CMB Fluctuations and String Compactification Scales
Yoshinobu Habara, Hikaru Kawai, Masao Ninomiya, Yasuhiro Sekino

TL;DR
This paper introduces a quantum-based mechanism involving numerous string-related fields to explain cosmic microwave background temperature fluctuations, providing new constraints on extra dimensions and string scales.
Contribution
It presents a novel quantum mechanism for CMB fluctuations involving a large number of string and Kaluza-Klein modes, distinct from traditional inflationary models.
Findings
Observable temperature fluctuations can arise from summing contributions of about 10^{14} fields.
Tensor fluctuations remain largely unaffected by these fields.
The model predicts a specific pattern of small non-Gaussianity.
Abstract
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.
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