What is the Cosmic Microwave Background and how can we observe it today?

  • Context: Undergrad 
  • Thread starter Thread starter Mr Davis 97
  • Start date Start date
  • Tags Tags
    Cmb Intuition
Click For Summary

Discussion Overview

The discussion revolves around the Cosmic Microwave Background (CMB), its nature, how it can be observed today, and the implications of an expanding universe on its characteristics. Participants explore conceptual issues related to the CMB's origin, its observational aspects, and the effects of cosmic expansion on its properties.

Discussion Character

  • Exploratory
  • Conceptual clarification
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants express confusion about the CMB, questioning how it can be observed today despite being emitted 380,000 years after the Big Bang.
  • One analogy compares the CMB to light signals emitted from particles in a body of water, suggesting that the CMB fills the universe rather than encompasses it.
  • Participants discuss the idea that the Earth has absorbed nearby light signals, implying that the CMB consists of light from distant regions that has taken billions of years to reach us.
  • There is a suggestion that the CMB radiation measured in the future will differ from current measurements, raising questions about its utility if it changes over time.
  • Some argue that the initial characteristics of the CMB are known due to plasma physics, and that expansion is the primary factor affecting its properties as it travels.
  • One participant raises a question about whether all radiation from recombination could eventually reach us, considering the finite nature of the universe and the concept of a cosmological event horizon.
  • Another participant explains that in an accelerating universe, there is a maximum distance beyond which signals cannot reach us, complicating the understanding of CMB observations.

Areas of Agreement / Disagreement

Participants do not reach a consensus on several points, including the implications of the CMB's changing characteristics over time and the nature of the universe (finite vs. infinite). The discussion remains unresolved regarding the extent to which all CMB radiation can be observed.

Contextual Notes

Limitations include the dependence on assumptions about the universe's structure and the unresolved nature of how the expansion affects the CMB's observability over time.

Mr Davis 97
Messages
1,461
Reaction score
44
I am having conceptual issues about what the CMB actually is. I read that it is the remnant radiation at the moment of recombination roughly 380,000 years after the Big Bang. But what about this statement implies that we would be able to observe this radiation today? To put it naively, when I look up into the night sky, where exactly is this radiation coming from? As a parallel, when I see a star I know that I am seeing the light that it emitted possibly millions of years ago relative to me. How can I really make a parallel statement when it comes to the CMB radiation, when looking out into the void of deep space, when at the time that radiation was present everywhere in this universe at the same time? I guess my main concern is how radiation encompassing the entire universe changes over time in an expanding universe. Also, if at the time 380,000 years after the big bang, this light was free to roam all over the universe, why can't it emitting from inside my house or a patch of land nearby? Why do have to look into deep space?
 
Space news on Phys.org
Mr Davis 97 said:
To put it naively, when I look up into the night sky, where exactly is this radiation coming from?
It comes from the gas that filled the universe back then. Imagine you're immersed in a large body of water, and then every particle of H2O sends a sound or light signal (somehow, magically) in every direction. You'll see it coming at you from all directions, with signals from progressively further afar arriving progressively later.
Same with CMBR, only instead of water you have plasma emitting light, which then travels in every direction.

Mr Davis 97 said:
I guess my main concern is how radiation encompassing the entire universe changes over time in an expanding universe.
It doesn't 'encompass' the universe, it fills the universe. I'm not sure if how it changes is relevant - in any case, it gets redshifted.

Mr Davis 97 said:
Also, if at the time 380,000 years after the big bang, this light was free to roam all over the universe, why can't it emitting from inside my house or a patch of land nearby? Why do have to look into deep space?
Because it's not being emitted now in your house. It was emitted long ago, and to see it you need to look in directions where there are no opaque objects obstructing its path.
 
  • Like
Likes   Reactions: stoomart, Orodruin and Drakkith
Bandersnatch said:
It comes from the gas that filled the universe back then. Imagine you're immersed in a large body of water, and then every particle of H2O sends a sound or light signal (somehow, magically) in every direction. You'll see it coming at you from all directions, with signals from progressively further afar arriving progressively later.
Same with CMBR, only instead of water you have plasma emitting light, which then travels in every direction.
So with this pool analogy, would it be at all correct to say that we (the Earth) in the pool have already absorbed the light signals in the near vicinity, and that what the CMB is is the light was emitted from water far away from us that we are just now receiving?
 
Mr Davis 97 said:
So with this pool analogy, would it be at all correct to say that we (the Earth) in the pool have already absorbed the light signals in the near vicinity, and that what the CMB is is the light was emitted from water far away from us that we are just now receiving?
Yes. All the radiation emitted nearby has already passed us by, or impinged on some disinterested dinosaurs etc. We're only receiving the light emitted from sufficiently far away, so that it had to travel for the past 13.7 Gy to get here. Tomorrow we'll see light from even further away.
 
Bandersnatch said:
Yes. All the radiation emitted nearby has already passed us by, or impinged on some disinterested dinosaurs etc. We're only receiving the light emitted from sufficiently far away, so that it had to travel for the past 13.7 Gy to get here. Tomorrow we'll see light from even further away.
So doesn't that imply that the CMB radiation that scientists measure in 1,000,000 years (if we're still here) will be different than the radiation we are measuring now? If that is so then what makes the CMB useful if it can change over time?

Also, what makes the CMB useful if we only have partial information regarding the measurement, since much of that light we have already absorbed?
 
The valuable thing about CMBR is that its initial characteristics are known due to how plasma physics works, and there's just one major thing that affects these characteristics as it travels - namely the expansion. So if some future scientist observes CMBR, she'll know exactly how much expansion has happened in the intervening time by measuring how much the radiation differs from the calculated initial state.

Furthermore, expansion affects just one of many characteristics of this radiation (wavelength). So, even as CMBR will differ in this one aspect at various times in the history of the universe, the remaining characteristics will still be visible in an unchanged state, giving the same information of the state of the universe at its emission.
 
Bandersnatch said:
The valuable thing about CMBR is that its initial characteristics are known due to how plasma physics works, and there's just one major thing that affects these characteristics as it travels - namely the expansion. So if some future scientist observes CMBR, she'll know exactly how much expansion has happened in the intervening time by measuring how much the radiation differs from the calculated initial state.

Furthermore, expansion affects just one of many characteristics of this radiation (wavelength). So, even as CMBR will differ in this one aspect at various times in the history of the universe, the remaining characteristics will still be visible in an unchanged state, giving the same information of the state of the universe at its emission.
One more question. Coming from the pool analogy, since the pool is finite, all of that initial radiation would reach us. How does this differ from the actual universe? Is it possible that all of the radiation from recombination would eventually reach us? Or does the expansion of the universe somehow preclude that?
 
1. It's possible that the universe is infinite,
2. Or, that it is finite and closed (instead of a pool, imagine a planet-wide ocean), in which case it'd be in principle possible for CMBR to 'circumnavigate' the universe.
3. Regardless of the above considerations, in an accelerating universe there exists a maximum distance from beyond which no signal can reach us (i.e. the cosmological event horizon). This simply means that light emitted from sufficiently far away won't be able to make headway against the (eventually) exponentially expanding universe. The closer the light was emitted to this horizon, the longer it'll take it to reach us, with light emitted at the horizon reaching us after infinite time. Even though the horizon is at a finite distance, it takes infinite time for light to get to us from it.

Since we don't know whether the universe is infinite of not, but it does appear that we're living in an accelerating one, this means that we're limited to a patch of the universe from which we may observe CMBR. We'll be always able to observe it, albeit in an ever-increasingly redshifted and dimmed form, as CMBR from even just a bit farther away will take ever longer and longer to get here.
 

Similar threads

  • · Replies 13 ·
Replies
13
Views
7K
  • · Replies 103 ·
4
Replies
103
Views
13K
  • · Replies 4 ·
Replies
4
Views
1K
  • · Replies 39 ·
2
Replies
39
Views
6K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 7 ·
Replies
7
Views
3K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 20 ·
Replies
20
Views
3K
  • · Replies 27 ·
Replies
27
Views
3K