# Determination of the NNLO low-energy constant $C_{93}$

**Authors:** Maarten Golterman, Kim Maltman, Santiago Peris

arXiv: 1706.03672 · 2017-10-04

## TL;DR

This paper determines the NNLO low-energy constant $C_{93}$ in chiral perturbation theory using hadronic tau decay data, addressing systematic uncertainties and implications for muon g-2 calculations.

## Contribution

It provides a precise value for $C_{93}$ from tau decay data and assesses the impact of higher-order effects on this determination.

## Key findings

- Estimated $C_{93}$ value from $I=1$ vector channel data.
- Assessed the effect of SU(3) flavor-breaking on $C_{93}$.
- Discussed implications for muon anomalous magnetic moment.

## Abstract

Experimental data from hadronic $\tau$ decays allow for a precision determination of the slope of the $I=1$ vacuum polarization at zero momentum. We use this information to provide a value for the next-to-next-to-leading order (NNLO) low-energy constant $C_{93}$ in chiral perturbation theory. The largest systematic error in this determination results from the neglect of terms beyond NNLO in the effective chiral Lagrangian, whose presence in the data will, in general, make the effective $C_{93}$ determined in an NNLO analysis mass dependent. We estimate the size of this effect by using strange hadronic $\tau$-decay data to perform an alternate $C_{93}$ determination based on the slope of the strange vector polarization at zero momentum, which differs from that of the $I=1$ vector channel only through $SU(3)$ flavor-breaking effects. We also comment on the impact of such higher order effects on ChPT-based estimates for the hadronic vacuum polarization contribution to the muon anomalous magnetic moment.

## Full text

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## Figures

6 figures with captions in the complete paper: https://tomesphere.com/paper/1706.03672/full.md

## References

40 references — full list in the complete paper: https://tomesphere.com/paper/1706.03672/full.md

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Source: https://tomesphere.com/paper/1706.03672