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Paper   IPM / Astronomy / 14587
School of Astronomy
  Title:   Schrödinger field theory in curved spacetime: In-In formalism and three-point function for inflationary background
1.  Abasalt. Rostami
2.  Javad. T. Firouzjaee
  Status:   Published
  Journal: JHEP
  Year:  2016
  Supported by:            ipm IPM
We review the Schr¨odinger picture of field theory in curved spacetime and using this formalism, the power spectrum of massive non-interacting, minimally coupled scalars in a fixed de Sitter background is obtained. To calculate the N-point function in Schr¨odinger field theory, the in-in formalism is extended in the Friedmann-Lema�?ıtre-Robertson-Walker (FLRW) universe. We compute the three-point function for primordial scalar field fluctuation in the single field inflation by this in-in formalism. The results are the same as the three-point function in the Heisenberg picture.

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