Cargando…
Abundance of live (244)Pu in deep-sea reservoirs on Earth points to rarity of actinide nucleosynthesis
Half of the heavy elements including all actinides are produced in r-process nucleosynthesis, whose sites and history remain a mystery. If continuously produced, the Interstellar Medium is expected to build-up a quasi-steady state of abundances of short-lived nuclides (with half-lives ≤100 My), incl...
Autores principales: | Wallner, A., Faestermann, T., Feige, J., Feldstein, C., Knie, K., Korschinek, G., Kutschera, W., Ofan, A., Paul, M., Quinto, F., Rugel, G., Steier, P. |
---|---|
Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Pub. Group
2015
|
Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4309418/ https://www.ncbi.nlm.nih.gov/pubmed/25601158 http://dx.doi.org/10.1038/ncomms6956 |
Ejemplares similares
-
First measurements of the total and partial stellar neutron cross sections to the s-process branching-point $^{79}Se$
por: Dillmann, I, et al.
Publicado: (2006) -
Future radioisotope measurements to clarify the origin of deep-ocean 244Pu
por: Wang, Xilu, et al.
Publicado: (2021) -
Recent near-Earth supernovae probed by global deposition of interstellar radioactive (60)Fe
por: Wallner, A., et al.
Publicado: (2016) -
The supernova-nucleosynthesis $^{40}Ca(\alpha, \gamma)^{44}Ti$ reaction
por: Nassar, H, et al.
Publicado: (2006) -
Study of Photon Strength Functions of Actinides: the case of U-235, Np-238 and Pu-241
por: Guerrero, C, et al.
Publicado: (2010)