Testing gravity with CAMB and CosmoMC
arXiv:1106.4543 · doi:10.1088/1475-7516/2011/08/005
Abstract
We introduce a patch to the commonly used public codes CAMB and CosmoMC that allows the user to implement a general modification of the equations describing the growth of cosmological perturbations, while preserving the covariant conservation of the energy-momentum. This patch replaces the previously publicly released code MGCAMB, while also extending it in several ways. The new version removes the limitation of late-time-only modifications to the perturbed Einstein equations, and includes several parametrization introduced in the literature. To demonstrate the use of the patch, we obtain joint constraints on the neutrino mass and parameters of a scalar-tensor gravity model from CMB, SNe and ISW data as measured from the correlation of CMB with large scale structure.
11 pages, 3 figures, 1 table; The new MGCAMB patch is available at http://www.sfu.ca/~aha25/MGCAMB.html
References in corpus (16)
- Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
- Disappearing cosmological constant in f(R) gravity
- Conditions for the cosmological viability of f(R) dark energy models
- The Large Scale Structure of f(R) Gravity
- A Parameterized Post-Friedmann Framework for Modified Gravity
- Approaches to Understanding Cosmic Acceleration
- Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological Implications
- Distinguishing Modified Gravity from Dark Energy
- Searching for modified growth patterns with tomographic surveys
- Crossing the Phantom Divide with Parameterized Post-Friedmann Dark Energy
- On the Growth of Perturbations as a Test of Dark Energy
- A high redshift detection of the integrated Sachs-Wolfe effect
- Cosmological Constraints on f(R) Acceleration Models
- Constraints on a New Post-General Relativity Cosmological Parameter
- Parametrized Post-Friedmann Signatures of Acceleration in the CMB
- A Multi-Parameter Investigation of Gravitational Slip