DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology
We present the Einstein-Boltzmann module of the Disco-Dj (DIfferentiable Simulations for COsmology — Done with J ax) software package. This module implements a fully differentiable solver for the linearised cosmological Einstein-Boltzmann equations in the Jax framework, and allows computing Jacobian...
| Main Authors: | , , |
|---|---|
| Format: | Journal article |
| Language: | English |
| Published: |
IOP Publishing
2024
|
| _version_ | 1811139816881913856 |
|---|---|
| author | Hahn, O List, F Porqueres, N |
| author_facet | Hahn, O List, F Porqueres, N |
| author_sort | Hahn, O |
| collection | OXFORD |
| description | We present the Einstein-Boltzmann module of the Disco-Dj (DIfferentiable Simulations for COsmology — Done with J ax) 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, with a forecast for Euclid as an example. Since the implementation is significantly shorter and more modular than existing solvers, we believe it will be more straightforward to extend our solver to include additional physics, such as additional dark energy and dark matter models, modified gravity, or other non-standard physics in the future. |
| first_indexed | 2024-09-25T04:12:06Z |
| format | Journal article |
| id | oxford-uuid:5e73ce6b-07c5-4cc4-acca-537354469d26 |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-09-25T04:12:06Z |
| publishDate | 2024 |
| publisher | IOP Publishing |
| record_format | dspace |
| spelling | oxford-uuid:5e73ce6b-07c5-4cc4-acca-537354469d262024-06-26T20:10:53ZDISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmologyJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:5e73ce6b-07c5-4cc4-acca-537354469d26EnglishJisc Publications RouterIOP Publishing2024Hahn, OList, FPorqueres, NWe present the Einstein-Boltzmann module of the Disco-Dj (DIfferentiable Simulations for COsmology — Done with J ax) 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, with a forecast for Euclid as an example. Since the implementation is significantly shorter and more modular than existing solvers, we believe it will be more straightforward to extend our solver to include additional physics, such as additional dark energy and dark matter models, modified gravity, or other non-standard physics in the future. |
| spellingShingle | Hahn, O List, F Porqueres, N DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology |
| title | DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology |
| title_full | DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology |
| title_fullStr | DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology |
| title_full_unstemmed | DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology |
| title_short | DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology |
| title_sort | disco dj i a differentiable einstein boltzmann solver for cosmology |
| work_keys_str_mv | AT hahno discodjiadifferentiableeinsteinboltzmannsolverforcosmology AT listf discodjiadifferentiableeinsteinboltzmannsolverforcosmology AT porqueresn discodjiadifferentiableeinsteinboltzmannsolverforcosmology |