# A Measurement of the Branching Ratio of $\pi^0$ Dalitz Decay using $K_L   \rightarrow \pi^0\pi^0\pi^0$ Decays

**Authors:** E. Abouzaid, M. Arenton, A.R. Barker, L. Bellantoni, E. Blucher, G.J., Bock, E. Cheu, R. Coleman, M.D. Corcoran, B. Cox, A.R. Erwin, C.O. Escobar,, A. Glazov, A. Golossanov, R.A. Gomes, P. Gouffon, Y.B. Hsiung, D.A. Jensen,, R. Kessler, K. Kotera, A. Ledovskoy, P.L. McBride, E. Monnier, H. Nguyen, R., Niclasen, D.G. Phillips II, E.J. Ramberg, R.E. Ray, M. Ronquest, E. Santos,, W. Slater, D. Smith, N. Solomey, E.C. Swallow, P.A. Toale, R. Tschirhart,, Y.W. Wah, J. Wang, H.B. White, J. Whitmore, M. J. Wilking, B. Winstein, R., Winston, E.T. Worcester, T. Yamanaka, E. D. Zimmerman, R.F. Zukanovich

arXiv: 1902.01375 · 2019-11-27

## TL;DR

This paper reports a precise measurement of the Dalitz decay branching ratio of the neutral pion, using data from the KTeV experiment, improving the accuracy over previous results.

## Contribution

The study provides the most precise measurement to date of the $\pi^0$ Dalitz decay branching ratio, utilizing a large dataset and normalization to $K_L$ decays, with corrections based on theoretical mass spectrum predictions.

## Key findings

- Measured branching ratio with a threefold reduction in uncertainty.
- Results consistent with previous measurements.
- Provides a corrected full mass range branching ratio.

## Abstract

We present a measurement of $B(\pi^0 \rightarrow e^+e^- \gamma)/B(\pi^0 \rightarrow \gamma\gamma)$, the Dalitz branching ratio, using data taken in 1999 by the E832 KTeV experiment at Fermi National Accelerator Laboratory. We use neutral pions from fully reconstructed $K_L$ decays in flight; the measurement is based on about 60 thousand $K_L \rightarrow \pi^0\pi^0\pi^0 \rightarrow \gamma\gamma~\gamma\gamma~e^+e^-\gamma$ decays. We normalize to $K_L \rightarrow \pi^0\pi^0\pi^0 \rightarrow 6\gamma$ decays. We find $B(\pi^0 \rightarrow e^+e^- \gamma)/B(\pi^0 \rightarrow \gamma\gamma)$ $(m_{e^+e^-}$ > 15 MeV/$c^2)$ = $[3.920 \pm 0.016(stat) \pm 0.036 (syst)] \times 10^{-3}$. Using the Mikaelian and Smith prediction for the $e^+e^-$ mass spectrum, we correct the result to the full $e^+e^-$ mass range. The corrected result is $B(\pi^0 \rightarrow e^+e^- \gamma)/B(\pi^0 \rightarrow \gamma\gamma) = [1.1559 \pm 0.0047(stat) \pm 0.0106 (syst)]$%. This result is consistent with previous measurements and the uncertainty is a factor of three smaller than any previous measurement.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1902.01375/full.md

## Figures

7 figures with captions in the complete paper: https://tomesphere.com/paper/1902.01375/full.md

## References

19 references — full list in the complete paper: https://tomesphere.com/paper/1902.01375/full.md

---
Source: https://tomesphere.com/paper/1902.01375