I'm continuing on my quest to really understand EU and plasma universe. I can see why you and the rest of the EU folk are frustrated with the mainstream, and I understand why you have to express that frustration vigourously occasionally, but this time I have to say that your post leaves me flummoxed. I am interested in the EU because I refuse to take things on faith and I insist on thinking for myself, but I have to apply that to EU too, and this is an area that I have researched.Michael Mozina wrote:http://chandra.harvard.edu/blog/node/399
I'll bet.However, we didn't explain *how* the gas got to be so hot and we obtained a number of questions from people about this.Nothing like a million+ degree enigma on your hands thanks to your 'discovery'.
OK, so is the EU position that because we create plasmas with electricity in the lab that plasmas on a cosmic scale can only be created electrically? (Although even that is not strictly the only way we create plasmas on earth - for example, any flame is at least a partially ionised plasma)What a bunch of pure nonsense. Here on Earth we heat and sustain plasma at high temperatures with *electricity*! The single most logical explanation for a high temp halo is not a spherically identical bunch of supernova events, or from an external galaxy colliding with our galaxy, and hitting everything at once. That's just pure nonsense on a stick! Who even wrote this crap?Chandra spokesman wrote: Smita Mathur, one of the co-authors, explained to me that there could be several different energy sources for heating the gas. One leading candidate is a galactic wind driven by supernova explosions. Another is that material from well outside the galaxy fell inwards and was heated by shock waves in the process.
A couple of questions: First, I didn't see any mention in the paper that the plasma is heated evenly. Did I just miss it? Second, how fast do you think the temperature of a plasma such as this one will fall?Bull! A shock wave isn't going to heat everything evenly or maintain it at high temperatures. Space is *cold* in their model, particularly away from all the stars. Any excess heat would be dissipated rapidly in the form of photons like they one's they're observing in the first place.It's important to appreciate that there does not need to be a continuous heating source for the gas.
How does the plasma lose energy? It seems to me that you are right - the only way it can do so is radiatively (obviously conduction and convection don't play a part). Ok, so what does this actually mean? A hot gas means that the individual atoms, ions and electrons are moving rapidly. This is the definition of temperature - the higher the temperature, the greater the kinetic energy of the atoms,ions and electrons. By what mechanism do they lose energy and thus reduce the temperature of the gas? I think you are right again - they do so by emitting photons - the very photons detected by Chandra. Now the key question, how are those photons emitted? The answer is that the photons are mainly emitted when atoms (not ions) collide, which results in excitation of the atomic state, which then relaxes to a lower state emitting a photon. Since this mechanism requires atoms, it is mainly forbidden transitions in metals which are responsible for the cooling, although some energy is lost by inelastic scattering of protons (hydrogen ions) or by recombination of electrons with ions. In any case, the rate of cooling depends on the frequency of collisions, which is obviously less in a less dense medium. The less dense the gas the lower the rate of cooling, and it can be shown that the rate of cooling goes as the square of the number density (particles per unit volume) of the plasma.Pure horse pucky. A high temperature ion is going to release it's energy *faster* in a diffuse and cold environment because nothing close by is radiating heat back into the ion and heating it back up again! That's a completely absurd statement. They have physics standing on it's head. They live inside of a universe of "alternative facts" apparently.Because the gas is extremely diffuse it loses energy by radiation very slowly,
Michael, I'm all for berating the mainstream when they screw up, but in this case, electricity is not required to keep a low density plasma at a high temperature for a very long time.More horse manure. There's no sunlight way out there to keep anything heated up. If we tossed *anything* at millions of degrees into deep space, it's going to cool off in short order (days), even if it's a *dense* and massive object. Tiny ions and individual particles will emit heat and cool off *instantly* (seconds/hours) by emitting photons. Do they actually think that the ion can emit photons for millions of years and not lose energy? Really?implying that it also cools down very slowly, over a timescale of ten billion years or more.
That claim is utterly irrational and it's complete and utter nonsense.
There *must* be a continuous source of energy that maintains the plasma at such hot temperatures, and the only logical choice is *electricity*, but that's the "forbidden term" in astronomy.
So shall we do some sums? Sums which I have just done, having just read the Chandra paperThe only thing that stays heated continuously is the hot air coming out of their mouths.So, once the gas is heated it stays hot for a very long time.
This has to be the single *lamest* and most pitiful "explanation" for anything that I've ever seen. Their "explanation" defies the laws of physics. There's nothing true or even logical about their so called "explanation", it's a complete pile of horse manure.
The radius of the halo is 300,000 light years which gives a volume of 9.5e64 m3. Let us take the mass of the plasma as 10 billion solar masses or 2e40 kg. The density is therefore 2e40/9.5e64 = 2.1e-25 kg/m3 = 2.1e-28 g/cm3. The mass of a proton is 1.6e-24 g, so we should expect, on average, 0.00013 ions per cm3, which is, as you can see a very low density with a very low cooling rate.
A well accepted cooling function for plasma at a ten million degrees is n2 x 10-30 J cm-3 s-1 where n is the number density per cm3 (see https://ned.ipac.caltech.edu/level5/Sep ... escu2.html). That gives a rate of cooling for this halo at 1.7e-38 J cm-3 s-1 or, over 10 billion years, 5.4e-21 J cm-3. The kinetic energy of a proton is given by 3/2(kT) where T is the temperature and k is Boltzmann's constant - at ten million degrees that is 4.1e-16J. So in 10 billion years, taking into account that an average ion occupies 7,700 cm3, a plasma at this temperature and density will lose only ten percent of its energy through radiative cooling. It ain't seconds or hours.