Inflation and expansion of the universe

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SUMMARY

The universe is expanding, and observations indicate that the recession speed of celestial objects increases with distance. The furthest observable point in time is approximately 379,000 years after the Big Bang, when protons and electrons formed neutral atoms, allowing light to travel freely. This event, known as recombination, led to the creation of the Cosmic Microwave Background (CMB), which marks the limit of our observational capabilities using electromagnetic (EM) radiation. Neutrinos could potentially provide insights beyond this limit, but their weak interaction with matter makes focused observation impractical.

PREREQUISITES
  • Understanding of the Big Bang theory
  • Familiarity with Cosmic Microwave Background (CMB) radiation
  • Knowledge of electromagnetic (EM) radiation properties
  • Basic principles of particle physics, particularly neutrino interactions
NEXT STEPS
  • Research the properties and significance of Cosmic Microwave Background (CMB) radiation
  • Explore the implications of neutrino astronomy for understanding the early universe
  • Study the effects of plasma on electromagnetic radiation
  • Investigate advanced observational techniques in cosmology
USEFUL FOR

Astronomers, physicists, and anyone interested in cosmology and the fundamental principles of the universe's expansion and early formation.

phtdegroot
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We know from observations that the universe is expanding and that the speed of recession of celestial objects increases the further we look back in space.
However, looking further in space is also looking back in time, so does this mean that we are looking at the end of inflation ?
 
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We can't see that far back in time, phtdegroot. The furthest we can see back is to about 379,000 years after the big bang. At this time, the hot plasma that permeated the universe reached a lower enough temperature for protons to combine with electrons to form neutral atoms. This is important because plasma interacts very strongly with EM radiation such as light, absorbing or scattering it before it can travel far. As a consequence, prior to this point in time light could not travel very far and it is impossible to see any further back in time using EM radiation. The CMB was created by this recombination event, and represents the furthest we can see at this time. To see further we could use neutrinos, except that they interact so weakly with other matter that it's essentially impossible to focus them down to a single spot like we can do with light and EM radiation.
 
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