Preference for evolving dark energy in light of the galaxy bispectrum
Zhiyu Lu, Th’eo Simon, Pierre Zhang
arXiv:2503.04602v2 Announce Type: replace
Abstract: We analyse pre-DESI clustering data using a dark energy equation of state $w(z)$ parametrised by $(w_0, w_a)$, finding a $2.8-3.9sigma$ preference for evolving dark energy over the cosmological constant $Lambda$ when combined with cosmic microwave background data from Planck and supernova data from Pantheon+, Union3, or DESY5. Our constraints, consistent with DESI Y1 results, are derived from the power spectrum and bispectrum of SDSS/BOSS galaxies using the Effective Field Theory of Large Scale Structure (EFTofLSS) at one loop. The evidence remains robust across analysis variations but disappears without the one-loop bispectrum. When combining DESI baryon acoustic oscillations with BOSS full-shape data, while marginalising over the sound horizon in the latter to prevent unaccounted correlations, the significance increases to $3.7-4.4sigma$, depending on the supernova dataset. Using a data-driven reconstruction of $w(z)$, we show that the evidence arises from deviations from $Lambda$ at multiple redshifts. In addition, our findings are interpreted within the Effective Field Theory of Dark Energy (EFTofDE), from which we explicitly track the non-standard time evolution in EFTofLSS predictions. For perturbatively stable theories in the $w arXiv:2503.04602v2 Announce Type: replace
Abstract: We analyse pre-DESI clustering data using a dark energy equation of state $w(z)$ parametrised by $(w_0, w_a)$, finding a $2.8-3.9sigma$ preference for evolving dark energy over the cosmological constant $Lambda$ when combined with cosmic microwave background data from Planck and supernova data from Pantheon+, Union3, or DESY5. Our constraints, consistent with DESI Y1 results, are derived from the power spectrum and bispectrum of SDSS/BOSS galaxies using the Effective Field Theory of Large Scale Structure (EFTofLSS) at one loop. The evidence remains robust across analysis variations but disappears without the one-loop bispectrum. When combining DESI baryon acoustic oscillations with BOSS full-shape data, while marginalising over the sound horizon in the latter to prevent unaccounted correlations, the significance increases to $3.7-4.4sigma$, depending on the supernova dataset. Using a data-driven reconstruction of $w(z)$, we show that the evidence arises from deviations from $Lambda$ at multiple redshifts. In addition, our findings are interpreted within the Effective Field Theory of Dark Energy (EFTofDE), from which we explicitly track the non-standard time evolution in EFTofLSS predictions. For perturbatively stable theories in the $w