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6 - Fitness and the cosmic environment

Published online by Cambridge University Press:  18 December 2009

Paul C. W. Davies
Affiliation:
College of Liberal Arts and Sciences, Arizona State University
John D. Barrow
Affiliation:
University of Cambridge
Simon Conway Morris
Affiliation:
University of Cambridge
Stephen J. Freeland
Affiliation:
University of Maryland, Baltimore
Charles L. Harper, Jr
Affiliation:
John Templeton Foundation
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Summary

The problem of what exists: why this universe?

Einstein reportedly said: “What really interests me is whether God had any choice in the creation of the world”. What he meant by this informal remark was whether the physical universe must necessarily exist as it is or whether it could have been otherwise (or could have not existed at all). Today, almost all scientists believe that the universe could indeed have been otherwise; no logical reason exists why it has to be as it is. In fact, it is the job of the experimental scientist to determine which universe actually exists, from among the many universes that might possibly exist. And it is the job of the theoretician to construct alternative models of physical reality, perhaps to simplify or isolate a particular feature of interest. To be credible, these models must be mathematically and logically self-consistent. In other words, they represent possible worlds.

Let me give one example from my own research (Birrell and Davies, 1978). The equations of quantum field theory describing a system of interacting subatomic particles are often mathematically intractable. But several “toy models” exist, the equations for which may be solved exactly because of special mathematical features. One of these, known as the Thirring model, describes a two-spacetime-dimensional world inhabited by self-interacting fermions. This impoverished model of reality is designed to capture some features of interest to physicists in the real world. It is not, obviously, an attempt to describe the real world in its entirety.

Type
Chapter
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Fitness of the Cosmos for Life
Biochemistry and Fine-Tuning
, pp. 97 - 113
Publisher: Cambridge University Press
Print publication year: 2007

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References

Abbot, D., Davies, P. C. W. and Pati, A. (2008). Quantum Aspects of Biology. London: Imperial College Press.CrossRefGoogle Scholar
Barrow, J. (1991). Pi in the Sky. Oxford: Oxford University Press.Google Scholar
Barrow, J. (2003). Glitch. New Scientist (7 June), p. 44.Google Scholar
Barrow, J. D. and Tipler, F. J. (1986). The Anthropic Cosmological Principle. Oxford: Oxford University Press.Google Scholar
Birrell, N. D. and Davies, P. C. W. (1978). Massless Thirring model in curved space: thermal states and conformal anomaly. Physical Reviews D18, 4408.Google Scholar
Bostrom, N. (2003). Are we living in a computer simulation?Philosophical Quarterly, 53 (211), 243.CrossRefGoogle Scholar
Brock, G. R. and Goode, J. A., eds. (1996). Evolution of Hydrothermal Ecosystems on Earth (and Mars?). New York, NY: Wiley.Google Scholar
Chaitin, G. (1988). Randomness in arithmetic. Scientific American, 259 (1), 80.CrossRefGoogle Scholar
Chapelle, F. H.et al. (2002). A hydrogen-based subsurface microbial community dominated by methanogens. Nature, 415, 312.CrossRefGoogle ScholarPubMed
Davies, P. (1991). The Mind of God. London and New York: Simon and Schuster.Google Scholar
Davies, P. (2003). The Origin of Life. London: Penguin.Google Scholar
Davies, P. C. W. (2004). Does quantum mechanics play a non-trivial role in life?BioSystems, 78, 69.CrossRefGoogle ScholarPubMed
Davies, P. (2006). The Goldilocks Enigma: Why the Universe Is Just Right for Life. London: Penguin Books.Google Scholar
Davies, P. (2007). Cosmic Jackpot. London: Penguin Books.Google Scholar
Freund, F., Dickinson, J. T. and Cash, M. (2002). Hydrogen in rocks: an energy source for deep microbial communities. Astrobiology, 2, 83.CrossRefGoogle ScholarPubMed
Greene, B. (2000). The Elegant Universe. New York, NY: Vintage.Google Scholar
Haught, J. (1986). What Is God?New York, NY: Paulist Press.Google Scholar
Hawking, S. (1988). A Brief History of Time. New York, NY: Bantam, p. 174.Google Scholar
Henderson, L. J. (1913). The Fitness of the Environment: An Inquiry into the Biological Significance of the Properties of Matter. New York: Macmillan. Repr. (1958) Boston, MA: Beacon Press; (1970). Gloucester, MA: Peter Smith.Google Scholar
Kauffman, S. A. (1993). The Origins of Order. Oxford: Oxford University Press.Google Scholar
Kolesnikov, A. I., Zanotti, J., Loong, C.et al. (2004). Anomalously soft dynamics of water in a nanotube: a revelation of nanoscale confinement. Physical Review Letters, 93, 035503.CrossRefGoogle Scholar
Linde, A. (1990). Inflation and Quantum Cosmology. Boston, MA: Academic Press.CrossRefGoogle Scholar
Maher, K. and Stephenson, D. (1988). Impact frustration of the origin of life. Nature, 331, 612.CrossRefGoogle ScholarPubMed
Morowitz, H. J.et al. (2000). The origin of intermediary metabolism. Proceedings of the National Academy of Sciences, USA, 97, 7704.CrossRefGoogle ScholarPubMed
Pešić, P. D. (1993). The smallest clock. European Journal of Physics, 14, 90.CrossRefGoogle Scholar
Postgate, J. (1996). The Outer Reaches of Life. Cambridge, UK: Cambridge University Press. See also Online Extreme Environments articles: www.lyon.edu/projects/marsbugs/extreme.html.Google Scholar
Ragenauer-Lieb, K., Yuen, D. and Branlund, J. (2001). The initiation of subduction: criticality by addition of water?Science, B294, 578.CrossRefGoogle Scholar
Rees, M. (2001). Our Cosmic Habitat. Princeton, NJ: Princeton University Press.Google Scholar
Rees, M. (2003). Interview. Edge 116 (19 May).Google Scholar
Shi, T.et al. (1997). Characterization of viable bacteria from Siberian permafrost by 16S rDNA sequencing. Microbial Ecology, 33, 169.CrossRefGoogle ScholarPubMed
Sleep, N., Zahnle, K. and Kasting, J. (1989). Annihilation of ecosystems by large asteroid impacts on the early Earth. Nature, 342, 139.CrossRefGoogle ScholarPubMed
Susskind, L. (2005). The Cosmic Landscape: String Theory and the Illusion of Intelligent Design. New York: Little Brown.Google Scholar
Swinburne, R. (1993). The Coherence of Theism, rev. edn. Oxford: Clarendon Press.CrossRefGoogle Scholar
Tegmark, M. (2003). Parallel universes. Scientific American, May, 40 (cover story).CrossRef
Tegmark, M. (2004). Parallel universes. In Science and Ultimate Reality: Quantum Theory, Cosmology and Complexity, ed. Barrow, J. D., Davies, P. C. W. and Harper, C. L. Jr.Cambridge, UK: Cambridge University Press, p. 459.CrossRefGoogle Scholar

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