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A couple of questions about The Big Bang Theory 
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#1
Jun1613, 10:44 PM

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I understand the concept used here, but am unsure about how scientists can be so sure of the actual age of our universe. They explain it by saying it's like pressing rewind, based on the speed that galaxies are moving away from our own, but I don't understand how you can press rewind to find out how long ago "the beginning" really was, when we don't know where the universe ends, if there is an end.
Since scientists will admit they have no idea how big the universe actually is, and like to use the term "The observable universe" how can they identify an end point to "rewind" from? Also, I understand the concept that "nothing" can move faster than the speed of light, with empty space being nothing, but is the light itself still not traveling faster than the speed of light in this instance? If light itself travels faster than the speed of itself based on the laws of physics, is that not a contradiction to that particular law of physics in itself? Anyways, I would appreciate some feedback on these two questions, and you don't have to "dumb" it down for me. I am not a physicist nor scientist, but will have no problem understanding any formula's that can help explain how these experts are making calculations that contradict their own "rules". So to sum it up, here are the 2 questions once again. 1: How can we press rewind to calculate the age of our universe when we don't know how big the universe is? 2: How can light travel faster than the speed of itself under any circumstances? 


#2
Jun1613, 10:51 PM

PF Gold
P: 6,118

2) I doesn't and no one has said that it does (if they know what they are talking about). You may be getting confused here because the expansion of the universe, under the accelerating effect of "dark energy" IS happening faster than c, but no speeding tickets are issued because nothing is moving faster than c in any inertial frame of reference. Google "metric expansion" and take a look at the link in my signature. 


#3
Jun1613, 10:55 PM

P: 2




#4
Jun1913, 02:29 PM

P: 5,632

A couple of questions about The Big Bang Theory
For a discussion on the age of the universe try here...and particularly the PLANCK section...
http://en.wikipedia.org/wiki/Age_of_the_universe Just last year, 2013, new data suggests the universe is a bit older than was thought...now about 13.8 billion years old. A good rule when thinking about the speed of light is to remember "locally, light always travels at speed 'c' ". That means right where you are , regardless of your speed relative to anything you'd like to pick, earth, sun, me, whatever, you will measure light at 'c'. That's because right where you are spacetime is flat close to you.....If I measure light right where I am, I will also measure 'c'; but if you try to observe my light from some distance, or me yours, we will in general observe different speeds.... When distances are involved, and spacetime is curved, like in cosmology and spacetime with gravity [curvature], observations of distant light may appear to show varying speeds... Here is an example: At the Hubble radius, a distance of about 13.2 billion light years all around us, space [and distant galaxies there] is receding from us at a recession velocity 'c'.....according to to our FLRW cosmological model...using the distance 'metric' mentioned in a post already. So right ' there', right 'now', light appears to us to be 'standing still'.....[right there any beings will measure their local light at 'c' and our light as 'standing still']....in the future that distant light will start to approach us because of the nature of the expansion of the universe...and will eventually arrive here on earth....Other measures, other models, will show something different. 


#5
Jun1913, 03:18 PM

PF Gold
P: 6,118




#6
Jun1913, 03:33 PM

P: 1,857

[tex]{\small\begin{array}{cccccc}\hline R_{0} (Gly) & R_{\infty} (Gly) & S_{eq} & H_{0} & \Omega_\Lambda & \Omega_m\\ \hline 14.4&17.3&3400&67.9&0.693&0.307\\ \hline \end{array}}[/tex] [tex]{\small\begin{array}{rrrrrrrrrrrrrrrr} \hline a=1/S&S&z&T (Gy)&R (Gly)&D_{now} (Gly)&D_{then}(Gly)&D_{hor}(Gly)&V_{now} (c)&V_{then} (c) \\ \hline 0.001&1090.000&1089.000&0.0004&0.0006&45.332&0.042&0.057&3.15&66.18\\ \hline 0.003&339.773&338.773&0.0025&0.0040&44.184&0.130&0.179&3.07&32.87\\ \hline 0.009&105.913&104.913&0.0153&0.0235&42.012&0.397&0.552&2.92&16.90\\ \hline 0.030&33.015&32.015&0.0902&0.1363&38.052&1.153&1.652&2.64&8.45\\ \hline 0.097&10.291&9.291&0.5223&0.7851&30.918&3.004&4.606&2.15&3.83\\ \hline 0.312&3.208&2.208&2.9777&4.3736&18.248&5.688&10.827&1.27&1.30\\ \hline 1.000&1.000&0.000&13.7872&14.3999&0.000&0.000&16.472&0.00&0.00\\ \hline 3.208&0.312&0.688&32.8849&17.1849&11.118&35.666&17.225&0.77&2.08\\ \hline 7.580&0.132&0.868&47.7251&17.2911&14.219&107.786&17.291&0.99&6.23\\ \hline 17.911&0.056&0.944&62.5981&17.2993&15.536&278.256&17.299&1.08&16.08\\ \hline 42.321&0.024&0.976&77.4737&17.2998&16.093&681.061&17.300&1.12&39.37\\ \hline 100.000&0.010&0.990&92.3494&17.2999&16.328&1632.838&17.300&1.13&94.38\\ \hline \end{array}}[/tex] 


#7
Jun1913, 03:41 PM

P: 5,632

At the Hubble radius, recession 'c' is correct...but my distance figure of 13.2 seems to be one of several I have in my notes....13.8 seems likely closer.....but that may be out of date also...
Something interesting is at 3c recession velocity...but I have forgotten just what. edit: I see Mordred posted while I was composing.... 


#8
Jun1913, 03:49 PM

P: 5,632

Mordred...those numbers look a little different than I have seen.....
are those up to date?? Or am I out of date because new 2013 Planck data changed the age of the universe a bit?? 


#9
Jun1913, 03:59 PM

P: 1,857

Those are Planck numbers as of 2013. here is the Wmap as of 2013. Jorrie's latest version includes both as well as adding graph capabilities and sone curvature flexibility.
Here is WMAp [tex]{\small\begin{array}{cccccc}\hline R_{0} (Gly) & R_{\infty} (Gly) & S_{eq} & H_{0} & \Omega_\Lambda & \Omega_m\\ \hline 14&16.5&3300&69.8&0.72&0.28\\ \hline \end{array}}[/tex] [tex]{\small\begin{array}{rrrrrrrrrrrrrrrr} \hline a=1/S&S&z&T (Gy)&R (Gly)&D_{now} (Gly)&D_{then}(Gly)&D_{hor}(Gly)&V_{now} (c)&V_{then} (c) \\ \hline 0.001&1090.000&1089.000&0.0004&0.0006&45.732&0.042&0.056&3.27&65.82\\ \hline 0.003&339.773&338.773&0.0025&0.0040&44.566&0.131&0.178&3.18&32.61\\ \hline 0.009&105.913&104.913&0.0156&0.0239&42.357&0.400&0.549&3.03&16.74\\ \hline 0.030&33.015&32.015&0.0918&0.1388&38.325&1.161&1.640&2.74&8.36\\ \hline 0.097&10.291&9.291&0.5317&0.7992&31.063&3.018&4.554&2.22&3.78\\ \hline 0.312&3.208&2.208&3.0271&4.4332&18.181&5.667&10.595&1.30&1.28\\ \hline 1.000&1.000&0.000&13.7533&13.9999&0.000&0.000&15.792&0.00&0.00\\ \hline 3.208&0.312&0.688&32.0781&16.4035&10.686&34.281&16.429&0.76&2.09\\ \hline 7.580&0.132&0.868&46.2361&16.4926&13.645&103.433&16.493&0.97&6.27\\ \hline 17.911&0.056&0.944&60.4216&16.4994&14.900&266.882&16.499&1.06&16.18\\ \hline 42.321&0.024&0.976&74.6094&16.4998&15.432&653.095&16.500&1.10&39.58\\ \hline 100.000&0.010&0.990&88.7972&16.4999&15.657&1565.669&16.500&1.12&94.89\\ \hline \end{array}}[/tex] 


#10
Jun1913, 04:26 PM

PF Gold
P: 6,118




#11
Jun1913, 04:58 PM

P: 1,857

I know you know that phinds that was for the OP on recessive velocity. Thought I mentioned that. From what I see from the calculator Vnow the 3c crosses just prior to OU.
around 42Gly. Its easy to finetune exactly where the 3c comes in. Although it would depend on which Hubble constant value you use. Planck or WMAP 


#12
Jun2013, 02:32 PM

P: 5,632

Mordred posts
yes..it's in Mordred's table posted above....3c is about the speed at z = 1090 or so which is the 'surface of last scattering...as far as we can see into the past before glare blocks our view....or back to about 380,000 years after the big bang.....all different explanations of the same phenomena... 


#13
Jun2013, 02:52 PM

P: 5,632

Mordred posts:
This is the third set of revised age data since I have been on the forums..... 


#14
Jun2013, 07:00 PM

P: 1,857

Roflmao, I wouldn't worry about recalibrating just yet. At least not until further verification evidence but thats just my opinion. Lol when I first started studying cosmology there have been numerous changes in the six parameters. I gotten so used to it I expect them to change slightly with each new dataset.



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