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Nucleosynthesis and the Time Dependence of Fundamental Couplings
High Energy Physics - Phenomenology · Submitted 11 Nov 1994
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Because the scale parameters of couplings set by dimensional transmutation depend exponentially on the dilaton vev, we may obtain stringent limits on the shift of the dilaton from the requirement that the induced shift in the couplings not vitiate the successful calculations of element abundances for big-bang nucleosynthesis.
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The abstract, sentence by sentence
We consider the effects of the time dependence of couplings due to their dependence on a dilaton field, as occurs in superstring theory, as well as in gravity theories of the Jordan-Brans-Dicke type. Because the scale parameters of couplings set by dimensional transmutation depend exponentially on the dilaton vev, we may obtain stringent limits on the shift of the dilaton from the requirement that the induced shift in the couplings not vitiate the successful calculations of element abundances for big-bang nucleosynthesis. These limits can be substantially stronger than those obtained directly from the dilaton-induced change in the gravitational coupling.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We consider the effects of the time dependence of couplings due to their dependence on a dilaton field, as occurs in superstring theory, as well as in gravity theories of the Jordan-Brans-Dicke type. | background 0.64 | 0.43 | 0.04 | asserted 0.73 |
| s1 | Because the scale parameters of couplings set by dimensional transmutation depend exponentially on the dilaton vev, we may obtain stringent limits on the shift of the dilaton from the requirement that the induced shift in the couplings not vitiate the successful calculations of element abundances for big-bang nucleosynthesis. | method 0.38 | 0.41 | 0.48 | hedged possibility 1.00 |
| s2 | These limits can be substantially stronger than those obtained directly from the dilaton-induced change in the gravitational coupling. | result 0.76 | 0.65 | 0.42 | asserted 0.68 |
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The paper
Original abstract
We consider the effects of the time dependence of couplings due to their dependence on a dilaton field, as occurs in superstring theory, as well as in gravity theories of the Jordan-Brans-Dicke type. Because the scale parameters of couplings set by dimensional transmutation depend exponentially on the dilaton vev, we may obtain stringent limits on the shift of the dilaton from the requirement that the induced shift in the couplings not vitiate the successful calculations of element abundances for big-bang nucleosynthesis. These limits can be substantially stronger than those obtained directly from the dilaton-induced change in the gravitational coupling.
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References
How the literature uses it
20 arXiv papers cite this in 31 sentences
Papers citing it · 25 sentences without a confident label
Uses its method or tool 1 paper
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This generally follows what is adopted in Refs. [ref] .
Constraining the time variation of the coupling constants from cosmic microwave background: effect of \Lambda_{QCD} · The Dilaton Dependence of $α$, $m_e$ and $m_p$ · 0.80
Cites it as support 1 paper
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This assumption is motivated by the fact that the $Q$-dependences of them are severely constrained by the tests of the equivalence principle, by the test of the time-variation of the fundamental couplings, and by the BBN constraints [ref] .
The swampland conjecture and the Higgs expectation value · Wilsonian approach · 0.99
Cites it as background 4 papers
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In particular, it has been extensively used to constrain the variations of fundamental constants [ref] and modified theories of gravity [ref] ; a summary of many of these studies can be found in [ref] .
BBN constraints on universally-coupled ultralight scalar dark matter · Introduction · 0.83
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There have been a number of articles considering the sensitivity of BBN to variations in the fundamental parameters of the Standard Model, including the electromagnetic fine structure constant [ref] , the quark masses [ref] , and recently, a more general consideration of the naturalness of the weak scale in a multiverse context [ref] .
Quantifying the sensitivity of Big Bang Nucleosynthesis to isospin breaking with input from lattice QCD · BBN and isospin · 1.00
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Depending on the Lagrangian implementation and its motivation, one or several constants can vary in coupled ways, typically one would expect a coupled variation of all constants within a theoretical framework motivated by GUTs or string theories [ref] .
The mass effect -- Variations of the electron mass and their impact on cosmology · Physical models: scalar fields and electron mass variation · 0.91
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