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Coincidence charged-current neutrino-induced deuteron disintegration

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Author(s)
Van Orden, J. W.
•
Ford, W. P.
•
Moreno Diaz, Oscar
•
Donnelly, T William
Date Issued
September 2015
Journal
Physical Review D
Publisher
American Physical Society
Citation
Moreno, O., T. W. Donnelly, J. W. Van Orden, and W. P. Ford. "Coincidence charged-current neutrino-induced deuteron disintegration." Phys. Rev. D 92, 053006 (September 2015). © 2015 American Physical Society
Version
Final published version
Abstract
Deuteron disintegration by charged-current neutrino (CCν) scattering offers the possibility to determine the energy of the incident neutrino by measuring in coincidence two of the three resulting particles: a charged lepton (usually a muon) and two protons, where we show that this channel can be isolated from all others—for instance, from those with a pion in the final state. We discuss the kinematics of the process for several detection scenarios, both in terms of kinematic variables that are natural from a theoretical point of view and others that are better matched to experimental situations. The deuteron structure is obtained from a relativistic model (involving an approximation to the Bethe-Salpeter equation) as an extension of a previous, well-tested model used in deuteron electrodisintegration. We provide inclusive and coincidence (semi-inclusive) cross sections for a variety of kinematic conditions, using the plane-wave impulse approximation, introducing final-state hadronic exchange terms (plane-wave Born approximation) and final-state hadronic interactions (distorted-wave Born approximation).
MIT Department
Massachusetts Institute of Technology. Center for Theoretical Physics
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Laboratory for Nuclear Science
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Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
http://hdl.handle.net/1721.1/98528
DOI of Published Version
https://doi.org/10.1103/PhysRevD.92.053006
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