Producing a scale-invariant spectrum of perturbations in a Hagedorn phase of string cosmology.
We study the generation of cosmological perturbations during the Hagedorn phase of string gas cosmology. Using tools of string thermodynamics we provide indications that it may be possible to obtain a nearly scale-invariant spectrum of cosmological fluctuations on scales which are of cosmological interest today. In our cosmological scenario, the early Hagedorn phase of string gas cosmology goes over smoothly into the radiation-dominated phase of standard cosmology, without having a period of cosmological inflation.
Nayeri
Ali
A
Jefferson Physical Laboratory, Harvard University, Cambridge, Massachusetts 02138, USA. nayeri@schwinger.harvard.edu
Brandenberger
Robert H
RH
Vafa
Cumrun
C