Testing influence of Hubble tension on the early Universe

Abstract The Hubble tension has profoundly shaped modern cosmological research. This study explores its impact on the early-universe physics in the modified emergent dark energy (MEDE) and $$\Lambda $$ Λ CDM model using Planck PR4, BK18, DESI2024/2025, and supernova samples (Pan+, Union3). First, Hu...

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Main Authors: Ming-Jian Zhang, Maoyou Yang, Junmei Wang
Format: Article
Language:English
Published: SpringerOpen 2025-07-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-025-14491-5
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author Ming-Jian Zhang
Maoyou Yang
Junmei Wang
author_facet Ming-Jian Zhang
Maoyou Yang
Junmei Wang
author_sort Ming-Jian Zhang
collection DOAJ
description Abstract The Hubble tension has profoundly shaped modern cosmological research. This study explores its impact on the early-universe physics in the modified emergent dark energy (MEDE) and $$\Lambda $$ Λ CDM model using Planck PR4, BK18, DESI2024/2025, and supernova samples (Pan+, Union3). First, Hubble constant negligibly affects the tensor-to-scalar ratio ( $$r < 0.031$$ r < 0.031 at 95%C.L.). Inclusion of DESI2025 achieves a 46% uncertainty reduction in key parameters. For CMB power spectra, DESI systematically amplifies TT/BB spectral discrepancies. Second, electron ionization fractions $$X_e(z)$$ X e ( z ) display pronounced deviations from the $$\Lambda $$ Λ CDM model at $$z=9.17$$ z = 9.17 , suggesting a connection between Hubble tension and reionization history. This finding resonates with JWST measurements on high-redshift galaxy evolution. Future observations, such as 21-cm surveys, are highly anticipated to resolve these tensions by probing early-universe evolution and dark energy interactions.
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spelling doaj-art-1a9f0f0b98b04c0fb251b917e952b5e02025-08-20T03:46:29ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522025-07-0185711010.1140/epjc/s10052-025-14491-5Testing influence of Hubble tension on the early UniverseMing-Jian Zhang0Maoyou Yang1Junmei Wang2International School for Optoelectronic Engineering, Qilu University of Technology (Shandong Academy of Sciences)International School for Optoelectronic Engineering, Qilu University of Technology (Shandong Academy of Sciences)International School for Optoelectronic Engineering, Qilu University of Technology (Shandong Academy of Sciences)Abstract The Hubble tension has profoundly shaped modern cosmological research. This study explores its impact on the early-universe physics in the modified emergent dark energy (MEDE) and $$\Lambda $$ Λ CDM model using Planck PR4, BK18, DESI2024/2025, and supernova samples (Pan+, Union3). First, Hubble constant negligibly affects the tensor-to-scalar ratio ( $$r < 0.031$$ r < 0.031 at 95%C.L.). Inclusion of DESI2025 achieves a 46% uncertainty reduction in key parameters. For CMB power spectra, DESI systematically amplifies TT/BB spectral discrepancies. Second, electron ionization fractions $$X_e(z)$$ X e ( z ) display pronounced deviations from the $$\Lambda $$ Λ CDM model at $$z=9.17$$ z = 9.17 , suggesting a connection between Hubble tension and reionization history. This finding resonates with JWST measurements on high-redshift galaxy evolution. Future observations, such as 21-cm surveys, are highly anticipated to resolve these tensions by probing early-universe evolution and dark energy interactions.https://doi.org/10.1140/epjc/s10052-025-14491-5
spellingShingle Ming-Jian Zhang
Maoyou Yang
Junmei Wang
Testing influence of Hubble tension on the early Universe
European Physical Journal C: Particles and Fields
title Testing influence of Hubble tension on the early Universe
title_full Testing influence of Hubble tension on the early Universe
title_fullStr Testing influence of Hubble tension on the early Universe
title_full_unstemmed Testing influence of Hubble tension on the early Universe
title_short Testing influence of Hubble tension on the early Universe
title_sort testing influence of hubble tension on the early universe
url https://doi.org/10.1140/epjc/s10052-025-14491-5
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