Was the Big Bang a Low Entropy State in the Universe?

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Discussion Overview

The discussion centers around the concept of entropy in relation to the Big Bang, specifically whether the Big Bang can be considered a low entropy state in the universe. Participants explore theoretical implications, cosmological models, and the relationship between entropy and the direction of time, with references to the standard cosmological model and ideas proposed by Roger Penrose.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification
  • Technical explanation

Main Points Raised

  • One participant notes that according to the standard cosmological model, as one approaches the Big Bang, the universe is radiation-dominated, leading to a constant entropy value, which they argue seems incorrect.
  • Another participant questions the expectation that entropy should approach zero as one approaches the Big Bang.
  • It is mentioned that the early radiation-dominated expansion was adiabatic, suggesting that entropy behavior may differ from initial assumptions.
  • Some participants reference Roger Penrose's idea that the Big Bang was a low entropy state, arguing that the uniformity and isotropy of the universe today could indicate it started in a highly ordered state.
  • There is a claim that if entropy were constant, it would imply a lack of direction for time, which is argued to be necessary in both the radiation-dominated and matter-dominated eras.
  • Another participant asserts that the universe must have started in a low-entropy state, as entropy is understood to always increase over time.
  • Concerns are raised about the implications of a universe composed solely of radiation, suggesting that without other forms of matter, the concept of time's direction becomes meaningless.

Areas of Agreement / Disagreement

Participants express differing views on the nature of entropy at the Big Bang, with some supporting the idea of a low entropy state while others challenge the assumptions behind constant entropy. The discussion remains unresolved, with multiple competing perspectives presented.

Contextual Notes

Participants reference the standard cosmological model and various interpretations of entropy without reaching a consensus on the implications of these ideas. The discussion highlights the complexity of entropy's role in cosmology and its relationship to time.

johne1618
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I understand that the standard cosmological model says that as one goes back in time towards the big bang the Universe is radiation-dominated. This means that the mass/energy density, rho, in the universe is given by the Stephan Boltzmann law:

rho = T^4

where T is the temperature of radiation in the Universe and "=" means proportional.

Now the temperature T is inversely proportional to the size of the Universe R so we have:

T = R^-1

Thus

rho = R^-4

Now the total energy of the Universe, E, is the energy density times R^3:

Therefore:

E = R^-1

Now the entropy of the Universe S is given by its total energy E divided by its temperature T:

S = E / T

S = R^-1 / R^-1 = 1

Thus as you go back to the beginning of the Universe the standard cosmology says the entropy is constant.

But this must be wrong.

Surely we expect the entropy to go to zero as we go back to the big bang?
 
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Why would you expect that?
 
johne1618 said:
Thus as you go back to the beginning of the Universe the standard cosmology says the entropy is constant.

But this must be wrong.

Surely we expect the entropy to go to zero as we go back to the big bang?
No, the early radiation-dominated expansion was indeed adiabatic.
 
I understand that Roger Penrose for example likes the idea that the Big Bang was a low entropy state. The fact that the Universe is so uniform and isotropic now could be due to it starting in a very ordered state. You can't get more ordered than zero entropy!

Also if entropy is constant we would not have a direction for time. We need a direction for time in the radiation-dominated era as much as the present matter-dominated era.
 
Last edited:
johne1618 said:
I understand that Roger Penrose for example likes the idea that the Big Bang was a low entropy state. The fact that the Universe is so uniform and isotropic now could be due to it starting in a very ordered state. You can't get more ordered than zero entropy!

Also if entropy is constant we would not have a direction for time. We need a direction for time in the radiation-dominated era as much as the present matter-dominated era.
It's not just Penrose. That our universe started in a low-entropy state is a necessary truth because of what we say when we mean "entropy": overall, entropy always increases into the future. Therefore it must have been much lower in the past.

As for the direction of time, if your universe is actually made of pure radiation, there is no direction of time, because the expansion is meaningless. It is only the existence of other forms of matter that makes the expansion meaningful.
 

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