4.6 Article

The matter bounce curvaton scenario

出版社

IOP Publishing Ltd
DOI: 10.1088/1475-7516/2011/03/003

关键词

alternatives to inflation; cosmological perturbation theory; cosmic singularity; physics of the early universe

资金

  1. Department of Physics at Arizona State University
  2. NSERC at McGill University
  3. Canada Research Chairs program
  4. National Natural Science Foundation of China [10975142, 10821063, 11033005]
  5. 973 program [1J2007CB81540002]
  6. Chinese Academy of Sciences [KJCX3-SYW-N2]

向作者/读者索取更多资源

Massless scalar fields originating in a quantum vacuum state acquire a scale-invariant spectrum of fluctuations in a matter-dominated contracting universe. We show that these isocurvature fluctuations transfer to a scale-invariant spectrum of curvature fluctuations during a non-singular bounce phase. This provides a mechanism for enhancing the primordial adiabatic fluctuations and suppressing the ratio of tensor to scalar perturbations. Moreover, this mechanism leads to new sources of non-Gaussianity of curvature perturbations.

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