%0 Generic %1 hahn2023discodj %A Hahn, Oliver %A List, Florian %A Porqueres, Natalia %D 2023 %K tifr %T DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology %U http://arxiv.org/abs/2311.03291 %X We present the Einstein-Boltzmann module of the DISCO-DJ (DIfferentiable Simulations for COsmology - Done with JAX) software package. This module implements a fully differentiable solver for the linearised cosmological Einstein-Boltzmann equations in the JAX framework, and allows computing Jacobian matrices of all solver output with respect to all input parameters using automatic differentiation. This implies that along with the solution for a given set of parameters, the tangent hyperplane in parameter space is known as well, which is a key ingredient for cosmological inference and forecasting problems as well as for many other applications. We discuss our implementation and demonstrate that our solver agrees at the per-mille level with the existing non-differentiable solvers CAMB and CLASS, including massive neutrinos and a dark energy fluid with parameterised equation of state. We illustrate the dependence of various summary statistics in large-scale structure cosmology on model parameters using the differentiable solver, and finally demonstrate how it can be easily used for Fisher forecasting. Since the implementation is significantly shorter and more modular than existing solvers, it is easy to extend our solver to include additional physics, such as additional dark energy models, modified gravity, or other non-standard physics.

@misc{hahn2023discodj, abstract = {We present the Einstein-Boltzmann module of the DISCO-DJ (DIfferentiable Simulations for COsmology - Done with JAX) software package. This module implements a fully differentiable solver for the linearised cosmological Einstein-Boltzmann equations in the JAX framework, and allows computing Jacobian matrices of all solver output with respect to all input parameters using automatic differentiation. This implies that along with the solution for a given set of parameters, the tangent hyperplane in parameter space is known as well, which is a key ingredient for cosmological inference and forecasting problems as well as for many other applications. We discuss our implementation and demonstrate that our solver agrees at the per-mille level with the existing non-differentiable solvers CAMB and CLASS, including massive neutrinos and a dark energy fluid with parameterised equation of state. We illustrate the dependence of various summary statistics in large-scale structure cosmology on model parameters using the differentiable solver, and finally demonstrate how it can be easily used for Fisher forecasting. Since the implementation is significantly shorter and more modular than existing solvers, it is easy to extend our solver to include additional physics, such as additional dark energy models, modified gravity, or other non-standard physics.}, added-at = {2023-11-07T06:37:48.000+0100}, author = {Hahn, Oliver and List, Florian and Porqueres, Natalia}, biburl = {https://www.bibsonomy.org/bibtex/2d4465e9e447d898dc9cc7b94b1e4c6cf/citekhatri}, description = {[2311.03291] DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology}, interhash = {3c15a50e3971186f82895f409b77350f}, intrahash = {d4465e9e447d898dc9cc7b94b1e4c6cf}, keywords = {tifr}, note = {cite arxiv:2311.03291Comment: 29 pages, 8 figures, to be submitted to JCAP, comments very welcome}, timestamp = {2023-11-07T06:37:48.000+0100}, title = {DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology}, url = {http://arxiv.org/abs/2311.03291}, year = 2023 }