# Measuring the cross section of the $^{15}$N($\alpha$,$\gamma$)$^{19}$F   reaction using a single-fluid bubble chamber

**Authors:** D. Neto, K. Bailey, J. F. Benesch, B. Cade, B. DiGiovine, A., Freyberger, J. M. Grames, A. Hofler, R. J. Holt, R. Kazimi, D. Meekins, M., McCaughan, D. Moser, T. O'Connor, M. Poelker, K. E. Rehm, S. Riordan, R., Suleiman, R. Talwar, C. Ugalde

arXiv: 2302.12760 · 2023-03-07

## TL;DR

This paper introduces a novel method using a single-fluid bubble chamber to measure the cross section of a key stellar nucleosynthesis reaction, leveraging reciprocity and increased luminosity for more sensitive detection.

## Contribution

The study demonstrates a new experimental approach with a bubble chamber to measure nuclear reaction cross sections via photodissociation, achieving sensitivity down to hundreds of picobarns.

## Key findings

- Successfully measured the $^{15}$N($	ext{α}$,$	ext{γ}$)$^{19}$F cross section.
- Validated the reciprocity theorem for nuclear reaction measurements.
- Potential to reach single picobarn sensitivity with improvements.

## Abstract

$^{15}$N($\alpha$,$\gamma$)$^{19}$F is believed to be the primary means of stellar nucleosynthesis of fluorine. Here we present the use of a single-fluid bubble chamber to measure the cross section of the time-inverse photo-dissociation reaction. The method benefits from a luminosity increase of several orders of magnitude due to the use of a thicker liquid target -- when compared to thin films or gas targets -- and from the reciprocity theorem. We discuss the results of an experiment at the Thomas Jefferson National Accelerator Facility, where the cross section of the photodisintegration process $^{19}$F($\gamma$, $\alpha$)$^{15}$N was measured by bombarding a superheated fluid of C$_3$F$_8$ with bremsstrahlung $\gamma$-rays produced by impinging a 4 - 5.5 MeV electron beam on a Cu radiator. From the photodissociation yield the cross section was extracted by performing a convolution with a Monte Carlo-generated $\gamma$-ray beam spectrum. The measurement produced a cross section that was then time inverted using the reciprocity theorem. The cross section for the $^{15}$N($\alpha$,$\gamma$)$^{19}$F reaction was determined down to a value in the range of hundreds of picobarns. With further improvements of the experimental setup the technique could potentially push cross section measurements down to the single picobarn range.

## Full text

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## Figures

16 figures with captions in the complete paper: https://tomesphere.com/paper/2302.12760/full.md

## References

55 references — full list in the complete paper: https://tomesphere.com/paper/2302.12760/full.md

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Source: https://tomesphere.com/paper/2302.12760