astroscott said:
Sorry to ressurect this thread but I've started a blog on this and was hoping that some of you could visit it and tell me what you think.
The address is http://phil-astroscott.blogspot.com/2010/06/hi-im-phil-and-ive-decided-to-take-my.html"
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Your blog is really nice visually and the tone is modest and friendly. New Zealand seems like a nice place. The NZ scenery carries over and suggests that the universe is also a nice place.
I think you should broaden the scope of your blog and allow for both some LEARNING and some recent NEWS about the universe. Focus less on your alternative ideas about the bb and inflation.
Are you familiar with those blue and red oval maps of the microwave sky? The CMB temperature maps? They show the temperature as it would be measured by an observer who is at rest relative to the expansion process, or if you like relative to the ancient matter.
The actual measured temp map, because the solar system is moving at about 370 km/s ina certain direction relative to the CMB, would have a hot spot in that direction and a cold spot in the reverse direction. Simple doppler. That doppler dipole, that hotspot coldspot artifact of our absolute motion, is taken out of the data before the map that you see is made.
Absolute time, absolute rest, absolute motion, and the "proper distance" measure that goes with them are everyday familiar appliances to cosmologists. They even come with the standard model of the universe that virtually everyone uses. Technically called the LambdaCDM version of the Friedmann Robertson Walker Lemaître model, but the technical terminology is a nuisance.
Proper distance is what you would measure if you had enough time and used radar, or timed a flash of light, having first STOPPED THE EXPANSION at some given instant in time.
You stop the expansion process at a given instant and then see how long it is for a flash of light to reach the other galaxy. That tells its proper distance at that given instant.
Some people call that the "freeze-frame" distance. Because the distance doesn't change while you are measuring it. The distance one would measure like that at this present moment, today, has a special name: "comoving". Again the jargon words are a nuisance but that's life.
Ned Wright's calculator converts redshift to the today proper distance. Try it out.
THE DISTANCE TO MOST of the GALAXIES we can see using a telescope are INCREASING FASTER THAN THE SPEED OF LIGHT not because of inflation but just because that is how it is. General Relativity allows this (although the earlier "special" theory did not) and in fact the standard model with the jargon name REQUIRES it.
This doesn't have anything to do with time dilation (your reasoning in your blog). It is true using our plain old earthbased clocks. It is true using the "universe time" built into the standard cosmology model. It is true simply because Gen Rel gives a more accurate picture of dynamic geometry than one gets from Euclid or from Special Rel---and in the more accurate form of geometry distances are allowed to increase. Distances can increase between objects which are stationary relative to the ancient CMB light, or the ancient matter, or the expansion process, or however you like to think of it.
The Hubble law v = Hd is formulated in terms of proper distance. Whenever you use the Hubble law you are using proper distance. d is the distance and v is the rate it is increasing (Since we are only going 370 km/s absolute motion, our time is approximately the same as universe standard time, so the idea of rate of distance increase is not ambiguous.)
If you look at v = Hd you will see that if d is big enough the rate of increase v must exceed lightspeed c. In fact MOST galaxies which we are now looking at have distances more than enough to make the recession rate exceed c.
There are other distance measures, and Ned Wright's calculator gives some of them as well. But for starters, I would suggest getting familiar with the type of distance that goes into Hubble's law.
Google "Wright calculator" and put in a few sample redshifts.
For other types of distance (like how long the light took to get here etc etc.) there is a survey paper by Hogg that I recall reading some years back. Probably googling "Hogg astronomy distances" would get it. But if you want a link, just ask.
There is another simpler calculator, by Morgan, that I like. Google "cosmos calculator".
The only drawback is that at the start of a session you have to enter your three parameters (.27, .73, 71) for matter fraction, cosmo constant, and Hubble constant. You get the proper distance out, and the rate it is increasing, for different redshifts.
There is a nice Scientific American article by Lineweaver and Davis (Australians). I have a link in my signature. It is the "anu.edu.au/~charley" link.
You may know all this stuff and want more advanced sources and comment. If this is too rudimentary for you please say! I wanted to start with very basic stuff. Especially if you want Hogg's explanation of astronomy's alternative distance measures, ask for the link!