The Deuterium-Lithium tension in Big Bang Nucleosynthesis

There are many tensions in the era of precision cosmology. The most prominent, at present, is the Hubble tension – the difference between traditional measurements, which consistently obtain H0 = 73 km/s/Mpc, and best fit* to the acoustic power spectrum of the cosmic microwave background (CMB) observed by Planck, H0 = 67 km/s/Mpc.

Publication Details

Journal
Front Matter
Published
2025-05-17
DOI
https://doi.org/10.59350/7pk4t-s3303
Primary Topic
Historical and Cultural Archaeology Studies
Type
article
Field-Weighted Citation Impact
0.00
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article

The Deuterium-Lithium tension in Big Bang Nucleosynthesis

Front Matter
Historical and Cultural Archaeology Studies
article

The Deuterium-Lithium tension in Big Bang Nucleosynthesis

article en

Abstract

There are many tensions in the era of precision cosmology. The most prominent, at present, is the Hubble tension – the difference between traditional measurements, which consistently obtain H0 = 73 km/s/Mpc, and best fit* to the acoustic power spectrum of the cosmic microwave background (CMB) observed by Planck, H0 = 67 km/s/Mpc.

Front Matter
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The Deuterium-Lithium tension in Big Bang Nucleosynthesis · Front Matter (2025) | TGRS Research Map | TGRS