Quantisation of Parameters and the String Landscape Problem
arXiv:hep-th/0612149 · doi:10.1088/1475-7516/2007/05/005
Abstract
We broaden the domain of application of Brustein and de Alwis recent paper [1], where they introduce a (dynamical) selection principle on the landscape of string solutions using FRW quantum cosmology. More precisely, we (i) explain how their analysis is based in choosing a restrictive range of parameters, thereby affecting the validity of the predictions extracted and (ii) subsequently provide a wider and cohesive description, regarding the probability distribution induced by quantum cosmological transition amplitudes. In addition, employing DeWitt's argument [2] for an initial condition on the wave function of the Universe, we found that the string and gravitational parameters become related through interesting expressions involving an integer, suggesting a quantisation relation for some of the involved parameters.
15 pages, 9 figures, RevTeX 4. Discussion expanded and references added. Version to appear in JCAP
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- The quantum realm of the "Little Sibling" of the Big Rip singularity
- The interacting multiverse and its effect on the cosmic microwave background
- Quantisation of the holographic Ricci dark energy model
- Inflationary de Sitter solutions from superstrings
- Resonant structure of space-time of early universe
- Pre-inflation from the multiverse: Can it solve the quadrupole problem in the cosmic microwave background?
- Instanton transition in thermal and moduli deformed de Sitter cosmology
- What if? - Exploring the Multiverse through Euclidean wormholes