Biswas, Tirthabir and Brandenberger, Robert and Mazumdar, Anupam and Siegel, Warren (2007) Non-perturbative gravity, Hagedorn bounce and the cosmic microwave background. Journal of Cosmology and Astroparticle Physics, 2007 (12). 011. ISSN 1475-7516Full text not available from this repository.
In Biswas et al (2006 J. Cosmol. Astropart. Phys. JCAP03(2006)009 [hep-th/0508194]) it was shown how non-perturbative corrections to gravity can resolve the big bang singularity, leading to a bouncing universe. Depending on the scale of the non-perturbative corrections, the temperature at the bounce may be close to or higher than the Hagedorn temperature. If matter is made up of strings, then massive string states will be excited near the bounce, and the bounce will occur inside (or at the onset of) the Hagedorn phase for string matter. As we discuss in this paper, in this case cosmological fluctuations can be generated via the string gas mechanism recently proposed in Nayeri et al (2005 Preprint hep-th/0511140). In fact, the model discussed here demonstrates explicitly that it is possible to realize the assumptions made in Nayeri et al (2005 Preprint hep-th/0511140) in the context of a concrete set of dynamical background equations. We also calculate the spectral tilt of thermodynamic stringy fluctuations generated in the Hagedorn regime in this bouncing universe scenario. Generally we find a scale-invariant spectrum with a red tilt which is very small but does not vanish.
|Journal or Publication Title:||Journal of Cosmology and Astroparticle Physics|
|Additional Information:||25 pages, 1 figure|
|Uncontrolled Keywords:||quantum gravity phenomenology ; string theory and cosmology ; physics of the early universe ; gravity|
|Departments:||Faculty of Science and Technology > Physics|
|Deposited By:||Dr Anupam Mazumdar|
|Deposited On:||27 Jan 2010 16:48|
|Last Modified:||27 Apr 2017 01:41|
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