What is a quantum fluctuation....

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SUMMARY

Quantum fluctuations during the inflationary period of the universe are critical for galaxy formation, as they create density variations in the early universe. These fluctuations arise from a single scalar field that transitions from a high-energy state to a minimum energy state, resulting in regions of varying energy density. Higher-density areas evolve into galaxy clusters, while lower-density regions become voids. The concept of cosmic structure is fundamentally linked to the amplification of these primordial density fluctuations through gravitational instability.

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  • Understanding of inflationary cosmology
  • Familiarity with scalar fields in physics
  • Knowledge of quantum mechanics and the uncertainty principle
  • Basic grasp of cosmic structure formation and power spectrum analysis
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  • Research the role of scalar fields in inflationary models
  • Study the implications of the uncertainty principle in quantum fluctuations
  • Explore gravitational instability and its effects on cosmic structure
  • Analyze the power spectrum of density fluctuations in cosmology
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Astronomers, physicists, cosmologists, and anyone interested in the fundamental processes of galaxy formation and the early universe.

wolram
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One reads a lot about quantum fluctuations but what exactly are they and how do they make a seed for galaxy formations ?
 
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The particular quantum fluctuations that you seem to be referencing here are the fluctuations that occurred during inflation which led to the pattern of large scale structure across our observable universe.

In most models, inflation is driven by a single scalar field. Scalar fields are fields which can be described by a single number at every point in space. The specific scalar field used to explain inflation would have had to experience some form of potential energy, and inflation occurs as the field slowly moves from a higher-energy state to the minimum energy state (inflation ends when it hits the minimum energy state).

However, quantum mechanics guarantees that the final picture won't be quite this simple, because the field value is guaranteed to bounce around a little bit even though the overall motion is downhill (towards the potential energy minimum). This leads to some regions in the early universe having ever so slightly higher energy density than other regions. Those higher-density regions eventually become dense regions of the universe, such as galaxy clusters, while the lower-density regions become voids.
 
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I always thought of them as random effects caused by particles obeying the uncertainty principle.
 
In the very early universe the size scale was not yet fixed.
 
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Chronos said:
In the very early universe the size scale was not yet fixed.

Size scale wasn't fixed? What does that mean?
 
Cosmic structure is a consequence of the amplification of primordial density fluctuations due to gravitational instability. Density fluctuations can be represented by a power spectrum and plotted as a function of distance, or z, according to taste. The expansion rate of the universe fluxctuated initially and continued to do so until some time after matter energy equality was achieved [i.e., after onset of the matter dominated epoch]
 
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