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Hence, the dynamical prop- erties are encoded in the properties of the corresponding eigenvalues. For hyperbolic critical points having eigenval- ues with a negative real part we can approximate the evolution of the dynamical system, linearizing the solution using the Hartman–Grobman theorem [75]...
To explore the viability of an inflationary model, prop- erties of the initial cosmological perturbations play a vital role. Such properties will mainly be described with statisti- cal parameters like the two point correlation function known as the power spectrum, scalar and tensor spectral index,...