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2011 QCD and High Energy Interactions - Rencontres de Moriond ...

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η → π + π − π 0 η ′ → γπ + π −<br />

a)<br />

η → π0π0π 0 η ′ → π + π− b)<br />

η<br />

c)<br />

d)<br />

π 0 → γγ e)<br />

Figure 5: Mass distributions of the pseudo-scalar meson c<strong>and</strong>idates for ψ ′ → γP : γη [ a): η → π + π − π 0 ; b):<br />

η → π 0 π 0 π 0 ], γη ′ [ c): η ′ → γπ + π − ; d): η ′ → π + π − η, η → γγ], γπ 0 [ e): π 0 → γγ]. For more <strong>de</strong>tails see 12 .<br />

<strong>and</strong> B(χ c1 → φω) = (2.2 ± 0.6 ± 0.2) × 10 −5 are also observed for the first time. This analysis<br />

is <strong>de</strong>scribed in <strong>de</strong>tails in 10 .<br />

7 ψ ′ → γP, P = π 0 , η, η ′ ; η → π + π − π 0 , η → 3π 0 , η ′ → γπ + π − , η ′ →<br />

π + π − η (η, π 0 → γγ)<br />

The processes ψ ′ → γπ 0 <strong>and</strong> ψ ′ → γη are observed for the first time with signal significances<br />

of 4.6σ <strong>and</strong> 4.3σ (Fig. 5), <strong>and</strong> branching fractions B(ψ ′ → γπ 0 ) = (1.58 ± 0.40 ± 0.13) × 10 −6<br />

<strong>and</strong> B(ψ ′ → γη) = (1.38 ± 0.48 ± 0.09) × 10 −6 , respectively; the first errors are statistical <strong>and</strong><br />

the second ones systematic. The branching fraction B(ψ ′ → γη ′ ) = (126 ± 3 ± 8) × 10 −6 is<br />

measured as well, leading for the first time to the <strong>de</strong>termination of the ratio of the η <strong>and</strong> η ′<br />

production rates from ψ ′ <strong>de</strong>cays, Rψ ′ = B(ψ′ → γη)/B(ψ ′ → γη ′ ) = (1.10 ± 0.38 ± 0.07)%; such<br />

ratio is below the 90% C.L. upper bound <strong>de</strong>termined by the CLEO Collaboration 11 <strong>and</strong> one<br />

or<strong>de</strong>r of magnitu<strong>de</strong> smaller w.r.t the corresponding η − η ′ production ratio for the J/ψ <strong>de</strong>cays,<br />

R J/ψ = (21.1 ± 0.9)% 11 . For a <strong>de</strong>tailed <strong>de</strong>scription of this analysis see 12 .<br />

References<br />

1. D. M. Asner et al. arXiv:0809.1869 [hep-ex].<br />

2. M. Ablikim et al. Nucl. Instrum. Meth. A 614 (2010) 345 [arXiv:0911.4960 [phys.ins-<strong>de</strong>t]].<br />

3. M. Ablikim et al. Phys. Rev. Lett. 104 (2010) 132002 [arXiv:1002.0501 [hep-ex]].<br />

4. S. Dobbs et al. Phys. Rev. Lett. 101 (2008) 182003 [arXiv:0805.4599 [hep-ex]].<br />

5. M. Ablikim et al. Phys. Rev. D 81 (2010) 052005 [arXiv:1001.5360 [hep-ex]].<br />

6. M. Ablikim et al. Phys. Rev. D 83 (<strong>2011</strong>) 012006 [arXiv:1011.6556 [hep-ex]].<br />

7. J. V. Bennett et al. Phys. Rev. Lett. 101 (2008) 151801 [arXiv:0807.3718 [hep-ex]].<br />

8. M. Ablikim et al. arXiv:1103.5564 [hep-ex].<br />

9. K. Nakamura et al. J. Phys. G 37 (2010) 075021.<br />

10. M. Ablikim et al. arXiv:1104.5068 [hep-ex].<br />

11. T. K. Pedlar et al. Phys. Rev. D 79, 111101 (2009) [arXiv:0904.1394 [hep-ex]].<br />

12. M. Ablikim et al. Phys. Rev. Lett. 105 (2010) 261801 [arXiv:1011.0885 [hep-ex]].

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