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In the context of Inflationary Cosmology, it is postulated that there was a period of shrinking Hubble Sphere radius $(aH)^{-1}$.

$$ \frac{d}{dt} (aH)^{-1} < 0 $$

Then the regions of the universe which appear to us to not be in causal contact can indeed have been in causal contact at some (conformal? physical? I'm not sure. My intuition would be physical) time in the past.

This solves the Horizon Problem, namely that we observe a homogenous isotropic universe to one part in 10,000, yet it doesn't seem that all regions of the universe were in casual contact to achieve such a uniformity.

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Anyway, when this shrinking Hubble sphere radius $(aH)^{-1}$ is invoked, it has the result of pushing the Hot Big Bang singularity back to negative infinity conformal time.

It is this statement that I am having trouble grasping.

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Explicitly

$$ \chi_{PH}(\tau) = \tau - \tau_i = \int_{t_i}^{t} \frac{1}{a(t)} dt = \int_{a_i}^a (a H)^{-1} d\log(a) $$

where by Friedmann

$$ (aH)^{-1} \propto a^{\frac{1+3w}{2}} $$

giving

$$ \chi_{PH}(a(\tau)) = \tau - \tau_i \propto \frac{2}{1+3w} \left[ a(\tau)^{\frac{2}{1+3w}} - a_i^{\frac{2}{1+3w} } \right] $$

So for a strong energy violating fluid such that

$$ 1 + 3w < 0 $$

this becomes

$$ \tau_i \propto \frac{2}{1+3w} a_i^{\frac{2}{1+3w}} \rightarrow -\infty $$

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I understand the maths behind it, and can't argue against that the initial conformal time goes to minus infitity, but I don't know how to think about that.

In a standard Hot Big Bang the singularity occurs at $\tau_i = 0$ conformal time. This seems fine to me.

I am aware that conformal time is unphysical, but unless the scale factor goes negative, then negative conformal time suggests to me negative physical time.

And a negative scale factor would bring a whole other conceptual problem!

Namely, they are directly related by

$$ d\tau = \frac{1}{a(t)} dt $$

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So my questions are;

What does it mean to have negative conformal time?

And what does it mean to have negative infinity conformal time?

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Thanks

share|improve this question
    
Why negative time should be different from, let's say, negative x coordinate? (btw, I don't know the answer) –  Antonio Ragagnin May 9 at 13:31
    
@AntonioRagagnin : Well, for a start we know that the scale factor satisfies $$ a(t) \propto t^{\frac{2(1+w)}{3}} $$ or $$ a(\tau) \propto \tau^{\frac{2}{(1+3w}} $$ and so having negative physical time or conformal time would give a negative scale factor. I do not think this should be the case. Certainly I have never seen graphs or data for example that consider such a thing. Moreover, the idea of the scale of the universe being negative does not make sense, as I understand it... –  Flint72 May 9 at 14:19
    
@AntonioRagagnin : ...The scale of the universe is a measure of the expansion of the universe, that is, a measure of the conformal distance and physical distance between bodies. Distance is a scalar quantity, which cannot be negative. Take for example the simple case of a radial null geodesic $$ ds^2 = a^2(\tau) \left[ d\tau^2 - d\chi^2 \right] $$. Then a negative scale would be like a sphere with negative radius. It is not defined. –  Flint72 May 9 at 14:27

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