Explore Superheavy Elements & Their Uses

  • Thread starter Thread starter sanman
  • Start date Start date
  • Tags Tags
    Elements
sanman
Messages
737
Reaction score
24
Stable SuperHeavy Elements

I'd read that a new "island of stability" of long-lived SuperHeavy elements is about to be reached.

http://en.wikipedia.org/wiki/Island_of_stability

The recent synthesis of Hassium-270 showed a surprisingly pleasant half-life of 30 seconds. That's pretty fabulous for something that has an atomic number of 108. These nifty long half-lives are due to the proximity to the ever-important magic numbers for nuclear stability.

The Superheavy element Unbihexium-310, having atomic number 126, is predicted to have a half-life of millions of years, due to its being "doubly magic" because of the closed neutron and proton shells.

http://en.wikipedia.org/wiki/Unbihexium

I wonder what novel scientific or engineering applications could benefit from a Superheavy element such as this? Radiation shielding, due to its larger nucleus? Perhaps quantum computing or superconductivity?

If they ever have to come up with a formal name for Unbihexium, I would recommend the name "Lexium" as an homage to the fictional mad scientist who is Superman's arch-enemy. And this is because atomic number 126 was designated by Action Comics as the atomic number for Kryptonite, which is dangerous to Superman.
 
Last edited:
Physics news on Phys.org
sanman said:
If they ever have to come up with a formal name for Unbihexium, I would recommend the name "Lexium" as an homage to the fictional mad scientist who is Superman's arch-enemy. And this is because atomic number 126 was designated by Action Comics as the atomic number for Kryptonite, which is dangerous to Superman.
I second that!

It would be amazing if we could synthesize elements with higer atomic numbers, surely they will have interesting properties.
 
Thread 'Why is there such a difference between the total cross-section data? (simulation vs. experiment)'
Well, I'm simulating a neutron-proton scattering phase shift. The equation that I solve numerically is the Phase function method and is $$ \frac{d}{dr}[\delta_{i+1}] = \frac{2\mu}{\hbar^2}\frac{V(r)}{k^2}\sin(kr + \delta_i)$$ ##\delta_i## is the phase shift for triplet and singlet state, ##\mu## is the reduced mass for neutron-proton, ##k=\sqrt{2\mu E_{cm}/\hbar^2}## is the wave number and ##V(r)## is the potential of interaction like Yukawa, Wood-Saxon, Square well potential, etc. I first...
Toponium is a hadron which is the bound state of a valance top quark and a valance antitop quark. Oversimplified presentations often state that top quarks don't form hadrons, because they decay to bottom quarks extremely rapidly after they are created, leaving no time to form a hadron. And, the vast majority of the time, this is true. But, the lifetime of a top quark is only an average lifetime. Sometimes it decays faster and sometimes it decays slower. In the highly improbable case that...
Back
Top