Exploring the Lambda Constant and the Big Bang Theory

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Discussion Overview

The discussion revolves around the lambda constant in cosmology, particularly its behavior during the early universe and its relationship to the inflationary epoch and the current accelerated expansion. Participants explore the implications of these concepts within the context of the Big Bang theory.

Discussion Character

  • Debate/contested
  • Conceptual clarification
  • Technical explanation

Main Points Raised

  • Some participants question whether the lambda constant's exponential growth during the first second of the universe was temporary, suggesting a need for specificity in the inquiry.
  • There is a distinction made between the inflationary epoch, which is associated with the inflaton field, and the cosmological constant (lambda), which is typically considered constant over time.
  • One participant notes that while inflation can be modeled with lambda, it is the scale factor that grows exponentially during inflation, not the lambda constant itself.
  • Another participant emphasizes that the universe has not been the same since the inflationary period, implying significant changes in its dynamics post-inflation.

Areas of Agreement / Disagreement

Participants express differing views on the nature of the lambda constant and its behavior during the early universe, indicating that multiple competing perspectives remain without consensus.

Contextual Notes

There are unresolved aspects regarding the definitions and implications of the lambda constant versus the inflaton field, as well as the conditions under which inflation occurs.

bobsmith76
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You know how the lambda constant just grew exponentially in the first second of the universe? That was just a temporary thing right?
 
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bobsmith76 said:
You know how the lambda constant just grew exponentially in the first second of the universe? That was just a temporary thing right?

Did it though? Think about it? Seriously hasn't it always been the same in one way. :wink:

I'm not sure what you are asking though as the first second contained an awful lot of stuff including some hyperinflation supposedly and the formation of atomic particles.

Could you rephrase it so you are being specific?
 
bobsmith76 said:
You know how the lambda constant just grew exponentially in the first second of the universe? That was just a temporary thing right?

Do you mean the inflationary epoch? Usually Lambda refers to cosmological *constant* with does not vary in time (there are various dark energy models that do vary in time, cosmological constant is only one of the many models to explain accelerated expansion in late time, i.e. now.) In the inflationary epoch, the inflation is supposedly caused by the inflaton field, which potential term is large and drives the inflation. That is different from Lambda.
 
As yenchin says, the inflationary expansion and the accelerated expansion of the modern epoch (perhaps due to lambda) are two separate things. Still, inasmuch as you can model inflation with lambda, such a constant in the early universe still could not have grown exponentially. Inflation has a rather strict requirement that the energy density (lambda) remain approximately constant during the expansion period. Instead, it is the scale factor, a(t), that grew exponentially during inflation: a(t) \propto e^{Ht}
 
bobsmith76 said:
You know how the lambda constant just grew exponentially in the first second of the universe? That was just a temporary thing right?

Yeah...and the Universe hasn't been the same SINCE.
 

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