David Bourget (Western Ontario)
David Chalmers (ANU, NYU)
Rafael De Clercq
Ezio Di Nucci
Jack Alan Reynolds
Learn more about PhilPapers
One of the outstanding achievements of recent cosmology has been to offer some prospect of a unified explanation of temporal asymmetry. The explanation is in two main parts, and runs something like this. First, the various asymmetries we observe are all thermodynamic in origin – all products of the fact that we live in an epoch in which the universe is far from thermodynamic equilibrium. Second, this thermodynamic disequilibrium is associated with the condition of the universe very soon after the Big Bang – the essential point being that in the rapidly expanding universe of the time, gravity is able to create organisation much faster than other processes can destroy it. The stars, galaxies and other forms of organisation we find in the present universe are all products of this early period. Such concentrated energy sources themselves make possible the kinds of asymmetric phenomena with which we are most familiar, such as life itself. If this explanation proves to be right it will surely rank as one of the most impressive achievements in the whole of natural philosophy. Where else do we find this breathtaking scale, this extraordinary conjunction of fundamental physics, the first moments of Creation, the possibility of life and the basic character of human experience? And it is very much a contemporary achievement: even if its roots go back on one side to the investigation of time asymmetry in nineteenth century statistical mechanics, and on the other to Hubble's discovery in the 1920's of the expansion of the universe, the body of the picture has only begun to be filled in in the last twenty or thirty years. This fascinating story has recently been given some well-deserved publicity in Stephen Hawking's bestseller, A Brief History of Time – well-deserved, not least, because Hawking himself is responsible for a considerable part of the story as it presently stands
|Keywords||No keywords specified (fix it)|
|Categories||categorize this paper)|
Setup an account with your affiliations in order to access resources via your University's proxy server
Configure custom proxy (use this if your affiliation does not provide a proxy)
|Through your library||
References found in this work BETA
No references found.
Citations of this work BETA
No citations found.
Similar books and articles
Huw Price (2002). Boltzmann's Time Bomb. British Journal for the Philosophy of Science 53 (1):83-119.
Ernan McMullin (2005). Anthropic Explanation in Cosmology. Faith and Philosophy 22 (5):601-614.
Quentin Smith (1997). Simplicity and Why the Universe Exists. Philosophy 72 (279):125 - 132.
Craig Callender, Thermodynamic Asymmetry in Time. Stanford Encyclopedia of Philosophy.
Jill North (2011). Time in Thermodynamics. In Criag Callender (ed.), The Oxford Handbook of Philosophy of Time. Oxford 312--350.
Owen Maroney (2010). Does a Computer Have an Arrow of Time? Foundations of Physics 40 (2):205-238.
Pierre Uzan (2007). The Arrow of Time and Meaning. Foundations of Science 12 (2):109-137.
Huw Price (1996). Time's Arrow & Archimedes' Point: New Directions for the Physics of Time. Oxford University Press.
Christopher Potter (2009). You Are Here: A Portable History of the Universe. Harpercollins Publishers.
Added to index2011-04-02
Total downloads180 ( #19,065 of 1,796,330 )
Recent downloads (6 months)6 ( #136,215 of 1,796,330 )
How can I increase my downloads?