pith. the verified trust layer for science. sign in

arxiv: 1301.1738 · v2 · pith:G24TNH54new · submitted 2013-01-09 · ⚛️ nucl-th · astro-ph.CO· hep-ph

Varying the light quark mass: impact on the nuclear force and Big Bang nucleosynthesis

classification ⚛️ nucl-th astro-ph.COhep-ph
keywords quarkmasslightnucleardeltaforcelimitvariation
0
0 comments X p. Extension
Add this Pith Number to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{G24TNH54}

Prints a linked pith:G24TNH54 badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

The quark mass dependences of light element binding energies and nuclear scattering lengths are derived using chiral perturbation theory in combination with non-perturbative methods. In particular, we present new, improved values for the quark mass dependence of meson resonances that enter the nuclear force. A detailed analysis of the theoretical uncertainties arising in this determination is presented. As an application we derive from a comparison of observed and calculated primordial deuterium and helium abundances a stringent limit on the variation of the light quark mass, $\delta m_q/m_q = 0.02 \pm 0.04$. Inclusion of the neutron lifetime modification under the assumption of a variation of the Higgs vacuum expectation value that translates into changing quark, electron, and weak gauge boson masses, leads to a stronger limit, $|\delta m_q/m_q| < 0.009$.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Fine-tunings in radiative $\alpha$-particle capture on $^{12}$C at astrophysical energies

    nucl-th 2026-01 unverdicted novelty 4.0

    Astrophysical S-factor data constrain variations in the electromagnetic fine-structure constant to |δ α/α| ≤ 0.0002 in radiative alpha capture on carbon-12.