How do they measure the CMB temperature?

In summary, the CMB temperature is measured by the frequency of the peak of its spectrum, which closely follows a Planck black-body spectrum. This radiation is a remnant of the hot ionized hydrogen and helium that were produced during nucleosynthesis in the Big Bang. The energy for this radiation is thought to have come from the annihilation of matter and antimatter particles in the early universe. As the universe cooled, the radiation became transparent and we can now see its remnant, known as the "Surface of Last Scattering," red-shifted by z ~ 1100 as the CMB. This radiation is remarkably homogeneous and isotropic, resulting in a nearly perfect black-body spectrum. Anisotropies in the radiation are
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touqra
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How do they measure the CMB temperature? Aren't they just some radiation?
 
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touqra said:
How do they measure the CMB temperature? Aren't they just some radiation?
Yes! The CMB very accurately follows to Planck spectrum of a black body at a specific temperature. That temperature is measured by the frquency of the peak of the spectrum as shown here.

Garth
 
  • #3
What is the black body here? Is it the whole universe? How does it happen that CMB is a perfect black body spectrum?
 
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The whole universe was originally filled with hot ionised hydrogen and helium that were the products of nucleosynthesis in the BB. The energy for the radiation is thought to have come from the epoch of matter-antimater annihilation where (108 + 1) matter particles annihilated 108 anti-matter particles leaving ~108 photons per atomic particle in the present universe.

That radiation was bounced around the very early and opaque universe until the plasma termperature fell to ~ 30000K when the protons and electrons associated to form neutral hydrogen atoms, then the universe became transparent.

We see that 'Surface of Last Scattering' all around us and now red-shifted by z ~ 1100 as the CMB.

The plasma and subsequent gas was remarkably homogeneous and isotropic and therefore its radiation follows a Planck black-body spectrum very closely.

There are anisotropies, of course, but they are another story.

Garth
 
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FAQ: How do they measure the CMB temperature?

What is the CMB temperature?

The CMB temperature, or Cosmic Microwave Background temperature, is the temperature of the radiation left over from the Big Bang. It is currently measured to be approximately 2.7 Kelvin (K), or -270.45 degrees Celsius.

How is the CMB temperature measured?

The CMB temperature is measured using specialized telescopes that detect the faint microwave radiation coming from all directions in the universe. The most famous of these telescopes is the Cosmic Background Explorer (COBE) satellite, which provided the first accurate measurement of the CMB temperature in 1992.

What does the CMB temperature tell us about the universe?

The CMB temperature is an important piece of evidence for the Big Bang theory, as it supports the idea that the universe was once much hotter and more dense. It also provides information about the composition and evolution of the universe, and can help us understand the structure of the universe on a large scale.

How has the CMB temperature changed over time?

The CMB temperature has decreased over time as the universe has expanded and cooled. In the early universe, it was much higher (around 3000 K) and has steadily decreased to its current measurement of 2.7 K. Scientists can use this information to study the history and evolution of the universe.

Are there any limitations to measuring the CMB temperature?

Yes, there are some limitations to measuring the CMB temperature. One limitation is the presence of foreground radiation, which can interfere with the measurements. Another limitation is the sensitivity of the instruments used, as the CMB radiation is extremely faint. However, scientists are constantly improving their techniques and technology to overcome these limitations and provide more accurate measurements of the CMB temperature.

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