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[ascl:1504.010] CosmoTransitions: Cosmological Phase Transitions

CosmoTransitions analyzes early-Universe finite-temperature phase transitions with multiple scalar fields. The code enables analysis of the phase structure of an input theory, determines the amount of supercooling at each phase transition, and finds the bubble-wall profiles of the nucleated bubbles that drive the transitions.

Code site:
https://github.com/clwainwright/CosmoTransitions http://cpc.cs.qub.ac.uk/summaries/AEML_v1_0.html
Described in:
http://adsabs.harvard.edu/abs/2012CoPhC.183.2006W
Bibcode:
2015ascl.soft04010W

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ascl:1504.010
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