Inflationary Energy: Origins & Conversion

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Discussion Overview

The discussion revolves around the origins and conversion of energy during the inflationary period of the universe, exploring theoretical implications and the nature of energy conservation in an expanding universe. Participants examine the transition from the inflation field to particle production and the underlying mysteries of energy sources.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants propose that the energy of the inflation field converts into particles, but question the source of this energy, suggesting it may borrow from the gravitational field.
  • Others argue that energy is not conserved in an expanding universe, referencing external sources to support this claim.
  • A participant notes that pair production occurs rapidly at the end of inflation, with a common hypothesis being that the inflaton energy arises from quantum fluctuations in vacuum energy, though this raises paradoxes regarding the existence of space and time prior to the Big Bang.
  • There is a discussion about the role of pressure in contributing to the gravitational field, with some asserting that pressure is part of the stress-energy tensor, which sources gravity.
  • One participant challenges the notion that the origin of inflaton energy is a mystery, stating that it does not originate from anywhere due to the non-conservation of energy in an expanding universe, while acknowledging the mystery of the inflaton particle itself.
  • Another participant suggests that the origins of energy in the universe may be more mysterious than its conservation issues.

Areas of Agreement / Disagreement

Participants express differing views on the nature of energy conservation in an expanding universe, with some asserting it is not conserved while others question the implications of this. There is no consensus on the origins of the inflaton energy, with multiple competing hypotheses and unresolved questions remaining.

Contextual Notes

The discussion highlights limitations in understanding the origins of energy and the implications of inflationary theory, particularly regarding the assumptions about vacuum energy and the nature of spacetime prior to the Big Bang.

windy miller
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As I understand it when inflation ends, it gives up the energy of the inflation field and converts into a "hot soup" of particles.
But where does the energy of the inflation field come from? Can it borrow it from the gravitational field ?
 
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You get pair production at a furious pace at the end of inflation from the energy of the inflaton field. Where the inflaton energy originates is an unsolved mystery. A common hypothesis is it arises due to quantum fluctuations in the vacuum energy density of the infant universe - IOW it arises from nothing. A lot of people find that unsatifying because you need space and time as a backround for vacuum energy to exist. If spacetime itself was created by the BB, no space or time existed prior to the BB - turning the whole vacuum fluctuation thing into a chicken and egg paradox. Bear in mind there is no gravitational field without matter or energy. Welcome to the conflicting world where quantum physics meets theoretical cosmology.
 
Isn't pressure a contributor to the gravitational field ?
 
windy miller said:
Isn't pressure a contributor to the gravitational field ?

Pressure appears in the stress-energy tensor, so it is part of the source of the gravitational field. But you can't have pressure without having matter or energy.
 
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Chronos said:
Where the inflaton energy originates is an unsolved mystery.
I don't think this is an accurate statement. Where the inflaton energy originates isn't a mystery at all: it doesn't originate from anywhere as energy isn't conserved in an expanding universe. In particular, the properties of inflation make it so that a small amount of initial energy gives rise to a huge amount of energy at a similar density spread across a much larger region of space. There's no real mystery as to how this occurs: inflation has a nearly-constant energy density, which leads to a nearly-exponential expansion rate, which leads to a nearly-exponential increase in energy.

The mystery is where the inflaton itself came from: what is the inflaton particle, and how did it come to have a nearly-uniform density over a small region of space?

Also note that there are other alternative explanations for the early universe besides inflation, and those give rise to somewhat different questions about how our universe got its start. The answer to the energy issue remains the same in all of these models, however: energy isn't conserved in an expanding universe.
 
I'm guessing the origins of energy in the universe is more a mystery than its subsequent conservation, or lack thereof.
 

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