Yoshinobu Habara, Hikaru Kawai, Masao Ninomiya, Yasuhiro Sekino
We propose a mechanism for the generation of temperature fluctuations of
cosmic microwave background. We consider a large number of fields, such as
Kaluza-Klein modes and string excitations. Each field contributes to the
gravitational potential by a small amount, but an observable level of
temperature fluctuations is achieved by summing up the contribution of
typically of order 10^{14} fields. Tensor fluctuations are hardly affected by
these fields. Our mechanism is based on purely quantum effects, and is
different from the "slow-roll" or "curvaton" scenario. Using the observed data,
we find constraints on the parameters of this model, such as the size of the
extra dimensions and the string scale. Our model predicts a particular pattern
of non-gaussianity with a small magnitude.
View original:
http://arxiv.org/abs/1103.0299
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