A couple of questions about The Big Bang Theory

In summary, scientists think that the universe is about 13.8 billion years old based on new data. They say that nothing can move faster than the speed of light and that this is not a contradiction because the expansion of the universe is happening faster than c.
  • #1
bpl1227
2
0
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?
 
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  • #2
bpl1227 said:
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?

1: It doesn't matter how big it is, it just matters how long things have been going on. Redshift of distant objects, and other information (the CBM for example) provide plenty of evidence for the age.

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
phinds said:
1: It doesn't matter how big it is, it just matters how long things have been going on. Redshift of distant objects, and other information (the CBM for example) provide plenty of evidence for the age.

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.

Thank you :)
 
  • #4
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.

Calculating the age of the universe is accurate only if the assumptions built into the models being used to estimate it are also accurate.

So in one sense nobody knows the actual age of the universe; we have no way to prove it...but there is lots of good evidence as outlined in the link if one assumes things started from a big bang. The FLRW λ-CDM cosmological model appears to show a good fit with observations...so it is the mainstream, consensus, [most popular] model so far. Of course most 'consensus science of past generations have been superseded by better models, so we will have to hope for now we are pretty close.

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?

That's not really the best way to think of it...there is no "empty space"...all space has vacuum energy of various types...and distant space IS receding away from us!..and we from it!

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.
 
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  • #5
Naty1 said:
... 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'

Actually, I've heard it said on this forum numerous times that it's about 3c at that distance. I've been quoting that myself for at least a year so if it's wrong, I'd like to know about it. Where did the 'c" come from? I'm sure it was one of the senior folks on the forum who stated it as 3c but I don't remember who.
 
  • #6
phinds said:
Actually, I've heard it said on this forum numerous times that it's about 3c at that distance. I've been quoting that myself for at least a year so if it's wrong, I'd like to know about it. Where did the 'c" come from? I'm sure it was one of the senior folks on the forum who stated it as 3c but I don't remember who.

You can relax Phinds its not in error. The c is simply a good multiplication factor. Recessive velocity is non inertia based for the OP. The galaxies are not moving at 3c. Recessive velocity is distance dependant. The greater the distance the greater the recessive velocity. I honestly wish they used a better term than velocity which implies momentum but were stuck with it. My sig contains a calculator called lightcone. Here is a sample printout. There is some guides including the metrics for the OP it will help with understanding how age is derived

[tex]{\small\begin{array}{|c|c|c|c|c|c|}\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}{|r|r|r|r|r|r|r|r|r|r|r|r|r|r|r|r|} \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
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
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
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}{|c|c|c|c|c|c|}\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}{|r|r|r|r|r|r|r|r|r|r|r|r|r|r|r|r|} \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
Mordred said:
You can relax Phinds its not in error. The c is simply a good multiplication factor. Recessive velocity is non inertia based for the OP.

I was not questioning whether any speed limits were being broken ... I understand recession velocity. My question is whether at the edge of the OU it is c or 3c.
 
  • #11
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
 
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  • #12
Mordred posts
Vnow the 3c crosses ...around 42Gly.

3c explanations:
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
Mordred posts:

Those are Planck numbers as of 2013.

Oh good grief...must I 'recalibrate' what little I know because the universe is a smidgeon older...
This is the third set of revised age data since I have been on the forums...
 
  • #14
Roflmao, I wouldn't worry about recalibrating just yet. At least not until further verification evidence but that's 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.
 

1. What is "The Big Bang Theory"?

The Big Bang Theory is a television sitcom that aired from 2007 to 2019. It follows the lives of a group of scientists and their interactions with their neighbor, a waitress and aspiring actress. The show is known for its humor and references to science and geek culture.

2. Is "The Big Bang Theory" scientifically accurate?

While the show does incorporate scientific concepts and terminology, it is primarily a comedy and not meant to be entirely accurate. Some of the science may be simplified or exaggerated for comedic effect.

3. Who are the main characters in "The Big Bang Theory"?

The main characters are Leonard Hofstadter, Sheldon Cooper, Penny, Howard Wolowitz, Raj Koothrappali, Bernadette Rostenkowski, and Amy Farrah Fowler. They are all scientists or science enthusiasts living in Pasadena, California.

4. How many seasons of "The Big Bang Theory" are there?

There are 12 seasons of "The Big Bang Theory", with a total of 279 episodes. The show concluded in 2019 as one of the longest-running and most successful sitcoms in television history.

5. Can I watch "The Big Bang Theory" if I am not a scientist?

Yes, "The Big Bang Theory" is enjoyed by a wide audience and does not require a scientific background to understand and appreciate the humor. However, some jokes and references may be more enjoyable for those with a basic understanding of science and pop culture.

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