Unparticles and inflation
arXiv:0802.4416 · doi:10.1103/PhysRevD.78.025023
Abstract
We study some of the roles for unparticles in an inflationary universe. Unparticles by themselves are not appropriate for generating the primordial perturbations since their power spectrum does not match what has been inferred from observations. In fact, when the scaling dimension for the unparticles exceeds three-halves, the unparticle power spectrum diverges. However, when a unparticle couples to an ordinary inflaton particle, loop corrections can produce a slight enhancement of the inflaton's power spectrum at longer wavelengths. We examine these loop corrections from unparticles in some detail to learn how they scale in the wavelength of a perturbation and how they depend on the scaling dimension of the field.
10 pages, 3 eps figures, uses ReVTeX; replaced with published version
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- Oscillation dynamics of active-unsterile neutrino mixing in a mixing scheme
- Unsterile-Active Neutrino Mixing: Consequences on Radiative Decay and Bounds from the X-ray Background
- Unparticle effects in neutrino telescopes
- Unparticles: Interpretation and Cosmology
- Strongly Coupled Sectors in Inflation: Gapless Theories and Unparticles