Cyclical Universe: Spontaneous Inflation & Time's Arrow

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Discussion Overview

The discussion revolves around the concept of spontaneous inflation and its implications for the arrow of time within the context of the universe's evolution. Participants explore theoretical aspects, critiques of inflation, and the relationship between quantum mechanics and cosmology.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants highlight the assumption of unitarity in the evolution of the comoving volume from the early universe to today, questioning its implications for the nature of inflation.
  • There is a discussion about the conservation of degrees of freedom and its relevance to the claim that the proto-inflationary patch and the current universe are the same system.
  • Participants express uncertainty regarding whether the universe can be considered a quantum system, particularly in the context of statistical mixtures and density matrices.
  • One participant mentions the maximum entropy of the universe and its relation to the total mass, suggesting that anomalies in the CMB anisotropy could provide insights into this topic.
  • There is a clarification regarding notational conventions for expressing scientific numbers, with participants discussing the potential for confusion in notation.
  • Some participants share personal anecdotes about their experiences with calculators and notation preferences, which leads to a light-hearted exchange.

Areas of Agreement / Disagreement

Participants generally express interest in the paper and its concepts, but there is no consensus on the assumptions regarding unitarity or the classification of the universe as a quantum system. The discussion remains unresolved on these critical points.

Contextual Notes

Participants note the complexity of the assumptions involved in the critique of inflation and the implications of unitarity, which are not fully explored or agreed upon.

Chronos
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This makes my 'interesting reads' selection list:

Spontaneous Inflation and the Origin of the Arrow of Time
http://arxiv.org/abs/hep-th/0410270
 
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Thank you for the reference, Chronos. This is actually a very interesting paper. I think I understood the main idea, although some aspects were not understandable for me. For example:

In any version of this critique of inflation, there is a crucially important assumption: that
the evolution of the comoving volume from the early universe to today is unitary (and hence
reversible). The assumption of unitarity seems innocuous, but is extremely profound in
this context; it underlies the claim that the small proto-inflationary patch and our current
universe are the same system, just in two different configurations.
An obvious prerequisite for unitary evolution is the conservation of the set of degrees
of freedom characterizing the system. Such an assumption is so deeply ingrained in our
understanding of dynamics that it is not usually spelled out explicitly, but in the case of an
expanding spacetime the issue is not so clear. Indeed, unitarity is directly at odds with the
reasoning behind the idea that it is much easier to begin inflation than to simply find the
universe in its current state: the assertion that there are not that many degrees of freedom
that need to be in their vacuum state in order for a small region to begin inflating. If the
evolution is truly unitary, there are a fantastically large number of such degrees of freedom,
I understand that in case of quantum systems, observables related by a unitary transformation have same spectrum. But I believe that in case of statistical mixtures the evolution is not unitary: as soon as one has two different density matrices, both cannot be related by a unitary transformation. If this is correct, shall I assume that the universe is considered as a quantum system? Why?
 
Thank you for the reference, Chronos. This is actually a very interesting paper. I think I understood the main idea, although some aspects were not understandable for me. For example:

In any version of this critique of inflation, there is a crucially important assumption: that the evolution of the comoving volume from the early universe to today is unitary (and hence reversible). The assumption of unitarity seems innocuous, but is extremely profound in this context; it underlies the claim that the small proto-inflationary patch and our current universe are the same system, just in two different configurations.
An obvious prerequisite for unitary evolution is the conservation of the set of degrees of freedom characterizing the system. Such an assumption is so deeply ingrained in our understanding of dynamics that it is not usually spelled out explicitly, but in the case of an expanding spacetime the issue is not so clear. Indeed, unitarity is directly at odds with the reasoning behind the idea that it is much easier to begin inflation than to simply find the universe in its current state: the assertion that there are not that many degrees of freedom that need to be in their vacuum state in order for a small region to begin inflating. If the evolution is truly unitary, there are a fantastically large number of such degrees of freedom,
I understand that in case of quantum systems, observables related by a unitary transformation have same spectrum. But I believe that in case of statistical mixtures the evolution is not unitary: as soon as one has two different density matrices, both cannot be related by a unitary transformation. If this is correct, shall I assume that the universe is considered as a quantum system? Why?
 
hellfire said:
Thank you for the reference, Chronos. This is actually a very interesting paper. I think I understood the main idea, although some aspects were not understandable for me. For example:

I understand that in case of quantum systems, observables related by a unitary transformation have same spectrum. But I believe that in case of statistical mixtures the evolution is not unitary: as soon as one has two different density matrices, both cannot be related by a unitary transformation. If this is correct, shall I assume that the universe is considered as a quantum system? Why?
I think that is an option still in play. Apparent anomalies in the CMB anisotropy could be an important piece in that puzzle. Did you happen to notice the curiously familiar number given for the maximum entropy of the universe -

The total amount of mass in the observable universe is ... ~10E22 [solar masses]. If all of this mass were collected into a single black hole, the entropy would be Smax(U) 10E121.
 
Last edited:
Chronos said:
..

The total amount of mass in the observable universe is ... ~10E22 [solar masses]. If all of this mass were collected into a single black hole, the entropy would be Smax(U) 10E121.

Hello Chronos, we have a potential bit of notational trouble
because of different conventions.
My casio "scientific" calculator and the old teletype version of BASIC and so many other people and things used (and still use) E22 to stand for 10^22
or 1022

so the "E" in the character string serves to replace the three characters
"10^"

It is an old, and I think honorable, convention. So I looked at Carroll's paper and on page 4, equations (5) and (6), he says that the
mass of the observable universe is, following the ancient honorable "E" tradition, E22 solar masses.

But you are using a different notational convention and say that he says
10E22 solar masses!

this I automatically read as 10 x 1022 = 1023

which is not what Carroll said. So there is a possibility for confusion.

I have a lot of writing invested in the old notational convention. If not too much trouble for you (if you have not already written many posts using your "E" which basically just means "^") could you change over?
 
I stand corrected. It's a habit I acquired using this calculator with an 'E' button that stood for exponent. Assuming I don't forget, I will amend my evil ways.
 
Chronos said:
I stand corrected. It's a habit I acquired using this calculator with an 'E' button that stood for exponent. Assuming I don't forget, I will amend my evil ways.

You are obliging and I thank you. Notation is just a question of habit, but it is less confusing when we adopt the same conventions. (I see we are both the slaves of our calculators)
 
marcus said:
You are obliging and I thank you. Notation is just a question of habit, but it is less confusing when we adopt the same conventions. (I see we are both the slaves of our calculators)
I still have trouble using regular calculators after years (late 70's to mid 80's) of my love affair with RPN. As a chemist in a pulp mill (with NO Personal Computer), I had to use those calculators a LOT. The programmable HPs were a lifesaver! The chemistry of a pulp mill is WAY complex. Why oh WHY did HP discontinue the wonderful HP15C? :cry: It's been years, but it's still a bummer. Perfect pocket size, lots of power... Oh well...
 
turbo-1 said:
I still have trouble using regular calculators after years (late 70's to mid 80's) of my love affair with RPN. As a chemist in a pulp mill (with NO Personal Computer), I had to use those calculators a LOT. The programmable HPs were a lifesaver! The chemistry of a pulp mill is WAY complex. Why oh WHY did HP discontinue the wonderful HP15C? :cry: It's been years, but it's still a bummer. Perfect pocket size, lots of power... Oh well...

I sympathize, but that doesn't do you any good, what you obviously want is not sympathy but an HP15C (with RPN of course, I had one too but it was a long time ago and I've adapted to "algebraic" notation) Ooops, I should get back on topic! mass and entropy-bound of observable U.
 

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