Difference between revisions of "Research on free energy rate density"
From Evo Devo Universe
Clementvidal (talk | contribs) (→Problem) |
Clementvidal (talk | contribs) (→People Interested) |
||
| Line 24: | Line 24: | ||
== People Interested == | == People Interested == | ||
| − | Bela Nagy | + | * Bela Nagy |
| − | |||
| − | |||
| − | + | * John Smart | |
| − | |||
| − | |||
| + | * Clément Vidal | ||
| + | other researchers having published on this issue: | ||
| + | * Robert Aunger | ||
| + | * Eric Chaisson | ||
== Bibliography == | == Bibliography == | ||
Revision as of 16:03, 12 August 2009
Contents
Situation
A metric to characterize the complexity of physical, biological and cultural systems in the universe has been proposed by Chaisson (2001; 2003) (see below).
Problem
- How can we precise and work with this metric?
- What happens if we use this metric for the early universe?
- Can we complete the curve to understand the past (early universe) and to the future (acceleration of technology)?
Progressing on these issues
We are looking for cosmologists to use this metric on the early universe. We are looking for futurists and statisticians to extrapolate the curve to the future.
Benefits
Such a quantitative understanding will allow us to better characterize the evolution of complexity in our universe.
People Interested
- Bela Nagy
- John Smart
- Clément Vidal
other researchers having published on this issue:
- Robert Aunger
- Eric Chaisson
Bibliography
- Chaisson, E.J. (2001) Cosmic Evolution: The Rise of Complexity in Nature, Harvard U. Press. ISBN 067400342X
- Chaisson, E.J. (2003) A Unifying Concept for Astrobiology, International Journal of Astrobiology, 2:91-101.
