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All of which may be interesting, and even true (or it may be borderline slander); it is also irrelevant ... because it does not answer the question. Please answer the question.
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It is not slanderous to attack fundamental assumptions, especially when it can be demonstrated that these assumptions result in a multiplication of parameters. There is no question if my hypothesis is true, a whole lot of people end up looking like fools, but I number myself in their ranks: I almost totally bought into the conventional models until 1) The ultra deep Hubble surveys revealed more of the same. 2) The distant IR, radio and Xray source counts continued to rise ad finum. 3) I dissected the methodology used by CMB and supernova researchers and found them remiss.
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Originally Posted by Nereid
Please answer the question - did Zwicky, in the 1930s, establish that the 'dark mass' of (certain) rich clusters exceeded the (estimated) mass of the individual galaxies (of those clusers), or not?
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Yes, and if I may, Zwicky is one of my heroes. His morphological approach to complex problems parallels my own. Some of the ‘dark matter’ in rich clusters has been tracked down: We know they are loaded with hot and cold hydrogen and other baryons. We also know a great deal of dark matter exists as neutrinos. Even so, the relative velocites of rich clusters indicate that they should not be held together unless there is a great deal more dark matter that is unaccounted for.
But there are two other possible explanations: 1) The clusters are actually flying apart, which would mean after clusters form through some kind of magic, ‘dark energy’ or some other force is tugging away at them. 2) Newtonian inverse square law expectations are incomplete or incorrect.
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In your answer you have made a (new) ATM claim ("The Newtonian and Einsteinian concepts of gravity are wrong"). With respect to the rich clusters which Zwicky studied, please show, quantitatively, that your claim is consistent with his results.Please answer the question asked.
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Galaxy clusters are an incredibly complex environment and frankly, not completely understood – we are only just beginning to get a handle on how much cold gas there is in these environments. I think this is a poor place to test an alternative hypothesis because so many assumptions are necessary. Our own back yard is the best place to look: Why are gravitational assists yielding results that are inconsistent with Newtonian expectations? Why are Martian probe parachute drag coefficients nonsensical? What is Titan made out of, and why can’t we model the atmosphere?
Much of your argument centers on the fact we have such a good, tight model of the universe that it is inconceivable that there could be fundamental flaws. I’m looking at our solar probes and saying that the baseline assumptions upon which the entire cosmic structure has been outlined must be wrong. Specific questions about galaxy clusters cannot be addressed until after the underlying flaws are eliminated.
For example, if there are intrinsic redshifts in certain galaxy types, these galaxies will not be identified as being part of a super rich cluster, even though they are. Once this is understood, some of the need for dark matter in clusters evaporates.
It is worth noting that at great distances, it is common to see blue galaxies in clusters, but locally they seem to have a cluster avoidance mechanism. If blue galaxies are slightly intrinsically redshifted, they are not field galaxies at all, but reside near cluster centers locally, just as they do in distant clusters. This is why I am so focused on Solar observations: The fundamentals must be corrected before evaluating massive distant systems.
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There are several, independent, methods used, by astronomer, to estimate the non-baryonic and non-luminous mass in rich clusters, including: the Sunyaev-Zel'dovich effect, virial theorem (the method Zwicky used), gravitational lensing (of background objects), and analysis of X-ray observations (at least two, independent, effects).
My question is: to what extent do these independent methods yield consistent results (estimates of the mass of DM), when applied to rich clusters? Please answer the question - are the (rich cluster, DM) estimates consistent with (cosmological, DM) estimates?
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It is reasonable to conclude that there is either dark matter, or a different systemic that we do not fully understand. For example, our estimates of gravitational lensing are based primarily upon the lensing observed near our own sun. But what is we seriously over estimate the mass of the sun? That would mean it takes less mass to bend the same amount of light. Virial theorem is also dependent upon the inverse squared relationship, and X-ray observations confirm there is less baryonic matter than necessary to account for cluster population velocity distributions.
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It seems that you are implying that not "all redshifts are Doppler", and that "distance scales [canNOT] rely upon this". Of course the first is a strawman (and inaccurate to boot). The second is a very severe claim - that astronomers merely "assume" that "cosmic distance scales" can be determined from observations of redshift.
To what extent are you prepared to defend this claim?The consistency between estimates of DM, derived from different, independent, methods.
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I question the claim of independence. There are two, actually three, unproven assumptions common to virtually all galactic studies: 1) Almost all redshift is Doppler recession. 2) Doppler recession leads to time dilation according to relativist principles. 3) Supernova are good standard candles – their distance magnitude relationship is well established within ~ ˝ magnitude.
If the first assumption is wrong, and different galaxy types have varying degrees of intrinsic redshifts, population studies over-estimate the distance to intrinsically redshifted systems, which also overestimates the size of these systems. Which also lead to the false conclusion that the proportion of these systems becomes less dense with increasing distance (if you over estimate the size, you over estimate the extinction rate.)
If the second assumption is wrong, so is the calculated value of relativistic attenuation (1/(1+z)^4). I think there is STRONG evidence the relativistic formula for distant attenuation is wrong: Surface brightness measurements indicate an attenuation rate much closer to 1/r^2, unless galaxies of the same type get brighter with increasing distance. I think using an ad hoc surface brightness evolution factor in order to prop-up the relativistic distance modulus is a an unsupportable assumption, given the wide range of galaxy types, metallicity, star forming regions and so on that we can find at every distance.
The third assumption is wrong. We now have enough local supernova type Ia with a wide enough latitude in absolute magnitude that we must anticipate and correct for distance selection effects – we must assume that the more distant supernova we detect are dominated by the brightest of the local types and adjust our estimates of distance accordingly. There are all kinds of cosmic implications when these systemic problems are addressed.
We are completely off-topic for this thread, but our inability to communicate is symptomatic of the Catch-22 nature of alternative approaches to such a complex and well developed system of theories. They are so interlocking, it is almost impossible to independantly dissect any part the whole. There should be all kinds of alarm bells going off in the astrophysical community because of the planetary probe gravitational discrepancies I have cataloged. Something fundamental is wrong.