The light-quark mass dependence of the nucleon axial charge

Authors

  • Fernando Alvarado IFIC
  • L. Alvarez-Ruso IFIC

DOI:

https://doi.org/10.31349/SuplRevMexFis.3.0308095

Abstract

The light-quark mass dependence of the nucleon axial isovector charge (gA) has been analysed up to NNLO, O(p4), in relativistic chiral perturbation theory using extended-on-mass-shell renormalization, without and with explicit Delta(1232) degrees of freedom. In the Delta-less case at this order, the gA(Mpi)  dependence of lattice QCD simulations cannot be reproduced using low energy constants extracted from pion-nucleon phenomenology. A good description of these LQCD data is only accomplished in the theory with Delta. From this fit we obtain gA(Mpiphys)=1.260(12) close to the experimental results and d16= -0.88(88) GeV-2 in agreement with pi N-> pi pi N. The sizeable errors are of theoretical origin, reflecting the difference between O(p3) and O(p4) at large Mpi.

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Published

2022-06-13

How to Cite

1.
Alvarado F, Alvarez-Ruso L. The light-quark mass dependence of the nucleon axial charge. Supl. Rev. Mex. Fis. [Internet]. 2022 Jun. 13 [cited 2022 Dec. 7];3(3):0308095 1-5. Available from: https://rmf.smf.mx/ojs/index.php/rmf-s/article/view/6234