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Related: About this forumU.S. back in race to forge unknown, superheavy elements
From the current issue of Science:
U.S. back in race to forge unknown, superheavy elements
Subtitle:
Robert Service, Science, July 23, 2024
The caption:
Some excerpts:
...From 1936 through 1976, LBNL used its atom smashers to discover 16 elements, from element 43 (technetium) to 106 (seaborgium). But in the decades that followed the axis of superheavy research shifted to facilities in Germany, Japan, and Russia, which collectively discovered the last 12 elements...
...In principle, synthesizing superheavy elements is simple. Researchers fire beams of ions of a lighter element into a thin target of a heavier element and hope the two nuclei fuse. The most recent superheavies, 114 through 118, were discovered using a beam of calcium-48, whose magic number of protons and neutrons lend it stability and a higher probability of merging with target nuclei. But that approach concluded with calcium ions fusing with californium to produce element 118, because elements heavier than californium cannot be made in large enough quantities for viable targets. So, physicists began firing beams of heavier but less stable ions, such as titanium and chromium...
...LBNLs new titanium beam is more powerful, generating some 6 trillion ions per second. It begins with a ceramic oven the size of a peanut that vaporizes titanium at temperatures of 1800°C. The atoms are confined by superconducting magnets that must be cooled to near absolute zero. Microwaves strip away about half of each atoms electrons, creating ions that are injected into a cyclotron that accelerates them to 11% the speed of light. They are then fired at a plutonium disk, which spins 30 times per second to help dissipate the heat of the collisions...
Elements 119 and 120 would start a new period in the periodic table.
getagrip_already
(17,182 posts)For a molecule of hamburgium today.
Arne
(3,568 posts)eppur_se_muova
(37,325 posts)NNadir
(34,487 posts)I seem to recall, though I don't have a reference, that Californium has been detected either in stars or in supernovae. I would expect that in the r-process, particularly in the presence of heavy elements traveling at relativistic speeds albeit with very short free mean paths, some superheavy elements in period 8 occur. Almost certainly they undergo rapid fission or decay, but the rate of formation could be appreciably high.
One wonders where in the periodic table a neutron star would lie.
An argument is often made that at least some of the thorium on this planet is the decay product of 244Pu and, less often, that some of the 235U arrived in the solar system, if not the Earth itself, and 247Cm.
If one wants to get a little weird about it - and I'm prone to that - one can argue that nuclear energy is sort of "solar" since it originates in stars.
eppur_se_muova
(37,325 posts)the dispersal of matter throughout the Universe after the Big Bang. So nuclear energy is really leftover energy (dare I say "fossil" energy?) from the creation of the Universe.
Yes, I've done some thinking about "where does all this energy come from?" but I don't know how anyone takes it back before the Singularity. :^/
I seem to recall that the decay of radiant energy flux from some supernovae has roughly that same half-life as one of the isotopes of Californium, but I don't think a connection was really proven.