Cymek said:
mollwollfumble said:
Tau.Neutrino said:
Hydrogen Squeezed Into a Metal, Possibly Solid, Harvard Physicists Say
Squeezed between two pieces of diamond, hydrogen has been transformed into a metallic form believed to exist inside giant planets like Jupiter, scientists reported on Thursday.
More…
sarahs mum said:
Means absolutely nothing to me.
http://www.sciencemag.org/news/2017/01/diamond-vise-turns-hydrogen-metal-potentially-ending-80-year-quest
Means a lot to me. Metallic hydrogen is a major component of planets such as Jupiter and Saturn.
If you go underneath the atmospheres of these two gas giants you find a surface of liquid metal hydrogen.
Another thing about liquid metal hydrogen. You know how white dwarfs are made from “degenerate matter”. Liquid metal hydrogen is an example of “degenerate matter” when it’s cooled sufficiently.
It’s very difficult to make because you require a lot of pressure.
Oh wait. This is solid metallic hydrogen. I hadn’t heard of that, I only know of liquid metallic hydrogen. Can you get solid metallic hydrogen inside giant planets?
We eagerly await final confirmation – or shattering of the diamond anvil cell, whichever comes first.
Would it be extremely dense ?
I’m not sure.
The density depends on the mass. Which doesn’t normally make sense, but does for metallic hydrogen. The greater the mass, the greater the density. This has nothing to do with gravity or pressure, it has to do with the way the Pauli Exclusion Principle works. A white dwarf star has a lot of mass so is extremely dense, this experiment only has a small amount of mass.
In normal atomic matters, the Pauli Exclusion Principle keeps the atoms apart. In metallic hydrogen, the electrons are not attached to the atomic nuclei any more, and so the Pauli repulsion between electron clouds no longer keeps the atomic nuclei apart. So what you get can be denser than, for example, platinum or osmium. The actual density depends on the electrostatic repulsion between the protons.
I don’t see any good pictures of this on the web. I did draw a picture of it myself a couple of years back.
As for a mass of metallic hydrogen this small, I don’t know how dense it would be. Let me check the web.
In 1996, when the first liquid metallic hydrogen was produced, it had a density of 0.6 g/cm^3. That’s a bit lighter than water.
For the present work, they give a density of solid metallic hydrogen of 6.7 * 10^23 atoms per cubic centimetre. Getting out the calculator, that’s close to 40 g/cm^3. Osmium is 22.6 g/cm^3 so this is more dense than normal matter, but only by a factor of 1.8.