5σ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond ΛCDM

We find that combined Planck cosmic microwave background, baryon acoustic oscillations, and supernovae data analyzed under Λ cold dark matter (ΛCDM) are in 4.9σ tension with the extended Baryon Oscillation Spectroscopic Survey (eBOSS) Lyα forest in inference of the linear matter power spectrum at wa...

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Main Authors: Keir K. Rogers, Vivian Poulin
Format: Article
Language:English
Published: American Physical Society 2025-01-01
Series:Physical Review Research
Online Access:http://doi.org/10.1103/PhysRevResearch.7.L012018
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author Keir K. Rogers
Vivian Poulin
author_facet Keir K. Rogers
Vivian Poulin
author_sort Keir K. Rogers
collection DOAJ
description We find that combined Planck cosmic microwave background, baryon acoustic oscillations, and supernovae data analyzed under Λ cold dark matter (ΛCDM) are in 4.9σ tension with the extended Baryon Oscillation Spectroscopic Survey (eBOSS) Lyα forest in inference of the linear matter power spectrum at wave number ∼1hMpc^{−1} and redshift = 3. Model extensions can alleviate this tension: running in the tilt of the primordial power spectrum (α_{s}∼−0.01); a fraction ∼(1−5)% of ultralight axion dark matter (DM) with particle mass ∼10^{−25} eV or warm DM with mass ∼10 eV. The new Dark Energy Spectroscopic Instrument survey, coupled with high-accuracy modeling, will help distinguish the source of this discrepancy.
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spelling doaj-art-0c0c8372bfd64626a074a3f0c2b189a32025-01-22T16:08:44ZengAmerican Physical SocietyPhysical Review Research2643-15642025-01-0171L01201810.1103/PhysRevResearch.7.L0120185σ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond ΛCDMKeir K. RogersVivian PoulinWe find that combined Planck cosmic microwave background, baryon acoustic oscillations, and supernovae data analyzed under Λ cold dark matter (ΛCDM) are in 4.9σ tension with the extended Baryon Oscillation Spectroscopic Survey (eBOSS) Lyα forest in inference of the linear matter power spectrum at wave number ∼1hMpc^{−1} and redshift = 3. Model extensions can alleviate this tension: running in the tilt of the primordial power spectrum (α_{s}∼−0.01); a fraction ∼(1−5)% of ultralight axion dark matter (DM) with particle mass ∼10^{−25} eV or warm DM with mass ∼10 eV. The new Dark Energy Spectroscopic Instrument survey, coupled with high-accuracy modeling, will help distinguish the source of this discrepancy.http://doi.org/10.1103/PhysRevResearch.7.L012018
spellingShingle Keir K. Rogers
Vivian Poulin
5σ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond ΛCDM
Physical Review Research
title 5σ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond ΛCDM
title_full 5σ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond ΛCDM
title_fullStr 5σ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond ΛCDM
title_full_unstemmed 5σ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond ΛCDM
title_short 5σ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond ΛCDM
title_sort 5σ tension between planck cosmic microwave background and eboss lyman alpha forest and constraints on physics beyond λcdm
url http://doi.org/10.1103/PhysRevResearch.7.L012018
work_keys_str_mv AT keirkrogers 5stensionbetweenplanckcosmicmicrowavebackgroundandebosslymanalphaforestandconstraintsonphysicsbeyondlcdm
AT vivianpoulin 5stensionbetweenplanckcosmicmicrowavebackgroundandebosslymanalphaforestandconstraintsonphysicsbeyondlcdm