How do inflatons and gravity interact?

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Discussion Overview

The discussion revolves around the interaction between inflatons and gravity, particularly in the context of the early universe during inflation and the current accelerated expansion of the universe. Participants explore theoretical implications, the role of gravity, and the nature of inflatons in these scenarios.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants propose that inflatons dominate when gravity is both strong (immediately after the big bang) and weak (during the current expansion of the observable universe).
  • Others argue that the mechanisms driving inflation in the early universe and the current accelerated expansion are not necessarily the same, suggesting a need for clarification on the definitions of "strong" and "weak" gravity.
  • It is noted that matter had not yet come into existence during inflation, leading to uncertainty about the role of gravity at that time. Some reference Guth's suggestion of a repulsive form of gravity that drives inflation.
  • Current models typically utilize General Relativity, where the stress-energy tensor during inflation is dominated by the inflaton, with no change in gravity, and interactions occur through energy, momentum, pressure, and twisting forces.
  • Questions arise regarding whether the density of a black hole creates similar effects as the inflaton field, with one participant highlighting the unique properties of the inflaton field, characterized by negative pressure.
  • There is uncertainty about whether the energy driving the current expansion decays into particles, with some indicating that a well-supported model for this accelerated expansion is lacking.
  • During primordial inflation, it is acknowledged that the accelerated expansion did lead to the production of particles.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the interaction of inflatons and gravity, and the discussion remains unresolved on several points, particularly concerning the nature of gravity during inflation and the current expansion.

Contextual Notes

Limitations include unclear definitions of gravity's strength, the dependence on specific models of inflation, and unresolved questions about the decay of energy into particles during different phases of cosmic expansion.

Pjpic
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Is the theory that inflatons become dominate when gravity is strong (as in right after the big band) and when gravity is weak (as in driving the current expansion of the observable universe)?
 
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The thing that drove inflation in the very early universe, and the thing that is currently driving the accelerating expansion of the universe, are not necessarily the same thing; in fact, in our best current model they aren't.

Also, you need to clarify what you mean by gravity being "strong" or "weak".
 
Matter had not yet come into existence at the time of inflation, so the role of gravity during inflation is not entirely clear. Guth suggests a special case of gravity during inflation - a repulsive form that drives inflation. In his version the energy driving inflation decays into the hot particle soup of the classical big bang.
 
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Pjpic said:
Is the theory that inflatons become dominate when gravity is strong (as in right after the big band) and when gravity is weak (as in driving the current expansion of the observable universe)?
Current models typically make use of General Relativity, with the stress-energy tensor during inflation dominated by the inflaton. That is, inflation models have no change in gravity at all, and the inflaton interacts with gravity just like everything else: through energy, momentum, pressure, and twisting forces.
 
Chronos said:
Matter had not yet come into existence at the time of inflation, so the role of gravity during inflation is not entirely clear. Guth suggests a special case of gravity during inflation - a repulsive form that drives inflation. In his version the energy driving inflation decays into the hot particle soup of the classical big bang.

a) The density of a black hole doesn't create the same effect?

b) Does the energy driving the current expansion decay into particles?
 
Pjpic said:
a) The density of a black hole doesn't create the same effect?
Nope. The inflaton field is a bizarre creature with an unusual stress-energy content. In particular, p \propto -\rho: it is a perfect fluid with a negative pressure. In the limit that p = -\rho/3, the density \rho is constant.

b) Does the energy driving the current expansion decay into particles?
Do you mean the current accelerated expansion? Nobody knows because we lack a well-understood and well-supported model describing this accelerated expansion.

During primordial inflation, yes, that accelerated expansion did end in the production of particles.
 
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