Early opaque universe - why little proton-photon scattering?

In summary, the early universe was opaque due to Thomson scattering off free electrons, which is much more likely than scattering off free protons due to the heavier mass of protons. This phenomenon is explained by the classical concept of power emitted being proportional to the time-averaged squared acceleration of the particle, which is in turn proportional to the mass of the particle. As a result, photons scatter off electrons with higher probability than they do off protons.
  • #1
Lapidus
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I read many times that the early universe was opaque foremost because of the scattering of photons off free electrons (Thomson scattering). Why is the scattering off free protons not equally important?

Btw, the same they say about stars. Photons within stars need a very long time to get out of the star because of scattering off the free electrons. Again, why not protons?

thanks!
 
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  • #2
The Thomson scattering cross section is proportional to [itex]m^{-2}[/itex], and so scattering off the much heavier protons is suppressed by a factor of a million relative to scattering off electrons.
 
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  • #3
Thanks!

And why is that so? Is there a simple physical argument behind this (curious) effect that photons scatter off particle with less mass with higher probability than they do with more massive particles?

My guess is that in Compton scattering the virtual particle in the Feynman graph is massive (an electron). So the more massive the propagator particle, the smaller the amplitude. Wrong?
 
  • #4
OR is it simply because the Compton wavelength is much smaller for protons than for electrons?
 
  • #5
It's best to think about Thomson scattering as a classical phenomenon, in which instead of photons bouncing of particles, one has a charged particle being accelerated by incident electromagnetic radiation and in turn radiating electromagnetic energy -- the scattered light. The power emitted is proportional to the time-averaged squared acceleration of the particle, which is itself proportional to [itex]m^{-2}[/itex] from Newton's 2nd law. This makes sense: electrons are more vigorously jiggled than protons by the electromagnetic radiation.
 
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1. What is the early opaque universe?

The early opaque universe refers to the period of time after the Big Bang, when the universe was extremely hot and dense. During this time, particles such as photons and protons were constantly colliding and scattering off of each other, making it difficult for light to travel freely. This resulted in the universe being opaque, or not transparent, to light.

2. Why was there little proton-photon scattering in the early universe?

Proton-photon scattering occurs when photons (particles of light) collide with protons (particles that make up the nucleus of an atom). In the early universe, the density of particles was so high that collisions were happening frequently, causing the universe to be opaque. However, as the universe expanded and cooled, the density of particles decreased, resulting in less frequent collisions and allowing light to travel more freely.

3. How did the early opaque universe become transparent?

As the universe expanded and cooled after the Big Bang, the density of particles decreased, allowing for less frequent collisions between protons and photons. This resulted in the universe becoming more transparent to light. Additionally, as the universe continued to expand, the wavelength of light also increased, making it easier for light to travel through the universe.

4. What role did the cosmic microwave background radiation play in understanding the early opaque universe?

The cosmic microwave background (CMB) radiation is the leftover heat energy from the Big Bang. It is considered the oldest light in the universe and can provide valuable information about the early universe. By studying the properties of the CMB, scientists were able to confirm the existence of the early opaque universe and understand the processes that led to its transparency.

5. How does understanding the early opaque universe help us understand the origins of the universe?

Studying the early opaque universe allows scientists to gain insight into the conditions and processes that occurred in the early stages of the universe. This can help us understand the origins of the universe and how it evolved into its current state. By understanding the early universe, we can also test and refine our theories and models of the Big Bang and the formation of the universe.

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