Linking Light Scalar Modes with A Small Positive Cosmological Constant in String Theory
arXiv:1611.05786 · doi:10.1007/JHEP06(2017)094
Abstract
Based on the studies in Type IIB string theory phenomenology, we conjecture that a good fraction of the meta-stable de Sitter vacua in the cosmic stringy landscape tend to have a very small cosmological constant when compared to either the string scale or the Planck scale , i.e., . These low lying de Sitter vacua tend to be accompanied by very light scalar bosons/axions. Here we illustrate this phenomenon with the bosonic mass spectra in a set of Type IIB string theory flux compactification models. We conjecture that small with light bosons is generic among de Sitter solutions in string theory; that is, the smallness of and the existence of very light bosons (may be even the Higgs boson) are results of the statistical preference for such vacua in the landscape. We also discuss a scalar field model to illustrate how this statistical preference for a small remains when quantum loop corrections are included, thus bypassing the radiative instability problem.
35 pages, 7 figures; added subsection: Finite Temperature and Phase Transition
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