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[ascl:1311.009] CosmoTherm: Thermalization code

CosmoTherm allows precise computation of CMB spectral distortions caused by energy release in the early Universe. Different energy-release scenarios (e.g., decaying or annihilating particles) are implemented using the Green's function of the cosmological thermalization problem, allowing fast computation of the distortion signal. The full thermalization problem can be solved on a case-by-case basis for a wide range of energy-release scenarios using the full PDE solver of CosmoTherm. A simple Monte-Carlo toolkit is included for parameter estimation and forecasts using the Green's function method.

Code site:
http://www.jb.man.ac.uk/~jchluba/Science/CosmoTherm/Welcome.html
Described in:
http://adsabs.harvard.edu/abs/2012MNRAS.419.1294C
Bibcode:
2013ascl.soft11009C

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ascl:1311.009
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