Weighing the string mass with the COBE data
摘要
In the context of the pre-big bang scenario the large-scale CMB anisotropy can be seeded by a primordial background of very light (or massless) axion fluctuations. In that case the slope of the temperature anisotropy spectrum, allowed by present observations, defines an allowed range of values for the string mass scale. Conversely, from the theoretical expected value of the string scale we can predict the slope of the anisotropy spectrum. In both cases there is a remarkable agreement between observations and theoretical expectations.
引用
@article{arxiv.gr-qc/9806073,
title = {Weighing the string mass with the COBE data},
author = {M. Gasperini},
journal= {arXiv preprint arXiv:gr-qc/9806073},
year = {2007}
}
备注
14 pages, latex, five figures included using epsf. Talk given at the"Fifth Paris Cosmology Colloquium" (Observatoire de Paris, 3-5 June 1998). To appear in the Proceedings (World Scientific, Singapore), ed. by H. J. De Vega and N. Sanchez. An updated collection of papers on the pre-big bang scenario is available at http://www.to.infn.it/~gasperin