How we are still able to detect CMB photons?

  • Thread starter CuriousNilave
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In summary, the expansion of space happened at a rate, not at a velocity. This does mean that some distances will grow faster than the speed of light but this is not due to anything actually moving in relation to something else. Even today distances will grow faster than the speed of light if you go far away enough.
  • #1
CuriousNilave
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This might be a silly question. But recently I got to know about CMB(cosmic microwave background) and this question is nagging me. During CMB , the universe was pretty small compared to now, so our current point of existence in space would have been very near the CMB, 13.7 bill yrs ago. So the photons from the CMB would have passed our point very early itself. Why is it passing our point now? Did the space between our point and CMB points increase faster than speed of light and because of this we are able to see CMB photons now?
 
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The CMB was released everywhere in the Universe. What we see now is simply microwaves from the part of the Universe that is just far away enough for the light from the CMB to take us 13.7 billion years to reach us. At the time of release, this was much closer to us than 13.7 billion light years, but it has taken so long because while the light has been progressing, the distance has grown due to expansion. The distance to those parts of the Universe today is significantly larger than 13.7 billion light years, which makes sense as part of the journey happened when the distance was smaller.
 
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  • #3
Thanks Orodruin. So did the expansion of space happened faster than speed of light during CMB period?
 
  • #4
CuriousNilave said:
So did the expansion of space happened faster than speed of light during CMB period?
First of all, expansion happens at a rate, not at a velocity. This does mean that some distances will grow faster than the speed of light but this is not due to anything actually moving in relation to something else. Even today distances will grow faster than the speed of light if you go far away enough.

Second, I suggest you read this FAQ: https://www.physicsforums.com/threads/at-what-velocity-does-the-universe-expand-can-it-be-faster-than-light.508610/
 
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  • #5
Thanks a lot.. This is very helpful!
 

Related to How we are still able to detect CMB photons?

What is CMB radiation and how is it detected?

CMB radiation, also known as cosmic microwave background radiation, is the residual energy left over from the Big Bang. It is detected through specialized instruments called radio telescopes, which can pick up the faint microwave signals emitted by the CMB.

Why is it important to study CMB radiation?

Studying CMB radiation allows us to understand the early universe and how it has evolved over time. It also provides evidence for the Big Bang theory and helps us to better understand the composition and structure of the universe.

How is it possible to still detect CMB photons if they were emitted over 13 billion years ago?

CMB photons are able to reach us because the universe has been expanding since the Big Bang, and this expansion has stretched their wavelengths. This stretching, known as redshifting, causes the photons to shift into the microwave frequency range, allowing us to detect them.

What challenges are faced in detecting CMB radiation?

One of the main challenges in detecting CMB radiation is filtering out other sources of microwave signals, such as radiation from Earth and our own galaxy. The instruments used to detect CMB must be highly sensitive and able to filter out these signals to accurately measure the CMB.

How has technology improved our ability to detect CMB radiation?

Over the years, advancements in technology have greatly improved our ability to detect CMB radiation. From more sensitive instruments to advanced data analysis techniques, technology has allowed us to gather more precise and detailed information about the CMB, leading to a better understanding of the early universe.

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