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  4. Dalitz plot analysis of the decay B[superscript ±]→K[superscript ±]K[superscript ±]K[superscript ∓]

Dalitz plot analysis of the decay B[superscript ±]→K[superscript ±]K[superscript ±]K[superscript ∓]

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Author(s)
Koeneke, Karsten
•
Sciolla, Gabriella
•
Cowan, Ray F
•
Sekula, S. J.
•
Spitznagel, Michael A
•
Yamamoto, R. K.
•
Taylor, Frank E
Date Issued
August 2006
Journal
Physical Review D
Publisher
American Physical Society
Citation
Aubert, B. et al. “Dalitz plot analysis of the decay B[superscript ±]→K[superscript ±]K[superscript ±]K[superscript ∓]” Physical Review D 74.3 (2006). © 2006 The American Physical Society
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Final published version
Abstract
We analyze the three-body charmless decay B[superscript ±]→K[superscript ±]K[superscript ±]K[superscript ∓] using a sample of 226.0±2.5 million BB̅ pairs collected by the BABAR detector. We measure the total branching fraction and CP asymmetry to be B=(35.2±0.9±1.6)×10[superscript -6] and A[subscript CP]=(-1.7±2.6±1.5)%. We fit the Dalitz plot distribution using an isobar model and measure the magnitudes and phases of the decay coefficients. We find no evidence of CP violation for the individual components of the isobar model. The decay dynamics is dominated by the K[superscript +]K[superscript -] S-wave, for which we perform a partial-wave analysis in the region m(K[superscript +]K[superscript -])<2  GeV/c[superscript 2]. Significant production of the f[subscript 0](980) resonance, and of a spin zero state near 1.55  GeV/c[superscript 2] are required in the isobar model description of the data. The partial-wave analysis supports this observation.
MIT Department
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Laboratory for Nuclear Science
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/1721.1/76202
DOI of Published Version
https://doi.org/10.1103/PhysRevD.74.032003
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