Uncovering the Optimal Epoch for Life in the Universe

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The discussion centers on the optimal epoch for life in the universe, highlighting a paper that suggests the current epoch is favorable due to the similar densities of matter and dark energy. This phenomenon, known as the cosmological coincidence problem, may be explained by a temporal selection effect, indicating that observers on terrestrial planets are statistically likely to find these densities comparable. The paper argues that the probability of such observations is high, given the age distribution of terrestrial planets. Additionally, the conversation touches on the intriguing coincidence between the derived age of the universe and the Hubble time, suggesting potential anthropic explanations for this alignment. Overall, the insights provided contribute to the ongoing exploration of the Anthropic Principle in cosmology.
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What epoch of the universe's evolution would be most conducive to life?
 
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An interesting queistion. http://www.phys.unsw.edu.au/~chas/resources/my/0703429.pdf" paper claims that about now is pretty good and argue that the co-incidence problem of the matter and vacuum ( or dark) energy densities can be explained by the fact that cosmologist would be most likely to exist at the epoch where the densities are similar.

I'm not endorsing their argument as such since I haven't read the paper in enough detail to be sure of the argument, but it is an interesting take on the Anthropic Principle.
 
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http://arxiv.org/astro-ph/0703429
The Cosmic Coincidence as a Temporal Selection Effect Produced by the Age Distribution of Terrestrial Planets in the Universe
Charles H. Lineweaver, Chas A. Egan
Submitted to ApJ

The energy densities of matter and the vacuum are currently observed to be of the same order of magnitude: (\Omega_{m 0} \approx 0.3) \sim (\Omega_{\Lambda 0} \approx 0.7). The cosmological window of time during which this occurs is relatively narrow. Thus, we are presented with the cosmological coincidence problem: Why, just now, do these energy densities happen to be of the same order? Here we show that this apparent coincidence can be explained as a temporal selection effect produced by the age distribution of terrestrial planets in the Universe. We find a large (\sim 0.68) probability that observations made from terrestrial planets will result in finding \Omega_m at least as close to \Omega_{\Lambda} as we observe today. Hence, we, and any observers in the Universe who have evolved on terrestrial planets, should not be surprised to find \Omega_m \sim \Omega_{\Lambda}. This result is relatively robust if the time it takes an observer to evolve on a terrestrial planet is less than \sim 10 Gyr

Lineweaver is one of the best expositors I know. His "inflation and the CMB" helped me and must helped a lot of people.
this is an interesting suggestion for solving the "coincidence problem"
whether or not it is right, I expect it is very clearly and understandably presented. first rate guy
 
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Would a similar anthropic argument explain the connected coincidental equality of the derived age of the universe (A) and Hubble time (HT) using the present best estimates of \Omega_{\Lambda}, \Omega_{DM}, \Omega_{m}?

Note: with an arbitrary proportion of DE and DM, which varies over cosmological time in the standard model, and with a flat universe, the derived age of the universe could be anything from
A > 2/3 HT to A => Infinity, whereas the present best values actually give a value of

A: Age of Universe = 13.81 Gyrs and
HT: Hubble Time = 13.89 Gyrs

Which is some coincidence!

The proportion of DE is constantly growing, because the density of matter (including DM) is \propto R^{-3}(t) whereas the density of DE is constant. The evolving relative abundance of DE and matter determines the age of the universe.

Therefore if this coincidence is significant, which calls for an explanation, one might suggest that either we exist only when the HT and A happen to be equal (an Anthropic explanation), or the relationship between DE and matter are such that they are always equal.

The latter would give a handle on a possible evolution of DE and therefore its nature.

Garth
 
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IIRC Steven Weinberg predicted the value of \Lambda (with about less than 20% deviation) before the SNIa observations making use of the anthropic argument only.
 
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Maybe there exist commonly physical models (including anthropic) that, like inflation, enact coincidences in cosmological quantities.
 
https://en.wikipedia.org/wiki/Recombination_(cosmology) Was a matter density right after the decoupling low enough to consider the vacuum as the actual vacuum, and not the medium through which the light propagates with the speed lower than ##({\epsilon_0\mu_0})^{-1/2}##? I'm asking this in context of the calculation of the observable universe radius, where the time integral of the inverse of the scale factor is multiplied by the constant speed of light ##c##.
The formal paper is here. The Rutgers University news has published a story about an image being closely examined at their New Brunswick campus. Here is an excerpt: Computer modeling of the gravitational lens by Keeton and Eid showed that the four visible foreground galaxies causing the gravitational bending couldn’t explain the details of the five-image pattern. Only with the addition of a large, invisible mass, in this case, a dark matter halo, could the model match the observations...
Hi, I’m pretty new to cosmology and I’m trying to get my head around the Big Bang and the potential infinite extent of the universe as a whole. There’s lots of misleading info out there but this forum and a few others have helped me and I just wanted to check I have the right idea. The Big Bang was the creation of space and time. At this instant t=0 space was infinite in size but the scale factor was zero. I’m picturing it (hopefully correctly) like an excel spreadsheet with infinite...

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