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This is a Blog on relativity and cosmology for engineers and the like. My website "Relativity-4-Engineers" has more in-depth stuff.

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Cosmology Equations Part 2

Posted October 18, 2006 12:58 PM by Jorrie

In the introductory part, the shape of the cosmic expansion parabola and 'tear drop' shape of the observable universe were shown. The parabola depends on the expansion model used - in this case the so-called "Einstein-De Sitter" model, which is a universe with enough matter to make it 'flat', with no cosmological constant.

The 'expansion law' of the Einstein-De Sitter model is particularly simple, given by:

where dt is a time differential, a the expansion factor and H0 the Hubble constant. The expansion factor is a linear scalar that today has the value a = 1. At the Big Bang, a = 0 and when the observable universe was half as large as it is now, a was 0.5.

This equation can be easily integrated against time, from t = 0 to t, to get:

which can be used to get the age of the "Einstein-De Sitter universe". In the days when it was believed that H0 = 50 km/s/Mpc, this gave an age of the universe of about 13 Gy. (A Mpc is about 3.2 million light-years).

Surprisingly, this is more or less the age that cosmologists agree upon today, except that it is coming from a different value for H0 (about 72 km/s/Mpc) and a very different model! In the coming parts of this mini-series, the reasons why a different model was required will be discussed.

PS. I am taking a long-weekend, away from projects and computers. Will be back on Tuesday 24th. If you have questions, I'll attempt answers them then! The equations obviously come from Relativity 4 Engineers (where else?)

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#1

Re: Cosmology Equations Part 2

10/19/2006 5:42 AM

My maths is shaky but I can follow your formula OK. But it does seem you assume a value for 'a' at the beginning of time to give the answer you want.

But whatever the scientific basis for 'a', my problem lies with the phylosophy because I find it difficult to grasp the concept of 'nothing' in a 3+1 dimensional world, where 'a' seems to be a value occuring at a point just after 'nothing' ends. Which then puts us into beginning of 'infinity' where 'forever' is another difficult concept to grasp.

I do not expect an answers as such. I just wondered.

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#4
In reply to #1

Re: Cosmology Equations Part 2

10/23/2006 11:46 AM

Quoting horace40: ". . .But it does seem you assume a value for 'a' at the beginning of time to give the answer you want. . . . But whatever the scientific basis for 'a', my problem lies with the philosophy because I find it difficult to grasp the concept of 'nothing' in a 3+1 dimensional world, where 'a' seems to be a value occurring at a point just after 'nothing' ends."

The expansion factor 'a' is not really a dimension. It just says that if a = 1 today, then long ago, 'a' must have been very much smaller than 1. The smallest 'a' that has been measured is in fact about: a = 1/1100 (one-eleven-hundredth) which represents the time when (at least our part of) the universe first became transparent.

Further, the hypothetical case of "a=0" simply means "before expansion started", about which can only be hypothesized - so try not to develop a headache about it!

Jorrie

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#2

Re: Cosmology Equations Part 2

10/19/2006 2:34 PM

Jorrie,

This question a not related directly to the immediate post but one that has come up for me several times. It has to do with what a geodesic is.

Is a geodesic the shortest path between two points in a given space. In other words, would the geodesic of a region of space with no gravity (flat space) just be a straight line? Is it more complicated than that (not just the shortest distance).

Sorry if this is a bit off topic,

Roger

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#3
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Re: Cosmology Equations Part 2

10/23/2006 11:14 AM

Hi Roger, you asked: "Is a geodesic the shortest path between two points in a given space."

Not necessarily. See below.

"In other words, would the geodesic of a region of space with no gravity (flat space) just be a straight line?"

In this case, yes.

A geodesic is really the path of least action and not the shortest path in general. In a gravity-free environment, it is a straight line and in a gravitational field it is not. An inertial orbit around Earth follows a space-time geodesic and it is easy to see that it is neither a straight line in space, nor the shortest spatial distance between two arbitrary points lying on the orbit.

Remember that in relativistic gravitation theory, what is normally considered is space-time, so what matters there is space-time geodesics, but they follow the same basic principle of least action.

Hope it helps. Jorrie

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#5

Re: Cosmology Equations Part 2

11/13/2006 1:30 PM

Jorrie,

where does this equation come from? Is it derived from something fundamental in relativity?

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#6
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Re: Cosmology Equations Part 2

11/13/2006 2:08 PM

Hi Roger, no it is not a specific relativistic requirement. The equation you refer to is loosely described in the eBook on page 177, coming from:

which is the square root of an energy divided by a 'distance'. The Einstein-de Sitter model deals with a universe that is precisely balanced between collapse and 'escape' (expanding forever), much like an escape velocity.

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#7
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Re: Cosmology Equations Part 2

11/13/2006 3:16 PM

That really gave me a lot of insight. Thanks Jorrie. I'll have to think about this a bit.

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