Gunn-Peterson effect and the Lyman-alpha forest

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In summary: The SDSS group observed the Gunn-Peterson trough at different redshifts, and they found that the trough is widest near the beginning of reionization and gets narrower as the reionization process proceeds.
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hellfire
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After the recombination epoch neutral hydrogen was formed in the universe. Since neutral hydrogen absorbs radiation in the Lyman-alpha transition, a dark epoch begun, which was finished with the reionization of hydrogen due to radiation sources.

The electromagnetic spectrum from quasars, which are at enough spatio-temporal distance (z > 6 ?) should show specific Lyman-alpha absobtion lines (inside the Ly-a forest) due to neutral hydrogen. This is called the Gunn-Peterson effect.

Questions:

1. is my understanding correct?
2. is the Gunn Peterson effect only a part of the the Ly-a forest, what is the differencie or how can this effect be registered…?

Thanks.
 
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  • #3
Hi,

In principle, neutral hydrogen pockets left over towards the end of reionization
could absorb all the hydrogen spectrum wave length.

In the discovery of the Gunn-Peterson effect, the SDSS group observed absorption
both in Ly-alpha and Ly-beta.
 
  • #4
hellfire,

Your understanding is correct, except regarding the Gunn-Peterson effect (otherwise known as the Gunn-Peterson trough). The Ly-a forest is so-called because the spectrum of the quasar looks like a forest, a bunch of absorption lines caused by the quasar light being absorbed by intervening clouds of neutral hydrogen at different distances (and therefore redshifts) from us.

If the quasar is far enough away, the light we’re seeing was emitted from the quasar before the universe was reioinized. This means that the “forest” of absorption lines becomes so dense, it looks like a trough (this is the Gunn-Peterson trough). That is, no light gets through to us for a certain span of redshifted Ly-a wavelengths, and that span defines the “edges” of the trough. The edge of the trough towards the red side of the spectrum is the Ly-a wavelength with a redshift corresponding to the redshift (distance) of the quasar. The blue side of the trough corresponds to the redshift or distance or time when the universe became reionized.
 

1. What is the Gunn-Peterson effect?

The Gunn-Peterson effect is an absorption phenomenon observed in the spectra of distant quasars. It is caused by the presence of neutral hydrogen gas in between the quasar and the observer, which absorbs certain wavelengths of light emitted by the quasar.

2. What is the Lyman-alpha forest?

The Lyman-alpha forest is a series of absorption lines observed in the spectra of distant quasars. These lines are caused by the absorption of specific wavelengths of light by neutral hydrogen gas in the intergalactic medium.

3. How is the Gunn-Peterson effect related to the Lyman-alpha forest?

The Gunn-Peterson effect is responsible for the formation of the Lyman-alpha forest. As light from a distant quasar passes through regions of neutral hydrogen gas, certain wavelengths are absorbed, resulting in the characteristic absorption lines seen in the Lyman-alpha forest.

4. What can the Gunn-Peterson effect and the Lyman-alpha forest tell us about the early universe?

By studying the properties of the Gunn-Peterson effect and the Lyman-alpha forest, scientists can gain valuable insights into the conditions of the early universe. This includes information about the distribution and density of neutral hydrogen gas, as well as the formation and evolution of galaxies and large-scale structures.

5. How do scientists use the Gunn-Peterson effect and the Lyman-alpha forest to study dark matter?

The Gunn-Peterson effect and the Lyman-alpha forest are important tools for studying dark matter, which is believed to make up a significant portion of the total matter in the universe. By analyzing the absorption lines in the Lyman-alpha forest, scientists can map the distribution of dark matter in the universe and gain a better understanding of its properties and role in the formation of galaxies.

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