Axion and Almost Massless Quark as Ingredients of Quintessence
arXiv:hep-ph/9811509 · doi:10.1088/1126-6708/1999/05/022
Abstract
It is pointed out that a natural introduction of quintessence is an axion with an almost massless quark. With an appropriate gauge or discrete symmetry, one can obtain the quintessence potential height of order . Even though the QCD axion with almost massless up quark is a possibility, we stress the almost massless quark in the hidden sector together with the QCD axion toward the quintessence.
Latex file of 7 pages
Cited by in corpus (49)
- Generalized Chaplygin Gas, Accelerated Expansion and Dark Energy-Matter Unification
- Encyclopaedia Inflationaris
- Nonminimal coupling and quintessence
- Generalized Chaplygin gas and CMBR constraints
- WMAP Constraints on the Generalized Chaplygin Gas Model
- The Revival of the Unified Dark Energy-Dark Matter Model ?
- Latest Supernova data in the framework of Generalized Chaplygin Gas model
- Dark Matter from an ultra-light pseudo-Goldsone-boson
- String or M theory axion as a quintessence
- The Quest for an Intermediate-Scale Accidental Axion and Further ALPs
- Exhaustive Study of Cosmic Microwave Background Anisotropies in Quintessential Scenarios
- Loop Corrections to Scalar Quintessence Potentials
- Cosmological acceleration, varying couplings, and Lorentz breaking
- Expected constraints on the generalized Chaplygin equation of state from future supernova experiments and gravitational lensing statistics
- A Quintessential Axion
- SUSY QCD and Quintessence
- Supernovae Ia Constraints on a Time-Variable Cosmological "Constant"
- Detection of isotropic cosmic birefringence and its implications for axion-like particles including dark energy
- Quintessence Model With Double Exponential Potential
- A Two-Field Quintessence Model
- Model for self-tuning the cosmological constant
- Accions
- Correlated Isocurvature Fluctuation in Quintessence and Suppressed CMB Anisotropies at Low Multipoles
- O(N) quintessence
- Large-scale inhomogeneities in modified Chaplygin gas cosmologies
- Dark Energy and Right-Handed Neutrinos
- String compactification, QCD axion and axion-photon-photon coupling
- Abelian discrete symmetries Z_{N} and Z_{nR} from string orbifolds
- Implications of the Cosmic Birefringence Measurement for the Axion Dark Matter Search
- Self-tuning solution of the cosmological constant problem with antisymmetric tensor field
- Axionic dark energy and a composite QCD axion
- Cosmic Birefringence from Monodromic Axion Dark Energy
- Quintessence from Shape Moduli
- Cosmic Microwave Background Anisotropy with Cosine-Type Quintessence
- Modification of Decay Constants of Superstring Axions: Effects of Flux Compactification and Axion Mixing
- Gauge Quintessence
- Perturbations in a scalar field model with virtues of CDM
- Natural Higgs-flavor-democracy solution of the mu problem of supersymmetry and the QCD axion
- Confusing the extragalactic neutrino flux limit with a neutrino propagation limit
- Dark world and baryon asymmetry from a common source
- Quintessence as k-essence
- Gauged Quintessence
- WMAP Constraints on Quintessence
- Exit from inflation and a paradigm for vanishing cosmological constant in self-tuning models
- The variation of the electromagnetic coupling and quintessence
- The electromagnetic coupling and the dark side of the Universe
- Cosmological perturbations for ultra-light axion-like particles in a state of Bose-Einstein condensate
- Inflation with blowing-up solution of cosmological constant problem
- Double Higgs mechanisms, supermassive stable particles and the vacuum energy