Vacuum energy density after inflation

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Discussion Overview

The discussion revolves around the concept of vacuum energy density in the context of inflationary cosmology and the potential implications of different pocket universes. Participants explore whether varying values of vacuum energy density can be derived from quantum field theory or if more exotic theories, such as string theory, are required. The scope includes theoretical implications and the relationship between vacuum decay and fundamental constants in nature.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants suggest that the idea of different vacuum energy densities in pocket universes could be derived from quantum field theory, specifically through a fundamental scalar with a metastable potential undergoing vacuum decay.
  • Others express skepticism about the ability of quantum field theory alone to account for variations in other physical constants, proposing that string theory or similar frameworks may be necessary for such alterations.
  • One participant notes that after vacuum decay, the behavior of many constants in nature could be altered, drawing parallels to the interaction of the Higgs field and suggesting that properties of the universe could vary significantly based on the new vacuum state.
  • It is mentioned that string theory may also allow for similar mechanisms, with many models producing new scalar fields that could lead to variations in physical properties.
  • Participants discuss the mathematical simplicity of the phenomenon and its relevance to other areas of physics, such as condensed matter systems undergoing phase transitions.

Areas of Agreement / Disagreement

Participants do not reach a consensus on whether quantum field theory alone is sufficient to explain the variations in vacuum energy density and other constants, as some argue for the necessity of string theory or similar theories. The discussion remains unresolved regarding the adequacy of each theoretical framework.

Contextual Notes

The discussion highlights the complexity of the relationship between vacuum decay and fundamental constants, with participants acknowledging that the details of the new vacuum state are crucial but not fully resolved in the conversation.

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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