Don't blame me for yet another lengthy post -- you're the one who keeps asking tough questions!
Lloyd wrote:When you started discussing your C.I. Electric Sun model, I remember you saying at that time that you got your idea for CI from some scientist, whose name I forget (something like Robitaille?).
Robitaille is worth studying in detail, as is Aspden, for the valuable work that they have done on a variety of related topics. But as concerns just the issue of compressive ionization, here is a good example, with the full abstract (since it's so central to the topics at hand).
Saumon, D.; Chabrier, G., 1992: Fluid hydrogen at high density: Pressure ionization. Physical Review A, 46 (4): 2084-2100 wrote:In an earlier paper [Phys. Rev. A 44, 5122 (1991)], we presented a Helmholtz-free-energy model for nonideal mixtures of hydrogen atoms and molecules. In the present paper, we extend this model to describe an interacting mixture of H2, H, H+, and e- in chemical equilibrium. This general model describes the phenomena of dissociation and ionization caused by pressure and temperature effects, as encountered in astrophysical situations and high-pressure experiments. The present model is thermodynamically unstable in the pressure-ionization regime and predicts the existence of a plasma phase transition with a critical point at Tc=15 300 K, Pc=0.614 Mbar, and ρc=0.35 g/cm3. The transition occurs between a weakly ionized phase and a partially (≊50%) ionized phase. Molecular dissociation and pressure ionization occur in the same narrow density range; atoms play a minor role in pressure ionization. In the high-density phase, complete pressure ionization is reached gradually. The sensitivity of the coexistence curve and of the critical point to model parameters and assumptions is discussed in detail.
I then apply these principles to all elements, where the heavier elements will be more easily ionized, as their outer electrons are not so tightly bound.
Lloyd wrote:Thornhill had discussed the same idea on his site, though I don't think he mentioned the term C.I. He had said that atoms in the core of a large body should gravitationally form dipoles, so that the negative sides face outward and the positive face inward. I think he "waved his hands" and the negative electron sides of the atoms formed electric currents toward the surface, leaving behind the positive nuclei. He then suggested that the nuclei would repel each other and result in equal pressure throughout the core. He said helioseismology showed that the Sun is indeed like that inside. Does that seem reasonable?
Helioseismology actually doesn't tell us much about the core, except that it is definitely there, and it definitely has a different density, because it produces a distinct shadow on the opposite side of the Sun. But p-waves don't pass through the core, so we don't know anything about the density gradient (if any). This, in fact, is what leaves the topic open to the speculation that it's hollow, while my take is that it's frozen rock solid, and p-waves bounce off of its rigidity. I agree that the density is probably quite consistent, and I agree that the reason would be electrostatic repulsion between ions. But we can't say that the seismic data support these assertions.
Regardless, the basic idea that gravity creates ionization is very reasonable. (See page 114 of Aspden, H., 2003: The Physics of Creation. Southampton, England: Sabberton Publications.) Protons are 1836 times heavier than electrons, and so will be more affected by gravity. A helium nucleus is 1836 x 4 times heavier, so the effect is even stronger. Hence positive ions will be pulled toward the core, and electrons will bubble up to the top, within the limits of the Coulomb forces at play (repulsion of like charges and attraction of opposite charges). Since the electric force is so much more powerful than gravity, it wouldn't seem that there would be much of a charge separation. But it's all relative. The Sun is 333,000 times more massive than the Earth, so there is 333,000 times more gravity, and 333,000 times more of a "fair weather field" than we have on Earth. Is an electric field like that going to start to display some distinctive properties? I think so.
But I really think that there is a lot more to it than just gravitational separation. The actual amount of gravitational force acting on any given particle is extremely small. But the weight of all of the particles above it adds up to a respectable force, once you get a couple hundred thousand kilometers inside the Sun. The pressure is, of course, an
effect of gravity, but you wouldn't call it gravitational separation, but rather, compressive ionization.
Lloyd wrote:Did the scientist say how far apart the adjacent nuclei would be at CI pressures?
Different scientists say different things.
The absolute limit for hydrogen "seems" to be 106 pm between nuclei, because 53 pm is the radius of the k-shell, which is the lowest electron level for hydrogen. At that distance, the density is 1.41 g/cm
3. Robitaille refers to the threshold of liquid metallic hydrogen, which is 0.6 g/cm
3, roughly 1/2 the absolute limit. The paper cited above found a threshold at 0.35 g/cm
3, which is 1/4 the absolute limit. At room temperature, hydrogen compressed to 0.07 g/cm
3 becomes an incompressible liquid, and this is at 1/20 of the absolute limit. Why so many different numbers? Great question!
Lloyd wrote:Kanarev in Russia seems to have done many experiments and determined the size and the toroidal shape of electrons (and protons). He found the electrons to be something like 2 or 3 orders of magnitude larger than protons. In that case it seems reasonable to me that the interatomic space might be too small for them.
This gets into a whole different brand of theory, about which I know extremely little. It's all interrelated, so how can you answer one question without answering all questions?
For now, I'm leaving the sub-atomic physics up to other theorists, and I'm using compressive ionization as a working hypothesis. There
is support for it, though not everybody agrees. Unfortunately, it's a tough thing to test, and there are few practical applications, so the lab results are sparse, and the theories are unconstrained. But it certainly seems to explain a lot of stuff.
Lloyd wrote:What would prevent electrons from being drawn back in between the positive nuclei? The electrons should be strongly "drawn" toward the nuclei.
This can only be because the nuclei are too close together, and there isn't the room for electrons. Maybe it's that the shells got broken, or, as Kanarev says, the electrons are too big. But if something like this were not the case, matter would be easily compressible down to the density of a neutron star, because the "degenerate matter" would have atomic nuclei and free electrons (and no electron shells) with no net electrostatic repulsion, and hence nothing to prevent the gravitational collapse. Yet this certainly isn't the rule, and might actually never happen (i.e., neutron stars might be impossible). And if it
was possible, what would prevent it in the core pressure (i.e., 10
17 N/m
2) inside the Sun? So there has to be something preventing it. That's the "something" that is the foundation of the compressive ionization model.
Lloyd wrote:Artificial diamonds are produced by subjecting carbon to extreme pressure. [...] Could diamonds be temporarily CI material when first formed?
I "think" that the graphite~diamond transition occurs before any sort of ionization kicks in. Graphite has a highly regular crystal lattice, and so do diamonds. But they're different. To go from the one to the other, you have to supply enough force to overcome the covalent bonds in the graphite, sending the electrons into higher energy states, to push the atoms closer. In the diamond arrangement, there are a new set of covalent bonds that can form, so the electrons settle back into lower states, and the new crystal lattice is stable in the new configuration. But I "think" that the electrons are never actually expelled, and thus it isn't ionization.
Lloyd wrote:The formation of a natural diamond requires very specific conditions [...] met in two places on Earth: the lithospheric mantle below relatively stable continental plates, and at the site of a meteorite impact.
This is why I track meteors -- if one of them ever impacts the Earth and I'm the first one there, I'll be rich!
And if I don't find any diamonds, I can still make beaucoup bucks doing an appearance on the "World's Most Dangerous Jobs" TV series.
CharlesChandler wrote:I thought that quasars are just randomly scattered in the vicinity of the AGN.
Lloyd wrote:No, they're not random. Thornhill and at least several TPODs say that quasars are seen to be on or very near the minor axes of nearby galaxies, the minor axis being the polar direction. And I think I now remember that Arp said that first.
Then I'd say that tokamak exhaust supplied the matter, especially if it was sputtering.
Lloyd wrote:Thornhill said quasars sometimes shoot out of galaxies equatorially, which explains the Dogleg galaxy, which has a spiral arm severed.
I'd call this a hurricane that spawned a tornado.
Lloyd wrote:Do you say that tokamaks transform into CI material? Or do tokamaks remain within CI material?
No -- I think that there are two types of stars: 1) slowly spinning stars (like our Sun) that are held together by CI, and 2) fast spinning stars that are held together by magnetic confinement (i.e., nat-tokamaks, including black holes, neutron stars, pulsars, magnetars, quasars, and white dwarfs). I think that when CI stars lose enough mass to drop below the threshold for CI, they bloat out into red giants, while nat-tokamaks whittle down to white dwarfs, still spinning really fast, and with powerful magnetic fields, and still generating the gamma rays indicative of nuclear fusion, but on a much smaller scale.