Model-Independent Search for CP Violation in D[superscript 0]→K[superscript −]K[superscript +]π[superscript −]π[superscript +] and D[superscript 0]→π[superscript −]π[superscript +]π[superscript +]π[superscript −] Decays
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Author(s)
Williams, Michael
Date Issued
November 2013
Journal
Physics Letters B
Publisher
Elsevier BV
Citation
Aaij, R., et al. “Model-Independent Search for CP Violation in D[superscript 0]→K[superscript −]K[superscript +]π[superscript −]π[superscript +] and D[superscript 0]→π[superscript −]π[superscript +]π[superscript +]π[superscript −] Decays.” Physics Letters B, vol. 726, no. 4–5, Nov. 2013, pp. 623–33.
© CERN for the benefit of the LHCb Collaboration
Version
Final published version
Abstract
A search for CP violation in the phase-space structures of D[superscript 0] and [bar over D][superscript 0]decays to the final states K[superscript -]K[superscript +] π[superscript -]π[superscript +] and π[superscript -]π[superscript +]π[superscript +]π[superscript -] is presented. The search is carried out with a data set corresponding to an integrated luminosity of 1.0fb[superscript -1] collected in 2011 by the LHCb experiment in pp collisions at a centre-of-mass energy of . For the K[superscript -]K[superscript +]π[superscript -]π[superscript +] final state, the four-body phase space is divided into 32 bins, each bin with approximately 1800 decays. The p-value under the hypothesis of no CP violation is 9.1%, and in no bin is a CP asymmetry greater than 6.5% observed. The phase space of the π[superscript -]π[superscript +]π[superscript +]π[superscript -] final state is partitioned into 128 bins, each bin with approximately 2500 decays. The p-value under the hypothesis of no CP violation is 41%, and in no bin is a CP asymmetry greater than 5.5% observed. All results are consistent with the hypothesis of no CP violation at the current sensitivity.
MIT Department
Massachusetts Institute of Technology. Department of Physics
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Attribution 3.0 United States (CC BY 3.0 US)
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DOI of Published Version
https://doi.org/10.1016/J.PHYSLETB.2013.09.011