Do We Live in a Vanilla Universe? Theoretical Perspectives on WMAP
Abstract
I discuss the theoretical implications of the WMAP results, stressing WMAP's detection of a correlation between the E-mode polarization and temperature anisotropies, which provides strong support for the overall inflationary paradigm. I point out that almost all inflationary models have a ``vanilla limit,'' where their parameters cannot be distinguished from a genuinely de Sitter inflationary phase. Because its findings are consistent with vanilla inflation, WMAP cannot exclude entire classes of inflationary models. Finally, I summarize hints in the current dataset that the CMB contains relics of new physics, and the possibility that we can use observational data to reconstruct the inflaton potential.
- Publication:
-
Intersections of Particle and Nuclear Physics
- Pub Date:
- February 2004
- DOI:
- 10.1063/1.1664199
- arXiv:
- arXiv:astro-ph/0308160
- Bibcode:
- 2004AIPC..698...64E
- Keywords:
-
- 12.10.-g;
- 98.80.Cq;
- 98.80.Es;
- Unified field theories and models;
- Particle-theory and field-theory models of the early Universe;
- Observational cosmology;
- Astrophysics
- E-Print:
- 10 pages, based on paper delivered at CIPANP 2003