Australian and US physicists say they have calculated the speed of the most complex nuclear reactions and found that they’re, well, really fast. We’re talking as little as zeptoseconds – a billionth of a trillionth of a second (10-21).
The finding follows a comprehensive project to calculate detailed models of the energy flow during nuclear collisions.
Cedric Simenel from the Australian National University worked with Kyle Godbey and Sait Umar from Vanderbilt University to model 13 different pairs of nuclei, using supercomputers at ANU and in the US.
In all they calculated 600 different collisions, from head-on to just grazing past each other. In some cases colliding particles stuck, in others they bounced off each other or adhered briefly (zeptosecond briefly) before separating.
Even at such speed, a number of processes take place, the researchers say.
First, the protons and neutrons swap between the newly-united fragments, in order to equalise their neutron-to-proton ratio. Known as charge equilibration, the calculations showed this is the fastest process, taking only one zeptosecond.
On similar time scale, the kinetic (movement) energy of the nuclei and their angular momentum (rotation) get converted to internal heat, a process known as dissipation.
However, a third process was much slower than the others. The mass equilibration process, in which the shape changes, as protons and neutrons flow from the larger fragment to the smaller one, was up to 20 times slower than the other mechanisms.
“This shows that the mass equilibration process is driven by a different mechanism which has little to do with the other processes,” Simenel says.
It was surprising to find, he adds, that the equilibration times are the same no matter the size of the nuclei. “The time is universal; they will be the same if we are colliding a uranium with a carbon, an iron with a lead, or a calcium with a zinc.”
A feature of the calculations is that they can be compared with measurable experimental quantities, and the ANU’s David Hinde, who was not a part of this project, suggests they could help efforts to add new elements to the periodic table.
“These time scales determine how we can picture the sequence of processes as two heavy nuclei move towards equilibration during superheavy element synthesis reactions,” he says
“This understanding will help to predict the best reactions to use to create and study the properties of new, even heavier, synthetic elements.”
The findings are reported in the journal Physical Review Letters.
Curated content from the editorial staff at Cosmos Magazine.
Read science facts, not fiction...
There’s never been a more important time to explain the facts, cherish evidence-based knowledge and to showcase the latest scientific, technological and engineering breakthroughs. Cosmos is published by The Royal Institution of Australia, a charity dedicated to connecting people with the world of science. Financial contributions, however big or small, help us provide access to trusted science information at a time when the world needs it most. Please support us by making a donation or purchasing a subscription today.