Vacuum energy density after inflation

In summary, the idea of different pocket universes can solve the alleged fine tuning of dark energy. This concept is supported by the Multiverse theory, which has been used to explain various aspects of physics. It is possible to derive the different values of vacuum energy density in these universes from quantum field theory alone, through a fundamental scalar with a metastable potential undergoing vacuum decay. This could result in radically different properties in the new ground state. String theory, which also produces similar scalar fields, could potentially exhibit the same phenomenon. This phenomenon is closely tied to the mathematics of inflation and has similarities with other physical systems undergoing phase transitions.
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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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Multiverse to the rescue again! It's the undisputed king of patent medicine curing everything from initial conditions to fine tuning, anthropism, the values of dimensionless constants and even falsification of TOE's..
 
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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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  • #4
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?
 
  • #5
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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What is vacuum energy density after inflation?

Vacuum energy density after inflation refers to the amount of energy present in the vacuum of space after the rapid expansion of the universe during the inflationary period. It is also known as the "zero-point energy" and is thought to be responsible for the ongoing expansion of the universe.

How is vacuum energy density after inflation measured?

Vacuum energy density after inflation is measured through a variety of methods, including observations of the cosmic microwave background radiation, the large-scale distribution of galaxies, and the effects of dark energy on the expansion of the universe. These measurements provide insights into the amount and behavior of vacuum energy density.

What is the significance of vacuum energy density after inflation?

Vacuum energy density after inflation plays a crucial role in our understanding of the universe and its evolution. It is believed to be a key factor in the acceleration of the expansion of the universe and the formation of galaxies and large-scale structures. It also has implications for theories such as inflation and dark energy.

Can vacuum energy density after inflation be harnessed for practical use?

Currently, there is no known way to harness vacuum energy density after inflation for practical use. The energy present in the vacuum is incredibly small and difficult to access, and our current understanding of physics does not allow for the direct extraction of this energy. However, ongoing research and advancements in technology may lead to potential applications in the future.

Are there any controversies surrounding vacuum energy density after inflation?

There are ongoing debates and controversies surrounding vacuum energy density after inflation, particularly in terms of its role in the expansion of the universe and the nature of dark energy. Some theories propose alternative explanations for the observed effects attributed to vacuum energy density, while others suggest that it may not exist at all. Further research and observations are needed to fully understand this concept.

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