Measurement of the antineutrino to neutrino charged-current interaction cross section ratio in MINERvA

L. Ren, L. Aliaga, O. Altinok, L. Bellantoni, A. Bercellie, M. Betancourt, A. Bodek, A. Bravar, H. Budd, T. Cai, M. F. Carneiro, H. Da Motta, J. Devan, S. A. Dytman, G. A. Díaz, B. Eberly, E. Endress, J. Felix, L. Fields, R. FineA. M. Gago, R. Galindo, H. Gallagher, A. Ghosh, T. Golan, R. Gran, J. Y. Han, D. A. Harris, K. Hurtado, M. Kiveni, J. Kleykamp, M. Kordosky, T. Le, E. Maher, S. Manly, W. A. Mann, C. M. Marshall, D. A. Martinez Caicedo, K. S. McFarland, C. L. McGivern, A. M. McGowan, B. Messerly, J. Miller, A. Mislivec, J. G. Morfín, J. Mousseau, D. Naples, J. K. Nelson, A. Norrick, Nuruzzaman, (MINERνA Collaboration)

Research output: Contribution to journalArticlepeer-review

15 Scopus citations

Abstract

We present measurements of the neutrino and antineutrino total charged-current cross sections on carbon and their ratio using the MINERvA scintillator-tracker. The measurements span the energy range 2-22 GeV and were performed using forward and reversed horn focusing modes of the Fermilab low-energy NuMI beam to obtain large neutrino and antineutrino samples. The flux is obtained using a subsample of charged-current events at low hadronic energy transfer along with precise higher energy external neutrino cross section data overlapping with our energy range between 12-22 GeV. We also report on the antineutrino-neutrino cross section ratio, RCC, which does not rely on external normalization information. Our ratio measurement, obtained within the same experiment using the same technique, benefits from the cancellation of common sample systematic uncertainties and reaches a precision of ∼5% at low energy. Our results for the antineutrino-nucleus scattering cross section and for RCC are the most precise to date in the energy range Eν<6 GeV.

Original languageEnglish (US)
Article number072009
JournalPhysical Review D
Volume95
Issue number7
DOIs
StatePublished - Apr 1 2017

Bibliographical note

Funding Information:
This work was supported by the Fermi National Accelerator Laboratory under U.S. Department of Energy Contract No. DE-AC02-07CH11359 which included the MINERvA construction project. Construction support was also granted by the United States National Science Foundation under Grant No. PHY-0619727 and by the University of Rochester. Support for participating scientists was provided by NSF and DOE (USA), by CAPES and CNPq (Brazil), by CoNaCyT (Mexico), by CONICYT programs including FONDECYT (Chile), by CONCYTEC, DGI-PUCP, and IDI/IGI-UNI (Peru).

Publisher Copyright:
© 2017 American Physical Society.

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