<p>The simple answer to your question is "yes" - the universe expanded at much greater speeds than $c$ during the inflationary epoch. This period of time was very quick but very dramatic, lasting from about $10^{-36}$ to $10^{-32}$ seconds. The universe expanded, in this very short period, by a factor of $10^{26}$. That's pretty incredible, when you think about it.</p>

<p>Inflation was originally proposed to solve, among other things, the horizon problem - that is, why the universe is isotropic and homogenous (on a large scale). This would mean that all the parts of the universe were in "causal contact" at one point in time. Inflation is the explanation for this.</p>

<p>Now, what does this all have to do with the CMB? Well, the temperature of the CMB is the same throughout the universe - a toasty 2.7 Kelvin. For the temperature to be uniform, all the regions of the universe would have had to be in causal contact in some point in time; hence, inflation explains the uniform temperature of the CMB.</p>

<p>However, the CMB was not around during the inflationary epoch. Far from it. It formed a lot later, when the universe was at the ripe old age of $379,000$ years. But the reason that it was formed (photon decoupling) equally throughout the universe is because the conditions were roughly equal, because of inflation. The CMB was, and still is, everywhere. It was never around during inflation, and as such was not otherwise affected by it.</p>

<p>I hope this helps.</p>

<hr>

<p>My sources for the times:</p>

<p><a href="https://en.wikipedia.org/wiki/Inflationary_epoch" rel="nofollow">Inflationary epoch</a></p>

<p><a href="http://map.gsfc.nasa.gov/universe/bb_cosmo_infl.html" rel="nofollow">NASA</a></p>

CC BY-SA 3.0
2014-09-17T23:01:22.177Z
2015-01-10T22:59:40.287Z
2015-01-10T22:59:40.287Z
HDE 226868
<p><strong><em>does that mean inflation occurred before the current laws of physics (read the four basic forces) precipitated, was c greater then than it is now?</em></strong></p>

<p><strong>NO</strong> Already the very concept of an <em>expansion velocity</em> is flawed. Expansion means that elements of the medium move away from each other with a relative velocity that is proportional to their distance (for small distances). The constant of proportionality, the <strong>expansion rate</strong>, is the sensible concept here and has dimension of a frequency. Currently the universe expands at about 73km/s/Mpc, which is the smallest natural frequency known. At the epoch of infation, the expansion rate was just much larger.</p>

<p>Of, course, over large sufficiently distances, any expansion results in superluminal velocities, but the laws of phyiscs only constrain the relative velocities of objects in close vicinity.</p>

CC BY-SA 3.0
2014-09-18T21:12:52.877Z
+1 for addressing some of the core misconceptions, although this stops short of addressing the follow-up question.
Stan Liou
CC BY-SA 3.0
2014-09-18T09:40:59.400Z
2014-09-18T09:40:59.400Z
Walter
<p>Yes, although we usually do not say the "expansion occurs faster than light."  In General Relativity space can be created between all points and that can result in points that were in causal contact (ie, they were able to see each other) before inflation, being, after inflation, farther away than light could travel in the age of the universe.  Basically, the rules in General Relativity are a bit more complicated than that of special relativity (which forbids accelerating an object to speeds greater than the speed of light).</p>

<p>Right now, since the local spacetime is not expanding as quickly as is the visible universe (that which we can see because it is within the distance that light travels in the age of the universe, c*t0), we are coming back into contact with regions of space that were out of contact since the inflationary period.   As time passes, we will be able to see a larger cosmic microwave background (CMB) surface. Spots on the CMB surface were not in contact with us (or each other) if they are more than 7 degrees apart since before the inflationary period.</p>

CC BY-SA 3.0
2014-09-17T22:41:52.853Z
Can you expand your last paragraph a bit? Regions that we were out of contact with before inflation are still moving away very fast.
HDE 226868
CC BY-SA 3.0
2014-09-18T17:48:26.087Z
Gravity has been slowing things down, so now things just outside of the visible universe are expanding away more slowly and light from them can eventually reach us.
eshaya
CC BY-SA 3.0
2014-09-18T22:20:14.083Z
While that may be the case, the expansion of the universe is accelerating.
HDE 226868
CC BY-SA 3.0
2014-09-19T04:18:30.560Z
I was trying to keep the cosmological constant out of this to keep it simple, but ...  True, since there is a cosmological constant, then there is some, minimum distance today at which everything is receding at c and that distance is shrinking.  It would be interesting to calculate that distance, but not necessary for this discussion.  You see, the visible universe continues to grow because tomorrow we will be able to see more distant galaxies than ever before because their light is, today, only one light-day away and that is well within that minimum distance.
eshaya
CC BY-SA 3.0
2014-11-07T17:21:02.847Z
I should have said in the last sentence that we will be able to see a larger CMB surface, not more galaxies, because near the edge of the visible universe galaxies have not yet formed. Spots on the CMB surface were not in contact with us (or each other if they are more than 7 degrees apart) since before the inflationary period.
eshaya
CC BY-SA 3.0
2014-09-17T22:28:03.067Z
2015-01-09T20:36:05.060Z
2015-01-09T20:36:05.060Z
eshaya
<p>If cosmological inflation occurred at speeds less than $c$, wouldn't we see the CMB right in front of our noses (or not at all) instead of at 13.7 billion light years?<br>
And <em>if</em> it happened faster than $c$, does that mean inflation occurred before the current laws of physics (read the four basic forces) precipitated, was $c$ greater then than it is now?</p>

CC BY-SA 3.0
2014-09-17T14:44:20.107Z
As far as I know CMB isn't at 13.7 Bly from us, it's actually everywhere in the universe, but dramatically redshifted to 2.73K microwaves.
Joan.bdm
CC BY-SA 3.0
2014-09-17T14:53:35.923Z
@Joan.bdm - But the CMB is the remains of the opacity wall at 60(?)ky after the big bang, isn't it? And since the BB occurred 13.7By ago, that light has traveled 13.7Bly, right? What am I doing wrong? Thanks for your reply, though.
stevenvh
CC BY-SA 3.0
2014-09-17T14:59:32.640Z
I think that is a common misconception, it wasn't an opacity wall (like the surface of a bubble), the whole universe was opaque and became transparent leading to the CMB we see today everywhere we look.
Joan.bdm
CC BY-SA 3.0
2014-09-17T15:05:13.477Z
Yes, inflation did occur at speeds greater than $c$. Joan's point about the CMB is also spot-on.
HDE 226868
CC BY-SA 3.0
2014-09-17T15:13:57.693Z
@HDE226868 - But the radiation we now see from the CMB did start 13.7By ago, doesn't it? In the CMB we see the universe as it was that long ago, and the light/radiation traveled 13.7Bly before it reaches us at this moment, right? I agree with Joan that it's around us (otherwise we wouldn't detect it), but my point is that what we see comes from 13.7Bly away. Agree?
stevenvh
CC BY-SA 3.0
2014-09-17T15:16:59.687Z
The CMB was not 13.7 billion light-years away 13.7 billion years ago. To the best of my knowledge, it was still everywhere.
HDE 226868
CC BY-SA 3.0
2014-09-17T15:23:12.630Z
@HDE226868 - (Disclaimer: I'm an engineer, not a cosmologist) However, I don't agree: If the radiation started 13.7By ago and reaches us now, and traveled at light speed, then it *must* have been 13.7Bly away when it started! Speed x time = distance. 1 light year/year (speed) x 13.7 billion years (time) = 13.7 billion light years (distance)
stevenvh
CC BY-SA 3.0
2014-09-18T07:56:35.660Z
@stevenvh No it doesn't. Since we are explicitly talking about the expansion of space, it necessarily was closer than naively calculated from transit time.
zibadawa timmy
CC BY-SA 3.0
2014-09-18T18:40:53.050Z
The CMB that we see was emitted about 13.7 billion years ago in terms of the cosmological time coordinate (based on clocks at rest in the local CMB frame), but from a location in space whose current [proper distance](http://en.wikipedia.org/wiki/Comoving_distance#Uses_of_the_proper_distance) ('current' using the definition of [simultaneity](http://en.wikipedia.org/wiki/Simultaneity) that's most common in cosmology) from us is more like 46 billion light-years, see the third paragraph of the [observable universe](https://en.wikipedia.org/wiki/Observable_universe) article on wikipedia.
Hypnosifl
CC BY-SA 3.0
2014-09-18T18:43:27.353Z
Also note that while all light waves in a vacuum travel at c as measured by local inertial observers, in a cosmological context the "speed of light" defined in terms of (proper distance traveled)/(cosmological time) may be different than c, as explained in the [proper distance subsection](http://en.wikipedia.org/wiki/Comoving_distance#Uses_of_the_proper_distance) of the [comoving distance article on wikipedia](http://en.wikipedia.org/wiki/Comoving_distance).
Hypnosifl
<cosmological-inflation><cosmic-microwave-background>
Did cosmological inflation occur at speeds greater than $c$?
stevenvh
# Did cosmological inflation occur at speeds greater than $c$?

(Asked by: username_0 on 2014-09-17)

If cosmological inflation occurred at speeds less than $c$, wouldn't we see the CMB right in front of our noses (or not at all) instead of at 13.7 billion light years?  
And *if* it happened faster than $c$, does that mean inflation occurred before the current laws of physics (read the four basic forces) precipitated, was $c$ greater then than it is now?

**Tags:** cosmological-inflation, cosmic-microwave-background
> **Comments:**
> **username_1**: As far as I know CMB isn't at 13.7 Bly from us, it's actually everywhere in the universe, but dramatically redshifted to 2.73K microwaves.  
> **username_0**: @Joan.bdm - But the CMB is the remains of the opacity wall at 60(?)ky after the big bang, isn't it? And since the BB occurred 13.7By ago, that light has traveled 13.7Bly, right? What am I doing wrong? Thanks for your reply, though.  
> **username_1**: I think that is a common misconception, it wasn't an opacity wall (like the surface of a bubble), the whole universe was opaque and became transparent leading to the CMB we see today everywhere we look.  
> **username_2**: Yes, inflation did occur at speeds greater than $c$. Joan's point about the CMB is also spot-on.  
> **username_0**: @HDE226868 - But the radiation we now see from the CMB did start 13.7By ago, doesn't it? In the CMB we see the universe as it was that long ago, and the light/radiation traveled 13.7Bly before it reaches us at this moment, right? I agree with Joan that it's around us (otherwise we wouldn't detect it), but my point is that what we see comes from 13.7Bly away. Agree?  
> **username_2**: The CMB was not 13.7 billion light-years away 13.7 billion years ago. To the best of my knowledge, it was still everywhere.  
> **username_0**: @HDE226868 - (Disclaimer: I'm an engineer, not a cosmologist) However, I don't agree: If the radiation started 13.7By ago and reaches us now, and traveled at light speed, then it *must* have been 13.7Bly away when it started! Speed x time = distance. 1 light year/year (speed) x 13.7 billion years (time) = 13.7 billion light years (distance)  
> **username_3**: @stevenvh No it doesn't. Since we are explicitly talking about the expansion of space, it necessarily was closer than naively calculated from transit time.  
> **username_4**: The CMB that we see was emitted about 13.7 billion years ago in terms of the cosmological time coordinate (based on clocks at rest in the local CMB frame), but from a location in space whose current [proper distance](http://en.wikipedia.org/wiki/Comoving_distance#Uses_of_the_proper_distance) ('current' using the definition of [simultaneity](http://en.wikipedia.org/wiki/Simultaneity) that's most common in cosmology) from us is more like 46 billion light-years, see the third paragraph of the [observable universe](https://en.wikipedia.org/wiki/Observable_universe) article on wikipedia.  
> **username_4**: Also note that while all light waves in a vacuum travel at c as measured by local inertial observers, in a cosmological context the "speed of light" defined in terms of (proper distance traveled)/(cosmological time) may be different than c, as explained in the [proper distance subsection](http://en.wikipedia.org/wiki/Comoving_distance#Uses_of_the_proper_distance) of the [comoving distance article on wikipedia](http://en.wikipedia.org/wiki/Comoving_distance).  

---

## 3 answers

### Answer by username_2 on 2014-09-17. Score: 8

The simple answer to your question is "yes" - the universe expanded at much greater speeds than $c$ during the inflationary epoch. This period of time was very quick but very dramatic, lasting from about $10^{-36}$ to $10^{-32}$ seconds. The universe expanded, in this very short period, by a factor of $10^{26}$. That's pretty incredible, when you think about it.

Inflation was originally proposed to solve, among other things, the horizon problem - that is, why the universe is isotropic and homogenous (on a large scale). This would mean that all the parts of the universe were in "causal contact" at one point in time. Inflation is the explanation for this.

Now, what does this all have to do with the CMB? Well, the temperature of the CMB is the same throughout the universe - a toasty 2.7 Kelvin. For the temperature to be uniform, all the regions of the universe would have had to be in causal contact in some point in time; hence, inflation explains the uniform temperature of the CMB.

However, the CMB was not around during the inflationary epoch. Far from it. It formed a lot later, when the universe was at the ripe old age of $379,000$ years. But the reason that it was formed (photon decoupling) equally throughout the universe is because the conditions were roughly equal, because of inflation. The CMB was, and still is, everywhere. It was never around during inflation, and as such was not otherwise affected by it.

I hope this helps.

---

My sources for the times:

[Inflationary epoch](https://en.wikipedia.org/wiki/Inflationary_epoch)

[NASA](http://map.gsfc.nasa.gov/universe/bb_cosmo_infl.html)


---

### Answer by username_5 on 2014-09-18. Score: 3

***does that mean inflation occurred before the current laws of physics (read the four basic forces) precipitated, was c greater then than it is now?***

**NO** Already the very concept of an *expansion velocity* is flawed. Expansion means that elements of the medium move away from each other with a relative velocity that is proportional to their distance (for small distances). The constant of proportionality, the **expansion rate**, is the sensible concept here and has dimension of a frequency. Currently the universe expands at about 73km/s/Mpc, which is the smallest natural frequency known. At the epoch of infation, the expansion rate was just much larger.

Of, course, over large sufficiently distances, any expansion results in superluminal velocities, but the laws of phyiscs only constrain the relative velocities of objects in close vicinity.

> **Comments:**
> **username_6**: +1 for addressing some of the core misconceptions, although this stops short of addressing the follow-up question.  

---

### Answer by username_7 on 2014-09-17. Score: 1

Yes, although we usually do not say the "expansion occurs faster than light." In General Relativity space can be created between all points and that can result in points that were in causal contact (ie, they were able to see each other) before inflation, being, after inflation, farther away than light could travel in the age of the universe. Basically, the rules in General Relativity are a bit more complicated than that of special relativity (which forbids accelerating an object to speeds greater than the speed of light).

Right now, since the local spacetime is not expanding as quickly as is the visible universe (that which we can see because it is within the distance that light travels in the age of the universe, c\*t0), we are coming back into contact with regions of space that were out of contact since the inflationary period. As time passes, we will be able to see a larger cosmic microwave background (CMB) surface. Spots on the CMB surface were not in contact with us (or each other) if they are more than 7 degrees apart since before the inflationary period.

> **Comments:**
> **username_2**: Can you expand your last paragraph a bit? Regions that we were out of contact with before inflation are still moving away very fast.  
> **username_7**: Gravity has been slowing things down, so now things just outside of the visible universe are expanding away more slowly and light from them can eventually reach us.  
> **username_2**: While that may be the case, the expansion of the universe is accelerating.  
> **username_7**: I was trying to keep the cosmological constant out of this to keep it simple, but ...  True, since there is a cosmological constant, then there is some, minimum distance today at which everything is receding at c and that distance is shrinking.  It would be interesting to calculate that distance, but not necessary for this discussion.  You see, the visible universe continues to grow because tomorrow we will be able to see more distant galaxies than ever before because their light is, today, only one light-day away and that is well within that minimum distance.  
> **username_7**: I should have said in the last sentence that we will be able to see a larger CMB surface, not more galaxies, because near the edge of the visible universe galaxies have not yet formed. Spots on the CMB surface were not in contact with us (or each other if they are more than 7 degrees apart) since before the inflationary period.  

---

