arXiv · hep-ph/9806327
Constraints on pre-big bang models for seeding large-scale anisotropy by massive Kalb-Ramond axions
Abstract
We discuss the conditions under which pre-big bang models can fit the observed large-scale anisotropy with a primordial spectrum of massive (Kalb--Ramond) axion fluctuations. The primordial spectrum must be sufficiently flat at low frequency and sufficiently steeper at high frequency. For a steep and/or long enough high-frequency branch of the spectrum the bounds imposed by COBE's normalization allow axion masses of the typical order for a Peccei--Quinn--Weinberg--Wilczek axion. We provide a particular example in which an appropriate axion spectrum is obtained from a class of backgrounds satisfying the low-energy string cosmology equations.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
M. Gasperini, G. Veneziano. 1998-06-09. Constraints on pre-big bang models for seeding large-scale anisotropy by massive Kalb-Ramond axions. https://doi.org/10.1103/physrevd.59.043503
Cite the original work for its findings. Save a collection to share your selection of sources.