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| Main Authors: | , |
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| Format: | Preprint |
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2025
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| Online Access: | https://arxiv.org/abs/2503.20951 |
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| _version_ | 1866915844061134848 |
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| author | Zanoletti, C. M. A. Leonard, C. D. |
| author_facet | Zanoletti, C. M. A. Leonard, C. D. |
| contents | To mitigate the severe information loss arising from widely adopted linear scale cuts in constraints on modified gravity parameterisations with Weak Lensing (WL) and Large-Scale Structure (LSS) data, we introduce a novel alternative method for data reduction. This Principal Component Analysis (PCA)-based framework extracts key features in the matter power spectrum arising from nonlinear effects in a set of representative gravity theories. By performing the analysis in the space of principal components, we can replace sweeping `linear-only' scale cuts with targeted cuts on the transformed data vector, ultimately reducing parameter bias and significantly tightening constraints. We forecast constraints on a minimal parameterised extension to $Λ$CDM which includes modifications to the growth of structure and lensing of light ($Λ$CDM$+μ_0+Σ_0$) using mock Stage-IV data for two simulated cosmologies: the $Λ$CDM model and Extended Shift Symmetric (ESS) gravity. Under the assumption of a Universe defined by $Λ$CDM and General Relativity, our method offers constraints on $μ_0$ a factor of 1.65 tighter than traditional linear-only scale cuts. Crucially, our approach also provides the necessary constraining power to break key degeneracies in modified gravity without relying on $fσ_8$ measurements, introducing a promising new tool for the analysis of present and future WL and LSS photometric surveys. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2503_20951 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Principal Components for Model-Agnostic Modified Gravity with 3x2pt Zanoletti, C. M. A. Leonard, C. D. Cosmology and Nongalactic Astrophysics 85-08 To mitigate the severe information loss arising from widely adopted linear scale cuts in constraints on modified gravity parameterisations with Weak Lensing (WL) and Large-Scale Structure (LSS) data, we introduce a novel alternative method for data reduction. This Principal Component Analysis (PCA)-based framework extracts key features in the matter power spectrum arising from nonlinear effects in a set of representative gravity theories. By performing the analysis in the space of principal components, we can replace sweeping `linear-only' scale cuts with targeted cuts on the transformed data vector, ultimately reducing parameter bias and significantly tightening constraints. We forecast constraints on a minimal parameterised extension to $Λ$CDM which includes modifications to the growth of structure and lensing of light ($Λ$CDM$+μ_0+Σ_0$) using mock Stage-IV data for two simulated cosmologies: the $Λ$CDM model and Extended Shift Symmetric (ESS) gravity. Under the assumption of a Universe defined by $Λ$CDM and General Relativity, our method offers constraints on $μ_0$ a factor of 1.65 tighter than traditional linear-only scale cuts. Crucially, our approach also provides the necessary constraining power to break key degeneracies in modified gravity without relying on $fσ_8$ measurements, introducing a promising new tool for the analysis of present and future WL and LSS photometric surveys. |
| title | Principal Components for Model-Agnostic Modified Gravity with 3x2pt |
| topic | Cosmology and Nongalactic Astrophysics 85-08 |
| url | https://arxiv.org/abs/2503.20951 |