• Inflation in the light of BICEP2 and PLANCK

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    • Keywords


      Inflation; supergravity; Gibbons–Hawking; BICEP2; PLANCK.

    • Abstract


      The BICEP2/Keck+PLANCK joint analysis of the 𝐵-model polarization and polarization by foreground dust sets an upper bound on the tensor-to-scalar ratio of 𝑟0.05 < 0.12 at 95% CL. The popular Starorbinsky model Higgs-inflation or the conformally equivalent Higgs-inflation model allow low 𝑟 values (∼10−3). We survey the generalizations of the Starobinsky–Higgs models which would allow larger values (𝑟 ∼ 0.1). The Starobinsky–Higgs inflation models require an exponential potential which can be naturally derived from SUGRA models. We show that a variation of the no-scale SUGRA model can give rise to the generalized Starobinsky models which give large 𝑟. We also examine non-standard boundary conditions which would allow a large deviation of the tensor spectral index from the slow roll values and propose that the presence of a thermal component in the tensor spectrum arises from Gibbons–Hawking temperature of the de-Sitter space.

    • Author Affiliations


      Subhendra Mohanty1

      1. Physical Research Laboratory, Ahmedabad 380 009, India
    • Dates

  • Pramana – Journal of Physics | News

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      Posted on July 25, 2019

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