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[ascl:1110.020] CROSS_CMBFAST: ISW-correlation Code

This code is an extension of CMBFAST4.5.1 to compute the ISW-correlation power spectrum and the 2-point angular ISW-correlation function for a given galaxy window function. It includes dark energy models specified by a constant equation of state (w) or a linear parameterization in the scale factor (w0,wa) and a constant sound speed (c2de). The ISW computation is limited to flat geometry. Differently from the original CMBFAST4.5 version dark energy perturbations are implemented for a general dark energy fluid specified by w(z) and c2de in synchronous gauge. For time varying dark energy models it is suggested not to cross the w=-1 line, as Dr. Wenkman says: "never cross the streams", bad things can happen.

Code site:
https://luth.obspm.fr/~luthier/corasaniti/?page_id=228
Appears in:
http://adsabs.harvard.edu/abs/2005PhRvD..71l3521C http://adsabs.harvard.edu/abs/2008AmJPh..76..197L
Bibcode:
2011ascl.soft10020C

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ascl:1110.020
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