Comparative Quantum Cosmology: Causality, Singularity, and Boundary Conditions
Southern New Hampshire University
Computer Futures, Inc.
Woodbury University, Department of Physics
California State Unversity, Los Angeles
Last modified: October 26, 2007
In this review article we compare the recent work of Peter Lynds, "On a
finite universe with no beginning or end",(http://arxiv.org/abs/physics/0612053) , with that of Stephen Hawking,
primarily "Quantum Cosmology, M-Theory, and the Anthropic Principle", (http://www.hawking.org.uk/text/physics/quantum.html) and two foundational works by Sean M. Carroll and Jennifer Chen, "Does Inflation Provide Natural Conditions for the Universe",(Gen.Rel.Grav. 37 (2005) 1671-1674; Int.J.Mod.Phys. D14 (2005) 2335-2340x), and "Spontaneous Inflation and the Origin of the Arrow of Time", ( http://arxiv.org/abs/hep-th/0410270) in order to evaluate their comparative treatments of the nature and role of causality, time ordering, thermodynamic reversibility, singularities and boundary conditions in the formation of the early universe. We briefly reference Smolin and Kauffman's recent arguments with respect to possible processes of "evolutionary selection" in early universe formation as an alternative explanation to key elements of Hawking's earlier "M-Theory", and its attendant anthropic principle. We also briefly excerpt a short section of Smolin's recent work on topology in quantum loop gravity, simply as an illustrative example of the type of complex quantum topological transformation which he offers as a theoretical alternative to
string theory in quantum cosmology.