arXiv · hep-th/0510219
Observational Consequences of Quantum Cosmology
Abstract
Our universe is born of a tunnelling from nothing in quantum cosmology. Nothing here can be interpreted as a state with zero entropy. As a reliable modification of the Hartle-Hawking wave function of the universe, the improved Hartle-Hawking wave function proposed by Firouzjahi, Sarangi and Tye gives many interesting observational consequences which we explore in this paper. Fruitful observations are obtained for chaotic inflation, including a detectable spatial curvature and a negligible tunnelling probability for eternal chaotic inflation. And we find that the tensor-scalar ratio and the spatial curvature for brane inflation type models should be neglected.
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Qing-Guo Huang. 2007-04-16. Observational Consequences of Quantum Cosmology. https://doi.org/10.1016/j.nuclphysb.2007.04.015
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