Search for B[subscript s][superscript 0]→μ[superscript +]μ[superscript -] and B[superscript 0]→μ[superscript +]μ[superscript -] Decays with CDF II
Name
Aaltonen-2011-Letters-Search for B0s.pdf
Size
203.93 KB
Format
Adobe PDF
Checksum (MD5)
867489dfbe616cf5b497051d5f50516e
Author(s) • • • •
Gomez-Ceballos, Guillelmo
Goncharov, Maxim
Makhoul, Khaldoun
Paus, Christoph M. E.
Bauer, Gerry P
Date Issued
November 2011
Journal
Physical Review Letters
Publisher
American Physical Society
Citation
Aaltonen, T. et al. “Search for B_{s}^{0}→μ^{+}μ^{-} and B^{0}→μ^{+}μ^{-} Decays with CDF II.” Physical Review Letters 107.19 (2011). © 2011 American Physical Society
Version
Final published version
Abstract
A search has been performed for B[subscript s][superscript 0]→μ[superscript +]μ[superscript -] and B[superscript 0]→μ[superscript +]μ[superscript -] decays using 7 fb[superscript -1] of integrated luminosity collected by the CDF II detector at the Fermilab Tevatron collider. The observed number of B[superscript 0] candidates is consistent with background-only expectations and yields an upper limit on the branching fraction of B(B[superscript 0]→μ[superscript +]μ[superscript -])<6.0×10-[superscript 9] at 95% confidence level. We observe an excess of B[subscript s][superscript 0] candidates. The probability that the background processes alone could produce such an excess or larger is 0.27%. The probability that the combination of background and the expected standard model rate of B[subscript s][superscript 0]→μ[superscript +]μ[superscript -] could produce such an excess or larger is 1.9%. These data are used to determine B(B[subscript s][superscript 0]→μ[superscript +]μ[superscript -])= (1.8[subscript -0.9][superscript+1.1])×10[superscript -8] and provide an upper limit of B(B[subscripts 0]→μ[superscript +] μ[superscript -])<4.0×10[superscript -8] at 95% confidence level.
MIT Department
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
DOI of Published Version
https://doi.org/10.1103/PhysRevLett.107.191801