https://www.futurity.org/plasma-liquid-metal-physics-2003862/
All ultra dense metals including hydrogen and water retain quantum behavior up to 90,000F This supports the idea that compressed matter is a heat source inside planets and other smaller bodies. On Tue, Mar 26, 2019 at 3:53 PM bobcook39...@hotmail.com < bobcook39...@hotmail.com> wrote: > I tend to agree that the cores of these heated planets and various moons > are pretty mysterious. I do not consider that pressure, temperature, > clculations will indicate much abouf the physical reality happenning in > macroscopic coherent systems that exist in the cores. > > > > Until the magnetic and electric together with gravitational potential and > kinetic energies for the quasi stable system is understood, the mysterious > characteristics of the mysterious cores will remain mysterious. > Evaluating coherent systems with classical pressure/temperatures models > that roughly work with chemically bound macroscopic systems > > will not do much for validation of physical models of those cores. > > > > Bob Cook > > > > --------------------------------------- > ------------------------------ > *From:* JonesBeene <jone...@pacbell.net> > *Sent:* Monday, March 25, 2019 2:32:47 PM > *To:* vortex-l@eskimo.com > *Subject:* RE: [Vo]:deuterium transition pressure to metalized forms > > > Jupiter has a mysterious internal heat source which is not based on > nuclear fission. > > > > The core of the planet is extremely hot but not enough for nuclear fusion > either. > > > > The heat source cannot be leftover from planetary formation as it is far > too intense. > > > > There are many conjectures about the source of heat since all the usual > suspects can be ruled out. > > > > It is therefore possible if not likely that ultradense hydrogen in > somehow involved. > > > > Well, I suppose that is why you posted it <g>. > > > > > > > > > > *From: *Axil Axil <janap...@gmail.com> > > > > http://science.sciencemag.org/content/361/6403/677 > > > > Insulator-metal transition in dense fluid deuterium > > > Abstract > > Dense fluid metallic hydrogen occupies the interiors of Jupiter, Saturn, > and many extrasolar planets, where pressures reach millions of atmospheres. > Planetary structure models must describe accurately the transition from the > outer molecular envelopes to the interior metallic regions. We report > optical measurements of dynamically compressed fluid deuterium to 600 > gigapascals (GPa) that reveal an increasing refractive index, the onset of > absorption of visible light near 150 GPa, and a transition to metal-like > reflectivity (exceeding 30%) near 200 GPa, all at temperatures below 2000 > kelvin. Our measurements and analysis address existing discrepancies > between static and dynamic experiments for the insulator-metal transition > in dense fluid hydrogen isotopes. They also provide new benchmarks for the > theoretical calculations used to construct planetary models. > > > > The article is questioned here > > > > http://science.sciencemag.org/content/363/6433/eaaw0969 > > > > The transition pressure to melalize deutriem is lower that expected from > first principle calculations. That meltaliation transition pressure is > measured to occur at 2,000,000 Bar. > > > > For comment on the critique see > > > > http://science.sciencemag.org/content/363/6433/eaaw1970 > > >
