Quintessential inflation with canonical and noncanonical scalar fields and Planck 2015 results
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology2015Vol. 92(2)
Citations Over TimeTop 10% of 2015 papers
Abstract
We investigate two classes of models of quintessential inflation, based upon canonical as well as noncanonical scalar fields. In particular, introducing potentials steeper than the standard exponential, we construct models that can give rise to a successful inflationary phase, with signatures consistent with Planck 2015 results. Additionally, using nonminimal coupling of the scalar field with massive neutrino matter, we obtain the standard thermal history of the Universe, with late-time cosmic acceleration as the last stage of evolution. In both cases, inflation and late-time acceleration are connected by a tracker solution.
Related Papers
- General Relativity from Planck-Satellite-Data(2014)
- → The Planck mass as a function of extra space volume(2009)
- Developing an equation to compute the wavelength ( g(2013)
- ON PLANCK′S MASS(2002)
- → The Relationship of Planck Constants and Wave Constants(2020)