How can we see the cosmic background radiation?

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Cosmic Background Radiation (CBR) can be observed because, at the time it was released, the universe was much larger than it appears when considering a simple expansion from a single point. The initial singularity of the Big Bang does not imply that the universe started from a single point, as density can be infinite while volume is not. During cosmic inflation, space expanded faster than light, allowing CBR photons to travel vast distances. The particles that emitted the CMB photons are not the same as the matter that currently makes up our bodies, as they are now located far away. Understanding these concepts clarifies how we can see CBR without violating light-cone rules.
FizX
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I am wondering how it is possible that we see CBR. Here's why:
When the big bang occured, there was a sea of particles that gave off radiation. Now, if we are now made out of those particles, then how are we seeing their radiation now?
The only way I see this happening is if matter traveled faster than light at some point. How else would we be seeing the radiation from the same particles we are made out of? It would be violating the light-cone rules. Can someone clarify this for me? Thanks
-Chax
 
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I think you need look no further than a static (one with no reception) channel on your T.V.
 
What's more, we are looking into the past with CBR. So, we have a long time to separate from those particles, but we are seeing them back in their primitive form much as our particles were.

Funny: So, those particles may some day very well become part of an ET fixing to hunt us down and exterminate us for unwittingly insulting them with our messages to outer space.
Indeed, what if those SOS signals you made as a kid playing with your Dad's flashlight actually translate into something insulting enough for ET to start an intergalactic war once ET sees it?

Oh no... What have you done??
 
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FizX said:
I am wondering how it is possible that we see CBR. Here's why:
When the big bang occured, there was a sea of particles that gave off radiation. Now, if we are now made out of those particles, then how are we seeing their radiation now?
The only way I see this happening is if matter traveled faster than light at some point. How else would we be seeing the radiation from the same particles we are made out of? It would be violating the light-cone rules. Can someone clarify this for me? Thanks
-Chax

This is indeed a good question, which luckily has a solution!
The point here is that when the CMB (Cosmic Microwave Background) raditation was released, the universe was in fact much bigger than what one naively would think if one just let's it expand from a single point with the speed of light.
First of all, the initial singularity of the Big Bang need not be equivalent with that the universe started out from a single point. Somewhat loosley speaking the singularity just means that the density goes to infinity, not that the volume has to go to zero.
Secondly, even if the universe is finite in size (a closed universe) and once was much smaller, the period of http://en.wikipedia.org/wiki/Cosmic_inflation" saves the day, since during this epoch space expanded much faster than the speed of light (which does not contradict General Relativity). When the CMBR finally was released the space was already huge.
 
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The more fundamental thing to point out (apologies if I'm being too obvious here) is that was are not 'made out of those particles' that gave off the CMB photons that we see today. The stuff we are made of did give off CMB photons, but those photons are now a very very long way away from us. The material that gave of the particular CMB photons is by the same token a very long way away from us.
 
Thanks guys, that really helped.
 
Abstract The Event Horizon Telescope (EHT) has significantly advanced our ability to study black holes, achieving unprecedented spatial resolution and revealing horizon-scale structures. Notably, these observations feature a distinctive dark shadow—primarily arising from faint jet emissions—surrounded by a bright photon ring. Anticipated upgrades of the EHT promise substantial improvements in dynamic range, enabling deeper exploration of low-background regions, particularly the inner shadow...
https://en.wikipedia.org/wiki/Recombination_(cosmology) Was a matter density right after the decoupling low enough to consider the vacuum as the actual vacuum, and not the medium through which the light propagates with the speed lower than ##({\epsilon_0\mu_0})^{-1/2}##? I'm asking this in context of the calculation of the observable universe radius, where the time integral of the inverse of the scale factor is multiplied by the constant speed of light ##c##.
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