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[ascl:1808.010] hi_class: Horndeski in the Cosmic Linear Anisotropy Solving System

hi_class implements Horndeski's theory of gravity in the modern Cosmic Linear Anisotropy Solving System (ascl:1106.020). It can be used to compute any cosmological observable at the level of background or linear perturbations, such as cosmological distances, cosmic microwave background, matter power and number count spectra (including relativistic effects). hi_class can be readily interfaced with Monte Python (ascl:1307.002) to test Gravity and Dark Energy models.

Code site:
http://www.thphys.uni-heidelberg.de/~zumalacarregui/hi_class.html http://www.hiclass-code.net https://github.com/miguelzuma/hi_class_public
Appears in:
https://ui.adsabs.harvard.edu/#abs/2018JCAP...08..022G https://ui.adsabs.harvard.edu/#abs/2017JCAP...08..019Z
Bibcode:
2018ascl.soft08010Z

Views: 295

ascl:1808.010
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