We compute the running of the scalar spectral index in general multi-field slow-roll inflation. By incorporating explicit momentum dependence at the moment of horizon crossing, we can find the running straightforwardly. At the same time, we can distinguish the contributions from the quasi de Sitter background and the super-horizon evolution of the field fluctuations.
|Journal||Journal of Cosmology and Astroparticle Physics|
|State||Published - 26 May 2015|
- cosmological perturbation theory
- physics of the early universe