Squeezing Full-shape Dynamical Dark Energy Constraints with Galaxy Alignments

Recent 2 σ –4 σ deviations from the cosmological constant ${\rm{\Lambda }}$ suggest that dark energy (DE) may be dynamical, based on baryon acoustic oscillations and full-shape galaxy clustering (FS GC) analyses. This calls for even tighter DE constraints to narrow down its true nature. In this Lett...

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Bibliographic Details
Main Authors: Junsup Shim, Teppei Okumura, Atsushi Taruya
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
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Online Access:https://doi.org/10.3847/2041-8213/add1dd
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