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  4. Improved parametrization of K[superscript +] production in p-Be collisions at low energy using Feynman scaling

Improved parametrization of K[superscript +] production in p-Be collisions at low energy using Feynman scaling

Author(s)
Mariani, C.
•
Cheng, G.
•
Shaevitz, M. H.
•
Conrad, Janet
Alternative Title
Improved parametrization of K+ production in p-Be collisions at low energy using Feynman scaling
Date Issued
December 2011
Journal
Physical Review D
Publisher
American Physical Society (APS)
Citation
Mariani, C. et al. “Improved Parametrization of K^{+} Production in p-Be Collisions at Low Energy Using Feynman Scaling.” Physical Review D 84.11 (2011): n. pag. Web. 2 Mar. 2012. © 2011 American Physical Society
Version
Final published version
Abstract
This paper describes an improved parametrization for proton-beryllium production of secondary K[superscript +] mesons for experiments with primary proton beams from 8.89 to 24  GeV/c. The parametrization is based on Feynman scaling in which the invariant cross section is described as a function of x[subscript F] and p[subscript T]. This method is theoretically motivated and provides a better description of the energy dependence of kaon production at low beam energies than other parametrizations such as the commonly used modified Sanford-Wang model. This Feynman scaling parametrization has been used for the simulation of the neutrino flux from the Booster Neutrino Beam at Fermilab and has been shown to agree with the neutrino interaction data from the SciBooNE experiment. This parametrization will also be useful for future neutrino experiments with low primary beam energies, such as those planned for the Project X accelerator.
MIT Department
Massachusetts Institute of Technology. Department of Physics
Terms of Use
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/1721.1/69570
DOI of Published Version
https://doi.org/10.1103/PhysRevD.84.114021
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