Computation of inflationary cosmological perturbations in chaotic inflationary scenarios using the phase-integral method

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

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21 pages, RevTex, to appear in Phys. Rev D

Scientific paper

10.1103/PhysRevD.79.103502

The phase-integral approximation devised by Fr\"oman and Fr\"oman, is used for computing cosmological perturbations in the quadratic chaotic inflationary model. The phase-integral formulas for the scalar and tensor power spectra are explicitly obtained up to fifth order of the phase-integral approximation. We show that, the phase integral gives a very good approximation for the shape of the power spectra associated with scalar and tensor perturbations as well as the spectral indices. We find that the accuracy of the phase-integral approximation compares favorably with the numerical results and those obtained using the slow-roll and uniform approximation methods.

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