Vacuum energy density after inflation

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SUMMARY

The discussion centers on the relationship between vacuum energy density and inflationary cosmology, specifically addressing whether varying vacuum energy densities in different pocket universes can be derived from quantum field theory or require string theory. It is established that a fundamental scalar with a metastable potential undergoing vacuum decay can lead to radically different physical properties across these universes. The conversation also highlights that while quantum field theory can explain some variations, string theory introduces additional complexities with new scalar fields, known as Moduli, that could further influence physical constants.

PREREQUISITES
  • Quantum Field Theory fundamentals
  • Understanding of vacuum decay mechanisms
  • Basic knowledge of inflationary cosmology
  • Familiarity with string theory concepts
NEXT STEPS
  • Explore the implications of fundamental scalars in quantum field theory
  • Research vacuum decay and its effects on physical constants
  • Study the role of Moduli in string theory
  • Investigate mathematical models of inflation and phase transitions in physics
USEFUL FOR

Cosmologists, theoretical physicists, and researchers interested in the interplay between quantum field theory and cosmological models, particularly those exploring the multiverse concept and vacuum energy dynamics.

windy miller
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Its said that if there are different pocket universes made by inflation then this solves the alleged fine tuning of dark energy. My question is this: can the idea of different values for the vacuum energy density in these different pockets be derived from quantum field theory or does it need something more exotic like string theory?
 
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windy miller said:
My question is this: can the idea of different values for the vacuum energy density in these different pockets be derived from quantum field theory or does it need something more exotic like string theory?

Field theory alone. All you need is a fundamental scalar with a metastable potential, which undergoes vacuum decay. The ensuing physics could (depending on the details of the new ground state) have radically different properties.
 
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Haelfix said:
Field theory alone. All you need is a fundamental scalar with a metastable potential, which undergoes vacuum decay. The ensuing physics could (depending on the details of the new ground state) have radically different properties.

Thanks, and those radically different properties you mention would they apply to just the vacuum energy density or to other values in physics? I believe that things like the masses of would only differ from pocket universe to pocket universe if string theory or something like it were true. Is that correct or incorrect?
 
In principle after vacuum decay, the behaviour of many of the constants in nature could be altered. It's a tiny bit involved, but a fundamental scalar could couple, almost like the interaction of the Higgs field does. The latter contributes to both gauge bosons, as well as fermions, so many properties of the surrounding universe would be radically different, depending on the details of the new vacuum.

String theory is something else, although a similar mechanism could exist within that framework as well. Many of the stringy models produce lots of new scalar fields (called Moduli), and the same sort of thing in principle could happen there.

The sketch of the phenomenon is really quite simple to describe mathematically, and similar things happen all over physics (for instance in condensed matter systems undergoing phase transitions) which is why its not completely crazy, and the details are very closely tied in with the mathematics of inflation.
 
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