Inflation, Dark Matter, and Dark Energy in the String Landscape
Abstract
We consider the conditions needed to unify the description of dark matter, dark energy, and inflation in the context of the string landscape. We find that incomplete decay of the inflaton field gives the possibility that a single field is responsible for all three phenomena. By contrast, unifying dark matter and dark energy into a single field, separate from the inflaton, appears rather difficult.
- Publication:
-
Physical Review Letters
- Pub Date:
- October 2006
- DOI:
- 10.1103/PhysRevLett.97.161301
- arXiv:
- arXiv:astro-ph/0605205
- Bibcode:
- 2006PhRvL..97p1301L
- Keywords:
-
- 98.80.Cq;
- 95.35.+d;
- 95.36.+x;
- Particle-theory and field-theory models of the early Universe;
- Dark matter;
- Dark energy;
- Astrophysics;
- High Energy Physics - Phenomenology;
- High Energy Physics - Theory
- E-Print:
- 4 pages RevTex4. Updated to include a toy model of reheating. Matches version accepted by Phys Rev Lett