Quintessence, Flat Potential and String/M Theory Axion
Kiwoon Choi
Abstract
A slow-rolling scalar field (Quintessence) has been proposed as the origin of accelerating universe at present. We discuss some features of quintessence, particularly those related with the flatness of its potential. We distinguish two types of quintessences, a metrical quintessence which couples to the particle physics sector only through the mixing with the spacetime metric and a non-metrical one without such property. It is stressed that these two types of quintessences have quite different features in regard to the fine tuning of parameters required for the flat potential, as well as different implications for the quintessence-mediated long range force. The fine tuning argument strongly suggests that non-metrical quintessence should correspond to the Goldstone boson of an almost exact nonlinear global symmetry whose explicit breaking by quantum gravity effects is highly suppressed. It is briefly discussed whether the radion field in higher dimensional theories can be a candidate for metrical quintessence. We finally discuss the possibility that string/M theory axion corresponds to a Goldstone-type quintessence, and argue that a certain combination of the heterotic M theory or Type I string theory axions can be a good candidate for quintessence if some conditions on the moduli dynamics are satisfied.
Create a lesson
Related papers
Chiral soliton lattice in inhomogeneous magnetic fields
Tomas Brauner, Ramkumar Radhakrishnan
From the November Revolution toward the Millennium
Chris Quigg
An Axial UA(1)Lμ-Lτ: UV Completion and Experimental Searches
Rundong Fang, Jinhui Guo, Ming Li et al.
Hunting long-lived doubly charged scalars at the HL-LHC
Biplob Bhattacherjee, Rituparna Ghosh, Swagata Mukherjee et al.
Enigmatic properties of Ξ(1620) and Ξ(1690)
Taísa Veloso, K. P. Khemchandani, A. Martinez Torres et al.
Exploring Z/γ-mediated heavy FCNCs at the FCC-ee
Abhik Sarkar, Subhajit Kala, Amir Subba et al.