PT Journal AU DUNE Collaboration (Abud, AAea Amedo, P Antonova, M Barenboim, G Benitez Montiel, C Cervera-Villanueva, A De Romeri, V Garcia-Peris, MA Lopez March, N Martin-Albo, J Martinez Mirave, P Mena, O Molina Bueno, L Novella, P Pompa, F Rocabado Rocha, JL Sorel, M Soto-Oton, J Tortola, M Tuzi, M Valle, JWF Yahlali, N TI Impact of cross-section uncertainties on supernova neutrino spectral parameter fitting in the Deep Underground Neutrino Experiment SO Physical Review D JI Phys. Rev. D PY 2023 BP 112012 EP 25pp VL 107 IS 11 DI 10.1103/PhysRevD.107.112012 LA English AB A primary goal of the upcoming Deep Underground Neutrino Experiment (DUNE) is to measure the Oo10 thorn MeV neutrinos produced by a Galactic core-collapse supernova if one should occur during the lifetime of the experiment. The liquid-argon-based detectors planned for DUNE are expected to be uniquely sensitive to the & nu;e component of the supernova flux, enabling a wide variety of physics and astrophysics measurements. A key requirement for a correct interpretation of these measurements is a good understanding of the energy-dependent total cross section & sigma;oE & nu; thorn for charged-current & nu;e absorption on argon. In the context of a simulated extraction of supernova & nu;e spectral parameters from a toy analysis, we investigate the impact of & sigma;oE & nu; thorn modeling uncertainties on DUNE's supernova neutrino physics sensitivity for the first time. We find that the currently large theoretical uncertainties on & sigma;oE & nu; thorn must be substantially reduced before the & nu;e flux parameters can be extracted reliably; in the absence of external constraints, a measurement of the integrated neutrino luminosity with less than 10% bias with DUNE requires & sigma;oE & nu; thorn to be known to about 5%. The neutrino spectral shape parameters can be known to better than 10% for a 20% uncertainty on the cross-section scale, although they will be sensitive to uncertainties on the shape of & sigma;oE & nu; thorn . A direct measurement of low-energy & nu;e-argon scattering would be invaluable for improving the theoretical precision to the needed level. ER