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For starters, the distribution from which the sample is drawn is known to be non-uniform, so just what low values from application of KS mean becomes unclear. Secondly, with such a small sample to begin with, a re-analysis (to compare any systematic differences within sub-groups) would very likely be meaningless ... unless, for example, all the spirals could be shown to belong to the same sub-group. - - - - - - - - - - - - - - - - - - - - I am curious about one implication of this 'intrinsic redshift', an aspect I don't think has been explored much in this thread so far. Suppose we were to get a mole of hydrogen from each of the two groups of spirals (the ones whose redshifts differ, systematically, per the Russel paper, by several hundred km/s) and bring them into a good lab. Suppose we took a sample of the hydrogen, from each source, together with some hydrogen from water we passed a current through, and put each sample in a spectroscope. Would all three samples of hydrogen show an H alpha line at 656.281 nm? Or would the two from the intrinsically redshifted galaxies have H alpha lines at different wavelengths? Or, to get a cleaner signal, if we collected positrons from those galaxies, would the annihilation line, observed in our lab, differ from 511 keV? Or would the maximum energy of the betas from the decay of 3H differ from 18.6 keV? Would the mass of a proton, from these galaxies, as measured in our lab, differ from 1.672 621 71 x 10-27 kg? And so on. Of course, we don't have to leave home to do some of these tests; we could get quite a few constraints on how different physics is, locally in these galaxies, by using the kind of approach Bahcall used to constrain variations in alpha over cosmological time. This kind of approach has the benefit that no telescope time is needed - I guess all the relevant data, for at least some studies of this kind, is already freely available to anyone with a broadband internet connection*. Does anyone reading this know if any proponent of 'intrinsic redshift' has even tried something like this? *Though you may need to live in the US, the EU, Canada, etc; I think there are some restrictions on data access wrt nationality. |
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Now that this has been done and nothing was found to contradict Russell's findings, it is suggested that the doing these investigations "would very likely be meaningless" anyway. Quote:
TomT |
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If that's so, then: a) there are too few galaxies, in each (sub-)group, to do any meaningful analysis b) to aggregate across sub-groups, you need to do some kind of meta-analysis ... for which I think you'll find you need different statistical tools ... As to frustration ... that's the way it goes when you do scientific research ... if a key assumption behind an approach (in this case, that the Virgo cluster is, in a key respect, homogeneous) turns out, later, to be wrong, then you have to go back and start again. If you're lucky, you don't need to go back to the very beginning; in this case, I don't think you've been lucky. Quote:
For example, the Bahcall method would show, to a pretty accurate level, just how different alpha is, in those galaxies, from what it is in labs here. As you know, alpha is dimensionless, and also a key parameter in modern quantum theory (QED), characterising the strength of the electromagnetic interaction. But my point was more general: there are quite a few tests one can make, of what 'local physics' is, using nothing more than data from photons from distant objects ... and such tests are pretty easy to do, if only because there is such a wealth of high-quality data available on the web ... and there are several examples in the astronomical literature* Here's something to think about: if all you have, wrt 'intrinsic redshifts', is a small number of marginal results, then no one will take you seriously. OTOH, if you also have some good results which show that 'local physics' is, in fact, different (at many sigma) than it is here, you have an independent set of results that points to something potentially very interesting. An analogy: the 'solar neutrino problem'. But, suppose that 'physics there' turns out to be the same as 'physics here', from many different, independent tests. Then 'intrinsic redshift' is more likely to be an artifact of your (small sample study) initial work. *the CMB was warmer in the past, footprints of deep gravitational wells in x-rays from accretion disks, ... |
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Cheers. P.S. Nereid, there are some questions from earlier in this thread you haven't responded to. |
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So that leaves 5 of Russell's spirals outside of this region on the near side and 9 outside on the far side, i.e. not distributed among the groups. Quote:
TomT |
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Well, if you'd be kind enough to point me to them (we have, what, one day left?) |
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Is that why you suddenly started posting to this thread again? You're not seriously suggesting you missed the complaints from the proponents when you decided to walk away from this dicussion?
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Of course. Are you asserting my list of candidate galaxies has been refuted? What about my simple request for the number and catalogue designations of cepheid calibrators used to 'normalize' the data? I already spoon fed you everything necessary to justify your objections. Unfortunately, it appears I am the only one putting any 'numbers' on the table. Does redshift distance - [insert favorite] independantly determined distance ring any bells? Asking me for more numbers when you have offered none is - an interesting debating tactic. It appears I am wasting my time. I concede I am no match for your suite of preconceived, inherently unfalsifiable Arpian notions.
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Perhaps you did not see this New Policies Regarding Against the Mainstream section New Policies Regarding Against the Mainstream section Quote:
__________________
RussT ________________________________ Everything is, as it should be, otherwise, it wouldn't be! |
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