Eur. Phys. J. A (2021) 57: 81
https://doi.org/10.1140/epja/s10050-021-00382-2

Regular Article – Theoretical Physics

Designing optimal experiments: an application to proton Compton scattering

¹ Department of Physics, The Ohio State University, 43210, Columbus, OH, USA
² Department of Physics, Institute for Nuclear Studies, The George Washington University, 20052, Washington, DC, USA
³ Department of Physics, Duke University, Box 90305, 27708, Durham, NC, USA
⁴ High Intensity Gamma-Ray Source, Triangle Universities Nuclear Laboratories, Box 90308, 27708, Durham, NC, USA
⁵ School of Physics and Astronomy, The University of Manchester, M13 9PL, Manchester, UK
⁶ Department of Physics and Astronomy and Institute of Nuclear and Particle Physics, Ohio University, 45701, Athens, OH, USA
⁷ Department of Statistics, The Ohio State University, 43210, Columbus, OH, USA

^c hgrie@gwu.edu

Received: 8 May 2020
Accepted: 29 January 2021
Published online: 27 February 2021

Abstract

Interpreting measurements requires a physical theory, but the theory’s accuracy may vary across the experimental domain. To optimize experimental design, and so to ensure that the substantial resources necessary for modern experiments are focused on acquiring the most valuable data, both the theory uncertainty and the expected pattern of experimental errors must be considered. We develop a Bayesian approach to this problem, and apply it to the example of proton Compton scattering. Chiral Effective Field Theory (EFT) predicts the functional form of the scattering amplitude for this reaction, so that the electromagnetic polarizabilities of the nucleon can be inferred from data. With increasing photon energy, both experimental rates and sensitivities to polarizabilities increase, but the accuracy of EFT decreases. Our physics-based model of EFT truncation errors is combined with present knowledge of the polarizabilities and reasonable assumptions about experimental capabilities at HIS and MAMI to assess the information gain from measuring specific observables at specific kinematics, i.e.  to determine the relative amount by which new data are apt to shrink uncertainties. The strongest gains would likely come from new data on the spin observables and at to 200 MeV and to . These would tightly constrain . New data on the differential cross section between 100 and 200 MeV and over a wide angle range will substantially improve constraints on , and . Good signals also exist around 160 MeV for and . Such data will be pivotal in the continuing quest to pin down the scalar polarizabilities and refine understanding of the spin polarizabilities.