Low-scale inflation in a model of dark energy and dark matter

Abstract

We present a complete particle physics model that explains three major problems of modern cosmology: inflation, dark matter and dark energy, and also gives a mechanism for leptogenesis. The model has a new gauge group $SU(2{)}_Z$ that grows strong at a scale $\Lambda \sim 10^{-3}$ eV. We focus on the inflationary aspects of the model. Inflation occurs with a Coleman-Weinberg potential at a low scale, down to $\sim 6\times 10^5\gev$, being compatible with observational data.

arXiv comment5 two-column pages, RevTex4; two reference added and minor changes made in the text; published in JCAP

References in corpus (11)

• Particle Physics Models of Inflation and the Cosmological Density Perturbation
• Reheating after Inflation
• Universe Reheating after Inflation
• The Cold Dark Matter Density Perturbation
• Quintessential inflation
• Deflationary Universe Scenario
• Modeling Quintessential Inflation
• On the Construction of Quintessential Inflation Models
• Coleman-Weinberg Potential In Good Agreement With WMAP
• A Model of Dark Energy and Dark Matter
• Unified Model for Inflation and Dark Energy with Planck-Scale Pseudo-Goldstone Bosons

Cited by in corpus (11)

• Higher Curvature Corrections to Primordial Fluctuations in Slow-roll Inflation
• Dynamical Dark Matter: II. An Explicit Model
• Metastability in Quadratic Gravity
• Phenomenological Constraints on Axion Models of Dynamical Dark Matter
• Mirror World and Superstring-Inspired Hidden Sector of the Universe, Dark Matter and Dark Energy
• Neutrino Condensate as Origin of Dark Energy
• Is Noncommutative Eternal Inflation Possible?
• The relic density of shadow dark matter candidates
• Majorana Neutrino Superfluidity and Stability of Neutrino Dark Energy
• Neutrino Phenomenology, Dark Energy and Leptogenesis from pseudo-Nambu-Goldstone Bosons
• Shadow Fermions, Messenger Scalars and Leptogenesis