We'd like to announce the release of our code for computing Bianchi type VIIh induced temperature fluctuations. The code is based on the solutions to the Bianchi model determined by Barrow et al. (1985). These solutions do not incorporate any dark energy, nonetheless the solutions provide a phenomenological setting within which to test the effect of Bianchi models. For more details on the equations implemented see the Appendix of our recent publication (astro-ph/0510349).
The code may be obtained from: http://www.mrao.cam.ac.uk/~jdm57/
I hope this forum can be used to provide support for the software library, but also feel free to e-mail me directly if you notice any bugs or have any other comments.
Bianchi VIIh simulations
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