Inflation: Monte-Carlo Code for Slow-Roll Inflation

Details Inflation: Monte-Carlo Code for Slow-Roll Inflation Inflation: Monte-Carlo Code for Slow-Roll Inflation

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ascl.soft01017f&link_type=abstract

Astrophysics Source Code Library, record ascl:1201.017

Astronomy and Astrophysics

Astrophysics

Scientific paper

Inflation is a numerical code to generate power spectra and other observables through numerical solutions to flow equations. The code generates tensor and scalar power spectra as a function of wavenumber and various other parameters at specific wavenumbers of interest (such as for CMB, scalar perturbations at smaller scales, gravitational wave detection at direct detection frequencies). The output can be easily ported to publicly available Markov Chain codes to constrain cosmological parameters with data.

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