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      Reducing the Spectral Index in Supernatural Inflation

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          Abstract

          Supernatural inflation is an attractive model based just on a flat direction with soft SUSY breaking mass terms in the framework of supersymmetry. The beauty of the model is inferred from its name that the model needs no fine-tuning. However, the prediction of the spectral index is \(n_s \gae 1\), in contrast to experimental data. In this paper, we show that the beauty of supernatural inflation with the spectral index reduced to \(n_s=0.96\) without any fine-tuning, by considering the general feature that a flat direction is lifted by a non-renormalizable term with an A-term.

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          Author and article information

          Journal
          2009-01-21
          2009-03-30
          Article
          10.1103/PhysRevD.79.083509
          0901.3280
          3e7e4654-18f5-47ec-993a-b9e53215628b

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

          History
          Custom metadata
          6 pages, 1 figure, to be published in Physical Review D
          hep-ph astro-ph.CO astro-ph.HE

          Cosmology & Extragalactic astrophysics,High energy & Particle physics,High energy astrophysical phenomena

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