Are fission tracks in meteorites from super-heavy elements?
- 13 October 1969
- journal article
- Published by Elsevier in Physics Letters B
- Vol. 30 (4), 246-248
- https://doi.org/10.1016/0370-2693(69)90430-4
Abstract
No abstract availableThis publication has 15 references indexed in Scilit:
- The possibility of extinct superheavy elements occurring in meteoritesEarth and Planetary Science Letters, 1969
- Elements 112 to 119: Were They Present in Meteorites?Science, 1969
- Stability of superheavy nuclei and their possible occurrence in naturePhysics Letters B, 1969
- Identification of Pu244 fission tracks and the cooling of the parent body of the Toluca meteoriteGeochimica et Cosmochimica Acta, 1968
- Closed shells for Z > 82 and N > 126 in a diffuse potential wellPhysics Letters, 1966
- Additional evidence of stability of the superheavy element 310126 according to the shell modelPhysics Letters, 1966
- Spontaneous fission tracks from extinct Pu244in meteorites and the early history of the solar systemJournal of Geophysical Research, 1965
- Fissiogenic xenon from the Pasamonte meteoriteJournal of Geophysical Research, 1965
- Origin, age, and composition of meteoritesSpace Science Reviews, 1964
- Determination of the Age of the ElementsPhysical Review Letters, 1960