Improved Constraints on the Variation of the Weak Scale from Big Bang Nucleosynthesis

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Autori principali: Meyer, Helen, Meißner, Ulf-G.
Natura: Preprint
Pubblicazione: 2024
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author Meyer, Helen
Meißner, Ulf-G.
author_facet Meyer, Helen
Meißner, Ulf-G.
contents We present an improved calculation of the light element abundances in the framework of Big Bang nucleosynthesis as a function of the Higgs vacuum expectation value $v$. We compare the methods of our calculation to previous literature including the recently published work of Burns et al. [1]. The PDG result for the $^4$He abundance can be explained within $2σ$ by $-0.014 \leq δv / v \leq 0.026$, for deuterium we find the constraint $-0.005 \leq δv / v \leq -0.001$. These bounds are more stringent than what was found earlier.
format Preprint
id arxiv_https___arxiv_org_abs_2403_09325
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Improved Constraints on the Variation of the Weak Scale from Big Bang Nucleosynthesis
Meyer, Helen
Meißner, Ulf-G.
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Lattice
High Energy Physics - Theory
Nuclear Theory
We present an improved calculation of the light element abundances in the framework of Big Bang nucleosynthesis as a function of the Higgs vacuum expectation value $v$. We compare the methods of our calculation to previous literature including the recently published work of Burns et al. [1]. The PDG result for the $^4$He abundance can be explained within $2σ$ by $-0.014 \leq δv / v \leq 0.026$, for deuterium we find the constraint $-0.005 \leq δv / v \leq -0.001$. These bounds are more stringent than what was found earlier.
title Improved Constraints on the Variation of the Weak Scale from Big Bang Nucleosynthesis
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Lattice
High Energy Physics - Theory
Nuclear Theory
url https://arxiv.org/abs/2403.09325