Big Bang Background Radiation: Questions Answered

In summary: This process goes on infinitely, so the cosmic microwave background will continue to be continuous forever. In summary, the cosmic microwave background is a continuous form of thermal radiation that was created about 370,000 years after the big bang during an event called recombination. It has been redshifted into the microwave range and will continue to be continuous forever as the radiation reaching us now was emitted from a larger distance than the radiation reaching us one second ago.
  • #1
JKFlyguy
23
0
Hi,

I have a simple question that will probably have a simple answer.
If the Big Bang was a finite event (i.e. took place over a certain amount of time) why is it that the background radiation from it as sensed on Earth (TV static) is continuous? Will it continue to be continuous forever? How is this possible if the radiation coming from it was a single, finite event?

Thanks,
Josh
 
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  • #2
It was finite in time, but happening over a large (possibly infinite) volume of space. We're getting CMBR from farther and farther away every instant.
The expansion of space is, however, continuously stretching the radiation, so it's not continuous in that sense (its energy goes down).
 
  • #3
The cosmic microwave background did not directly come from the big bang any more than you or I did, though you may read otherwise in some places. It was created about 370,000 years after the big bang during an event called 'recombination'.

http://en.wikipedia.org/wiki/Cosmic_microwave_background
http://en.wikipedia.org/wiki/Recombination_(cosmology)

The idea is that the entire universe was filled with a very hot plasma. Well, hot plasma radiates thermal radiation, which includes visible light. Once recombination occurred, it was like a fog lifting from the universe. The plasma turned into a neutral gas, which doesn't absorb light, so there was nothing to block the light from propagating. The CMB is this thermal radiation. It has been redshifted so much it is now out of the visible range and into the microwave range.

JKFlyguy said:
How is this possible if the radiation coming from it was a single, finite event?

The radiation reaching us now was emitted further away from us than the radiation that reached us one second ago, and that was emitted further away than the radiation that reached us 2 seconds ago.
 

Related to Big Bang Background Radiation: Questions Answered

1. What is the Big Bang Background Radiation?

The Big Bang Background Radiation, also known as the Cosmic Microwave Background (CMB), is the remnant thermal radiation left over from the initial stages of the Big Bang. It is the oldest light in the universe and is present in all directions, with a nearly uniform temperature of 2.725 Kelvin.

2. How was the Big Bang Background Radiation discovered?

The CMB was first predicted by George Gamow and Ralph Alpher in 1948, but it was not until 1965 that Arno Penzias and Robert Wilson accidentally discovered it while working at Bell Labs. They were trying to eliminate background noise in their radio antenna, but found a persistent noise that could not be eliminated. This turned out to be the CMB, confirming the Big Bang theory.

3. What does the Big Bang Background Radiation tell us about the universe?

The CMB provides strong evidence for the Big Bang theory, as it supports the idea that the universe began as a hot, dense state and has been expanding and cooling ever since. It also gives insight into the composition of the universe, as its temperature and fluctuations can tell us about the amount of matter and energy present.

4. What causes the fluctuations in the Big Bang Background Radiation?

The slight variations in temperature in the CMB are caused by density variations in the early universe. These density variations were the seeds for the formation of galaxies and other structures we see in the universe today. The study of these fluctuations has provided valuable information about the origin and evolution of the universe.

5. How can we observe the Big Bang Background Radiation?

The CMB is most commonly observed through microwave telescopes, which can detect the faint, low-energy radiation emitted by the CMB. The most famous instrument for studying the CMB is the Wilkinson Microwave Anisotropy Probe (WMAP), which has provided detailed maps of the CMB and has greatly advanced our understanding of the early universe.

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