Radiative pion photoproduction in covariant chiral perturbation theory

J. Rijneveen, N. Rijneveen, H. Krebs, A. M. Gasparyan, and E. Epelbaum
Phys. Rev. C 103, 045203 – Published 13 April 2021

Abstract

We present a calculation of radiative pion photoproduction in the framework of covariant chiral perturbation theory with explicit Δ(1232) degrees of freedom. The analysis is performed employing the small-scale expansion scheme adjusted for the Δ region. Depending on the channel, we include contributions up to next-to-next-to-leading order. We fit the available experimental data for the reaction γpγpπ0 and extract the value of the Δ+ magnetic moment. Errors from the truncation of the small-scale expansion are estimated using the Bayesian approach. We compare our results both with the previous studies within the δ-expansion scheme and with the Δ-less theory. We also give predictions for radiative charged-pion photoproduction.

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  • Received 22 September 2020
  • Accepted 16 March 2021

DOI:https://doi.org/10.1103/PhysRevC.103.045203

©2021 American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsNuclear Physics

Authors & Affiliations

J. Rijneveen1,*, N. Rijneveen1,†, H. Krebs1,‡, A. M. Gasparyan1,2,§, and E. Epelbaum1,∥

  • 1Ruhr-Universität Bochum, Fakultät für Physik und Astronomie, Institut für Theoretische Physik II, D-44780 Bochum, Germany
  • 2NRC Kurchatov Institute - ITEP, B. Cheremushkinskaya 25, 117218 Moscow, Russia

  • *jan.rijneveen@rub.de
  • nora.rijneveen@rub.de
  • hermann.krebs@rub.de
  • §ashot.gasparyan@rub.de
  • evgeny.epelbaum@rub.de

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Vol. 103, Iss. 4 — April 2021

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