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#221 | ||
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May 2004
New York City
5×7×112 Posts |
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Quote:
singularity. Cheesehd used the alternate "small dense state". But is it a "point" or not? A point has zero dimensions, zero properties. That would seem to be the necessary concept for this CCC sequential big bangs idea to work mathematically. But it couldn't work physically. I was perhaps being overly assertive, but there is no way for the infinitely spread-out Universe to pass through a zero-dimensional point to restart. Am I really being dogmatic? It seems obvious to me. |
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#222 | |
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May 2004
New York City
5×7×112 Posts |
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Universe has an infihite past, but rather whether there was a unique major event approx. 13.7 billion years ago which evolved space and matter and energy, such that the properties of the evolving universe changed both gradually and in sudden spurts through periods in which the laws of physics were not quite what they are now. Is that correct? This conception is what my monograph is trying to dispel. |
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#223 | |
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May 2004
New York City
5·7·112 Posts |
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That's fine, but I'm trying to understand your points and hopefully explain mine, and I do occasionally use words and ideas to do so that I didn't put in the monograph. ![]() BTW I've been working on draft 2, and this fundamental issue of the red shift and spectral lines is obviously important to resolve. |
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#224 | |
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May 2004
New York City
102138 Posts |
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the specially selected wavelength (in your example 6550) should represnt a "peak" (not a trough) in the measured spectrum. So I believe your numbers don't correctly represent a distant light source such as a star or galaxy. Perhaps 6547 0.95 6548 0.95 6549 0.96 6550 0.98 6551 0.96 6552 0.95 ? |
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#225 | |
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Bamboozled!
"πΊππ·π·π"
May 2003
Down not across
22×5×72×11 Posts |
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This is such basic spectroscopy, and something which has been understood for at least 150 years, that I wonder why someone writing about cosmogony doesn't know about it. Paul Last fiddled with by xilman on 2011-05-25 at 18:18 |
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#226 | |
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Oct 2007
Manchester, UK
101010011002 Posts |
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http://en.wikipedia.org/wiki/Absorption_spectroscopy |
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#227 | |
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May 2004
New York City
10000100010112 Posts |
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a lower intensity, not what Cheesehd and lava are trying to demonstrate, i.e. the shift in intensity downward in all frequencies toward the red, which I am suggesting is NOT demonstrated by Cheesehd's data/example because his "trough" at 6550 should be represented by a "peak" since the spectral lines represent the wavelengths at which MORE (not less) light is produced. That was a run-on sentence, but I'm leaving it. The issue is what does the data showing red shift actually look like. I think it's being looked at wrong, including here. Don't like being verbose, but as long as my alternative suggestion for how the red shift occurs is in question, I'm open to discussion. |
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#228 |
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May 2004
New York City
5×7×112 Posts |
And BTW thanks 4 pointing me to "cosmogony", which is an important
portion of what I'm trying to discuss in the "cosmology" monograph. The Wikipedia article mentions several issues I hadn't addressed (and some important ones I had), mostly epistemological, e.g. the quesrtion of the logical validity of infinite temporal regression. The article does express that origin explanations have long been theistic in nature, and that even current explanations that assume or explain the "beginning" of the universe, are iincomplete. The monograph emphasizes (and a bit better in my new draft) that there was no beginning. |
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#229 | |
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May 2004
New York City
5·7·112 Posts |
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#230 | |||
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"Richard B. Woods"
Aug 2002
Wisconsin USA
22·3·641 Posts |
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As I understand it, BB cosmologists contend not that any physics laws were different then than they are now, but only that, just as special relativity is asymptotic to Newtonian mechanics at speeds << c, so too do current physics laws that hold under "ordinary" circumstances diverge in extreme conditions to produce results that are not a linear extrapolation of what happens in nonextreme circumstances. IOW, what we know of current physics laws in our "ordinary" conditions may not yet incorporate asymptotic terms that become apparent only in extreme conditions. So, it's not that laws of physics were then (BB) not quite what they are now, but rather that additional terms of those laws may be apparent only in near-BB conditions. The laws haven't changed, but our current understanding of them is incomplete. Yes, of course. Quote:
E.g., regarding absorption lines, xilman's explanation is better than I would have written. As for the continuous emission spectrum behind my example's absorbing gas layer: it's composed of a myriad of emission lines (perhaps from a star, but that's not necessary for my example) that are smeared out by Doppler, relativistic, and other effects so that each "original" emission line gets broadened and merges with its neighbors. In other regions of the universe, such as nebulae, gases at low density and low pressure may emit light that is not smeared out by those effects, and so appears to us as discrete emission lines in a spectrum. Quote:
Does that mean you do not yet have ready your theory's explanation for the example I posed? It's okay with me to wait until you have that ready, if that's the case. |
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#231 | |
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May 2004
New York City
108B16 Posts |
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why do we even need the concept of a big bang to explain our universe? If you start with: the universe has always been (and I would continue that "like it is now") then no big bang explanation is necessary. |
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