2011

Signatures of Supersymmetry from the Early Universe

Baumann, Daniel, Green, Daniel

Understand

Supersymmetry plays a fundamental role in the radiative stability of many inflationary models.

  • Spontaneous breaking of the symmetry inevitably leads to fields with masses of order the Hubble scale during inflation.
  • When these fields couple to the inflaton they produce a unique signature in the squeezed limit of the three-point function of primordial curvature perturbations.
  • In this paper, we make this connection between naturalness, supersymmetry, Hubble-mass degrees of freedom and the squeezed limit precise.

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