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Accelerating Expansion

Philosophy and Physics with a Positive Cosmological Constant

Belot, Prof Gordon (Lawrence Sklar Collegiate Professor of Philosophy, Lawrence Sklar Collegiate Professor of Philosophy, University of Michigan)

Accelerating Expansion

Accelerating Expansion

Philosophy and Physics with a Positive Cosmological Constant

Accelerating Expansion

 

Accelerating Expansion explores some of the philosophical implications of modern cosmology, focused on the significance that the discovery of the accelerating expansion of the Universe has for our understanding of time, geometry, and physics.


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Beschrijving Accelerating Expansion

Accelerating Expansion explores some of the philosophical implications of modern cosmology, focused on the significance that the discovery of the accelerating expansion of the Universe has for our understanding of time, geometry, and physics. The appearance of the cosmological constant in the equations of general relativity allows one to model universes in which space has an inherent tendency towards expansion. This constant, introduced by Einstein but subsequently abandoned by him, returned to centre stage with the discovery of the accelerating expansion. This pedagogically-oriented essay begins with a study of the most basic and elegant relativistic world that involves a positive cosmological constant, de Sitter spacetime. It then turns to the relatives of de Sitter spacetime that dominate modern relativistic cosmology. Some of the topics considered include: the nature of time and simultaneity in de Sitter worlds; the sense in which de Sitter spacetime is a powerful dynamical attractor; the limited extent to which observation can give us information about the topology of space in a world undergoing accelerated expansion; and cosmologists' favourite sceptical worry about the reliability of evidence and the possibility of knowledge, the problem of Boltzmann brains.


ISBN
9780192866462
Pagina's
240
Verschenen
NUR
910
Druk
1
Uitvoering
Hardback
Taal
Engels
Uitgever
OUP Oxford

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