Bollen, G., Giuliani, S. A., Lund, K., Nazarewicz, W., Neufcourt, L., Nicoloff, C., Puentes, D., Ringle, R., Sumithrarachchi, C. S., Yandow, I. T.
Protons and neutrons in the atomic nucleus move in shells analogous to the electronic shell structures of atoms. Nuclear shell structure varies across the nuclear landscape due to changes of the nuclear mean field with the number of neutrons $N$ and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7b728c8334560e877b9d4b0b1b609b15