1. A comparison of Einstein-Boltzmann solvers for testing General Relativity
- Author
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Bellini, E., Barreira, A., Frusciante, N., Hu, B., Peirone, S., Raveri, M., Zumalacárregui, M., Avilez-Lopez, A., Ballardini, M., Battye, R. A., Bolliet, B., Calabrese, E., Dirian, Y., Ferreira, P. G., Finelli, F., Huang, Z., Ivanov, M. M., Lesgourgues, J., Li, B., Lima, N. A., Pace, F., Paoletti, D., Sawicki, I., Silvestri, A., Skordis, C., Umiltà, C., and Vernizzi, F.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We compare Einstein-Boltzmann solvers that include modifications to General Relativity and find that, for a wide range of models and parameters, they agree to a high level of precision. We look at three general purpose codes that primarily model general scalar-tensor theories, three codes that model Jordan-Brans-Dicke (JBD) gravity, a code that models f(R) gravity, a code that models covariant Galileons, a code that models Ho\v{r}ava-Lifschitz gravity and two codes that model non-local models of gravity. Comparing predictions of the angular power spectrum of the cosmic microwave background and the power spectrum of dark matter for a suite of different models, we find agreement at the sub-percent level. This means that this suite of Einstein-Boltzmann solvers is now sufficiently accurate for precision constraints on cosmological and gravitational parameters., Comment: 23 pages; 11 figures. Matches version accepted in PRD
- Published
- 2017
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