Uncovering the Optimal Epoch for Life in the Universe

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In summary, the author suggests that the anthropic argument can explain the coincidence problem of the matter and vacuum energy densities. They argue that because terrestrial planets are distributed in the universe in a way that produces this coincidence, we should not be surprised by the observed energy densities.
  • #1
Loren Booda
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What epoch of the universe's evolution would be most conducive to life?
 
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  • #2
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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  • #3
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: [tex](\Omega_{m 0} \approx 0.3) \sim (\Omega_{\Lambda 0} \approx 0.7)[/tex]. 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 ([tex]\sim 0.68[/tex]) probability that observations made from terrestrial planets will result in finding [tex]\Omega_m[/tex] at least as close to [tex]\Omega_{\Lambda}[/tex] as we observe today. Hence, we, and any observers in the Universe who have evolved on terrestrial planets, should not be surprised to find [tex]\Omega_m \sim \Omega_{\Lambda}[/tex]. This result is relatively robust if the time it takes an observer to evolve on a terrestrial planet is less than [tex]\sim 10[/tex] 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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  • #4
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 [itex]\Omega_{\Lambda}[/itex], [itex]\Omega_{DM}[/itex], [itex]\Omega_{m}[/itex]?

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 [itex]\propto R^{-3}(t)[/itex] 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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  • #5
IIRC Steven Weinberg predicted the value of [itex]\Lambda[/itex] (with about less than 20% deviation) before the SNIa observations making use of the anthropic argument only.
 
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  • #6
Maybe there exist commonly physical models (including anthropic) that, like inflation, enact coincidences in cosmological quantities.
 

1. What is the optimal epoch for life in the universe?

The optimal epoch for life in the universe refers to the time period during which conditions were most favorable for the emergence and sustenance of life on Earth. This is typically considered to be around 3.5-4 billion years ago, when early life forms such as bacteria and archaea first appeared and began to thrive.

2. How do scientists determine the optimal epoch for life in the universe?

Scientists use various methods to determine the optimal epoch for life in the universe, including studying geological and fossil records, analyzing the chemical composition of ancient rocks, and studying the evolution of early life forms. These methods provide clues about the conditions that were present during different time periods and help us understand when life may have first emerged.

3. What factors contribute to the optimal epoch for life in the universe?

Several factors contribute to the optimal epoch for life in the universe, including the availability of liquid water, a stable and moderate climate, and the presence of essential elements and compounds necessary for life to thrive. Other factors, such as the presence of a protective atmosphere and the absence of catastrophic events, also play a role.

4. Could there be other optimal epochs for life in the universe?

It is possible that there could be other optimal epochs for life in the universe, depending on the conditions present on other planets or moons. Some scientists speculate that there may have been other periods in Earth's history, such as during the Cambrian explosion, when life flourished and conditions were conducive to its development. Additionally, there may be other planets or moons in our own solar system or in other star systems that have or had their own optimal epochs for life.

5. How does studying the optimal epoch for life in the universe help us understand the origins of life?

Studying the optimal epoch for life in the universe provides valuable insights into the conditions that were necessary for life to emerge on Earth. By understanding the factors that contributed to the development of life in our own planet's history, scientists can better understand the potential for life to arise on other planets or moons in the universe. This knowledge can also inform our search for habitable exoplanets and our understanding of the origins of life in the universe.

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