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

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where the effective coefficients aA <strong>and</strong> aE correspond to W -annihilation <strong>and</strong> W -exchange amplitu<strong>de</strong>s<br />

respectively. Strong phases relative to the emission diagrams are also consi<strong>de</strong>red in these<br />

coefficients.<br />

For the P V mo<strong>de</strong>s, the effective strong coupling constants are <strong>de</strong>fined through the Lagrangian<br />

LV P P = igV P P V µ (P1∂µP2 − P2∂µP1), (6)<br />

where gV P P is dimensionless <strong>and</strong> obtained from experiments. By inserting the propagator of<br />

the intermediate state M, the annihilation amplitu<strong>de</strong>s are<br />

〈P V |Heff |D〉 = GF<br />

1<br />

√2 VCKMaA,EfMfDm 2 D<br />

m2 D − m2 gV P M2(ε<br />

M<br />

∗ · pD). (7)<br />

As for the P P mo<strong>de</strong>s, the intermediate mesons are scalar particles. The effective strong coupling<br />

constants are <strong>de</strong>scribed by<br />

LSP P = −gSP P mSSP P. (8)<br />

However, the <strong>de</strong>cay constants of scalar mesons are very small, which is shown in the following<br />

relation<br />

fS<br />

¯fS<br />

= m2(µ) − m1(µ)<br />

, (9)<br />

mS<br />

where fS is the vector <strong>de</strong>cay constant used in the pole mo<strong>de</strong>l, ¯ fS is the scale-in<strong>de</strong>pen<strong>de</strong>nt scalar<br />

<strong>de</strong>cay constant, m1,2 are the running current quark mass, <strong>and</strong> mS is the mass of scalar meson.<br />

Therefore, the scalar pole contribution is very small, resulting in little resonant effect of annihilation<br />

type contributions in the P P mo<strong>de</strong>s. On the contrary, large annihilation contributions are<br />

given in the P V mo<strong>de</strong>s by relative large <strong>de</strong>cay constants of intermediate pseudoscalar mesons.<br />

3 Numerical results <strong>and</strong> discussions<br />

In this method, only the effective Wilson coefficients with relative strong phases are free parameters,<br />

which are chosen to obtain the suitable results consistent with experimental data. For<br />

P P mo<strong>de</strong>s,<br />

For P V mo<strong>de</strong>s,<br />

a1 = 0.94 ± 0.10, a2 = (0.65 ± 0.10)e i(142±10)◦<br />

,<br />

aA = (0.20 ± 0.10)e i(300±10)◦<br />

, aE = (1.7 ± 0.1)e i(90±10)◦<br />

. (10)<br />

P V<br />

a<br />

P V<br />

P V<br />

1 = 1.32 ± 0.10, a2 = (0.75 ± 0.10)e i(160±10)◦<br />

,<br />

aA = (0.12 ± 0.10)e i(345±10)◦<br />

,<br />

P V<br />

aE = (0.62 ± 0.10)e i(238±10)◦<br />

. (11)<br />

All the predictions of the 100 channels are shown in the tables of ref. 9 . The prediction of<br />

branching ratio of the pure annihilation process D + s → π + π 0 vanishes in the pole mo<strong>de</strong>l within<br />

the isospin symmetry. It is also zero in the diagrammatic approach in the flavor SU(3) symmetry.<br />

Simply, two pions can form an isospin 0,1,2 state, but 0 is ruled out because of charged final<br />

states, <strong>and</strong> isospin-2 is forbid<strong>de</strong>n for the leading or<strong>de</strong>r ∆C = 1 weak <strong>de</strong>cay. The only left s-wave<br />

isospin-1 sate is forbid<strong>de</strong>n by Bose-Einstein statics. In the pole mo<strong>de</strong>l language, G parity is<br />

violated in the isospin-1 case. Therefore, no annihilation amplitu<strong>de</strong> contributes to this mo<strong>de</strong>.<br />

The theoretical analysis in the η − η ′ sector is kind of complicated. The predictions with η ′<br />

in the final state are always smaller in this hybrid method than those case of η due to the smaller<br />

phase space. However, it is opposite by experiments in some mo<strong>de</strong>s, such as D + s → π + η(η ′ ),

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