Baryonic acoustic oscillations and density perturbations

In summary, the connection between BAO and PDP is that the quantum fluctuations during inflation are the cause of both. Baryons and photons being in thermal equilibrium before decoupling leads to pressure forces, but the competition between this pressure and the gravitational force from high dark matter density causes oscillations and the formation of large scale structures after decoupling. PDP is not something that occurs before inflation, but rather during it and the resulting fluctuations in the inflaton field are the seeds of structure formation.
  • #1
jono90one
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Hi,
I am just trying to understand the connection between these two things. As far as I understand it:

BAO - Before decoupling the baryons were in thermal equilibrium with photons and as a result this gave rise to a pressure force. But given in regions of high dark matter density baryons are drawn in. So there is a competition between the outward pressure and this gravitational force giving rise to acoustic oscillations. After decoupling these then "clump" together in different regions of densities and begin to build large scale structures.

Primordial density perturbations (PDP) - Quantum mechanical fluctuations before inflation lead to small perturbations, when inflation occurs there is a super luminous expansion where virtual particles become real particles as the expansion is to fast for them to annihilate, this gives rise to oscillations which then become sub-horizon (connecting casually disconnected regions).

But are the above two anything different, they both lead to large scale structure. I understand that baryons won't have existed in the very early universe so clearly there is a difference in what is being described, but is it true that:
PDP leads to BAO which leads to Large Scale structure?

Thanks
 
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What causes the initial dark matter inhomogeneities that set up the BAO? That's where the PDP come in -- the quantum fluctuations generated during inflation are the seeds of structure formation, including the BAO.

Your take on PDP is a little off. First, the fluctuations occur during, not before, inflation. The exponential expansion causes the wavelengths of these fluctuations to grow larger than the causal universe (it's not "superluminal expansion" -- this is a common misconception). The result is a spectrum of fluctuations across a wide range of length scales. Once outside the horizon, the quantum fluctuations become classical curvature perturbations. You mention particles and antiparticles -- yes, this is the frequently seen cartoon that helps visualize this process, but it's not likely to be physically correct. Instead of particle creation during inflation, we have an amplification of quantum fluctuations of the inflaton field (yes, in normal QFT field fluctuations about the vacuum *are* particles, but during inflation the field is never in the true vacuum). The way to picture these fluctuations is as differences in the value of the inflaton field across space (the field essentially executes Brownian motion). Regions of the universe with different values of the inflaton field have different energy densities, and hence, expand at different rates. When the universe reheats, these different regions of the universe will have different densities -- these are the seeds of BAO and structure formation.
 
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1. What are baryonic acoustic oscillations?

Baryonic acoustic oscillations refer to a pattern of fluctuations in the density of matter in the universe, caused by acoustic waves that traveled through the early universe. These waves were created shortly after the Big Bang and were imprinted on the distribution of matter in the universe.

2. What are density perturbations?

Density perturbations are fluctuations in the density of matter in the universe. These perturbations can be observed on a large scale, such as in the distribution of galaxies, or on a small scale, such as in the distribution of matter within a galaxy.

3. How are baryonic acoustic oscillations and density perturbations related?

Baryonic acoustic oscillations and density perturbations are related in that the acoustic waves that created the oscillations also caused small variations in the density of matter. These variations grew over time, leading to the formation of galaxies and large-scale structures in the universe.

4. Why are baryonic acoustic oscillations and density perturbations important in cosmology?

Baryonic acoustic oscillations and density perturbations provide valuable information about the structure and evolution of the universe. By studying these patterns, scientists can better understand the processes that shaped the universe and the distribution of matter within it.

5. How do scientists study baryonic acoustic oscillations and density perturbations?

Scientists study baryonic acoustic oscillations and density perturbations by analyzing large-scale surveys of galaxies and their distribution. They also use computer simulations and theoretical models to better understand the underlying physics behind these phenomena.

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