CMBEASY:: an Object Oriented Code for the Cosmic Microwave Background
arXiv:astro-ph/0302138 · doi:10.1088/1475-7516/2005/10/011
Abstract
We have ported the cmbfast package to the C++ programming language to produce cmbeasy, an object oriented code for the cosmic microwave background. The code is available at www.cmbeasy.org. We sketch the design of the new code, emphasizing the benefits of object orientation in cosmology, which allow for simple substitution of different cosmological models and gauges. Both gauge invariant perturbations and quintessence support has been added to the code. For ease of use, as well as for instruction, a graphical user interface is available.
7 pages, 5 figures, matches published version, code at http://www.cmbeasy.org
References in corpus (2)
Cited by in corpus (41)
- The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
- Testing General Relativity in Cosmology
- CMB power spectrum contribution from cosmic strings using field-evolution simulations of the Abelian Higgs model
- Screening Modifications of Gravity through Disformally Coupled Fields
- Information field theory for cosmological perturbation reconstruction and non-linear signal analysis
- Testing the interaction between dark energy and dark matter via latest observations
- Cuscuton Cosmology: Dark Energy meets Modified Gravity
- Measuring the Speed of Dark: Detecting Dark Energy Perturbations
- The imprint of the interaction between dark sectors in large scale cosmic microwave background anisotropies
- CMB power spectra from cosmic strings: predictions for the Planck satellite and beyond
- Vector field models of modified gravity and the dark sector
- CMB polarization power spectra contributions from a network of cosmic strings
- Eddington-Born-Infeld gravity and the large scale structure of the Universe
- CMB Lensing Constraints on Neutrinos and Dark Energy
- Constraining Lorentz violation with cosmology
- A comparison of Einstein-Boltzmann solvers for testing General Relativity
- Non-isotropy in the CMB power spectrum in single field inflation
- Small scale aspects of warm dark matter : power spectra and acoustic oscillations
- Constraints from CMB on Spacetime Noncommutativity and Causality Violation
- Testing Cosmology with Cosmic Sound Waves
- Non-linear Matter Spectra in Coupled Quintessence
- Energy-momentum correlations for Abelian Higgs cosmic strings
- Constraining topological defects with temperature and polarization anisotropies
- CMB anisotropies in the presence of a stochastic magnetic field
- Effects of helical magnetic fields on the cosmic microwave background
- Growth index and statefinder diagnostic of Oscillating Dark Energy
- On the degeneracy between primordial tensor modes and cosmic strings in future CMB data from Planck
- Bayesian Limits on Primordial Isotropy Breaking
- Testing dark energy model with the large scale structure
- The signature of the scattering between dark sectors in large scale cosmic microwave background anisotropies
- Phenomenology of Gravitational Aether as a solution to the Old Cosmological Constant Problem
- Cosmic Microwave Background temperature and polarization anisotropies from the large-N limit of global defects
- CMB and matter power spectra from cross correlations of primordial curvature and magnetic fields
- Multiple Cosmic Collisions and the Microwave Background Power Spectrum
- Does Planck mass run on the cosmological horizon scale?
- CMB anisotropies from acausal scaling seeds
- The CMB in a Causal Set Universe
- Synchronous coordinates and gauge-invariant observables in cosmological spacetimes
- Scalar field descriptions of two dark energy models
- CMB anisotropies and linear matter power spectrum in models with non-thermal neutrinos and primordial magnetic fields
- Fast and precise way to calculate the posterior for the local non-Gaussianity parameter from cosmic microwave background observations