Note on OPE production amplitudes [#!aa!#]
Adam Szczepaniak, 08/25/99 pt

Charge exchange, OPE production amplitudes of $Y^0\pi ^+$ (Y is the isobar) via a1, a2, $\pi_2$ and $\hat\rho$.


\begin{displaymath}
\gamma p \to X^+ n \to Y^0 \pi^+ n (\to \pi^+\pi^-\pi^+ n)
\end{displaymath} (1)


\begin{displaymath}
{{d^2\sigma }\over {dtdM_{\rho \pi }d\Omega_k}}= {1\over 2}
...
...\Omega_k,\lambda_\gamma,\lambda_N,\lambda'_N,\lambda_Y)\vert^2
\end{displaymath} (2)

Spin projections of the isobar, $\lambda_Y$ and resonances, $\lambda_X$, $M_{Y\pi}$, (see below) are defined in the GJ frame i.e. resonance at rest, photon momentum along the z axis, ( $\lambda_\gamma$=photon helicity). In contrast, nucleon will be parametrized by its helicity.

The amplitude A is written as a product of the production amplitude AOPE (production as defined by Dennis) and the amplitude T for the resonance (assumed BW) to decay into $Y\pi$. (I think Dennis has that in his code, I'm giving it here to completeness),


\begin{displaymath}
A = \sum_{X,J^P,\lambda_X}A_{OPE}(s,t,\lambda_N,\lambda_\ga...
...,\lambda_X)
T(M_{Y^0\pi^+},\Omega_k,J^P,\lambda_X,\lambda_Y)
\end{displaymath} (3)


$\displaystyle A_{OPE}(s,t,\lambda_N,\lambda_\gamma,\lambda_N',J^P,\lambda_X
)$ = $\displaystyle \sqrt{2} g_{\pi NN} \left({s\over {s_0}}\right)^{\alpha_\pi(t)}
{{\sqrt{t'} }\over (t - m_\pi^2)}\beta(t)\delta_{\lambda_N,-\lambda'_N}$  
  x $\displaystyle \sum_{L_\gamma}\sqrt{{2L_\gamma+1}\over {4\pi}}\langle J,\lambda_...
...rangle
\left( {{\omega}\over m_X}\right)^{L_\gamma} g^{L_\gamma}_{X\gamma\pi}
.$ (4)

Here t'=|t-tmin|, $\omega=\lambda(m_X,0,t)$ is the breakup momentum of the resonance X with mass mX decaying into photon and an off-shell pion with mass t, $g_{\pi NN}^2/(4\pi) \sim 14.4$, $s=2E_\gamma m_n + m_n^2$, and $\alpha_\pi=0.9\mbox{GeV}^{-2}(t-m_\pi^2)$. The form factor $\beta(t)$ was fitted to the $\gamma p \to a^+_2 n$ data from Ref. [#!a21!#], [#!a22!#] and is given by

\begin{displaymath}
\beta(t) = (a_1 e^{b_1 t } + a_2 e^{b_2 t})^{1/2}
\end{displaymath} (5)

with $b_1 \sim 35\mbox{GeV}^{-2}$, $b_2 \sim 3\mbox{GeV}^{-2}$, $a_1
\sim 30$, $a_2 \sim 1.5$ for $s_0 = 10\mbox{GeV}^2$.


$\displaystyle T(M_{Y^0\pi^+},\Omega_k,J^P,\lambda_X,\lambda_Y)$ = $\displaystyle \sum_{L_{Y\pi}M_{Y\pi}}
{ {m_X g^{L_{Y\pi}}_{XY^0\pi^+}}\over {2(...
...ma_{X,J^P}}\over 2} ) } } \left( {{k_{Y\pi}(m_X)}\over {m_x}}\right)^{L_{Y\pi}}$  
  x $\displaystyle \langle s_Y\lambda_Y,L_{Y\pi}M_{Y\pi}\vert J_X\lambda_X\rangle Y_{L_{Y\pi},M_{Y\pi}}(\Omega_k)$ (6)

The photocouplings $g^{L_\gamma}_{X\gamma\pi}$ are calculated from the radiative widths $\Gamma_{X\gamma\pi}$ using


    $\displaystyle \Gamma_{X\to \gamma\pi}(E) = m_X \sum_{L_\gamma,L'_\gamma}
{{g^{L...
...gamma\pi}}\over {32\pi^2}}
\left({{q}\over {m_x}}\right)^{L_\gamma+L'_\gamma+1}$  
  x $\displaystyle \left[\delta_{L_\gamma,L'_\gamma}\left(\delta_{L_\gamma,J} + \del...
...'_\gamma,J+1}\delta_{L_\gamma,J-1}\right)
{{\sqrt{J(J+1)}}\over {2J+1}}\right],$  

with $q=\lambda(m_X,0,m_\pi)$. Note that, if there is more then one partial amplitude, $L_\gamma$ contributing, $\Gamma_{X\gamma\pi}$ determines only a product of different couplings. In such a case, to completely determine all $g^{L_\gamma}_{X\gamma\pi}$'s we assumed that the amplitude ratios are the same as for $X\to \rho\pi$.

The strong couplings are computed from


\begin{displaymath}
\Gamma^{L_{Y\pi}}_{X,J^P} = m_X {{ (g^{L_{Y\pi}}_{XY\pi})^2 ...
...2\pi^2}}
\left( {{k_{Y\pi}}\over {m_X}} \right)^{2L_{Y\pi}+1}.
\end{displaymath} (7)

Here $k_{Y\pi} = \lambda(m_X,m_Y,m_\pi)$ is the resonance breakup momentum. Photocouplings and strong couplings to selected $Y\pi$ channels are summarized in Table 2. These are calculated from Eqs. 78 using, where known, the PDG values [*] for $\Gamma_{X\gamma\pi}$ and $\Gamma^{L_{Y\pi}}_{X,J^P}$ and ``reasonable guesses'' otherwise, (all listed in Table. 1).


\begin{references}
\par\bibitem{aa} A.~Afanasev and A.P.~Szczepaniak almost fini...
...G.T.~Condo {\it et al.}, Phys. Rev. {\bf D}48, 3045 (1993).
\par\end{references}


Table I: Resonance parameters. $\rho \pi $ widths are taken from the PDG. $\Gamma $ is the total hadronic width, $\Gamma = \sum _{AB,L_{AB}}\Gamma ^{L_{AB}}_{XAB}$ and $\Gamma ^e$ is the total radiative width to $\gamma \pi $ Here I have assumed that resonances can be saturated by the (two body) decay channels listed above. This is close to reality, however in principle on can recalculate the couplings in Table 2 for the ``true'' PDG values''. (This assumption was made to make the theoretical model of Ref. [1] simpler).
Resonance JPC Mass[GeV] Partial waves $\Gamma^{L_{AB}}_{XAB}/
\Gamma$ $\Gamma $[MeV] $\Gamma ^e$[keV]
decay channel     (LAB, $L_\gamma=L^{\rho\pi})$      
a1 1++ 1.26     400 640
$\;\;\;\;\;\;\rho\pi$     S 0.99    
      D 0.01    
a2 2++ 1.32     110 295
$\;\;\;\;\;\;\rho\pi$     D 0.70    
$\;\;\;\;\;\eta\pi$     D 0.30    
$\pi_2$ 2-+ 1.67     258 300
$\;\;\;\;\;\;\rho\pi$     P 0.98*0.31    
      F 0.02*0.31    
$\;\;\;\;\;\;f_2\pi$     S 0.69    
$\hat\rho$ 1-+ 1.6     400 170
$\;\;\;\;\;\;\rho\pi$     P 0.50    
$\;\;\;\;\;\;b_1\pi$     S 0.50    



Table II: Strong and electromagnetic couplings corresponding to (BW) widths given in Table 1. Strong couplings, $g^{L_{Y\pi }}_{XY^0\pi ^+}$ to the charged state $Y^0\pi ^+$ when Y0 is part of an isovector should be reduced by $\sqrt {2}$.
Resonance Partial wave ${{(g^{L_{AB}}_{XAB}(k_{AB}(m_X)))^2}\over {4\pi}}$ ${{(g^{L_\gamma}_{X\gamma\pi})^2}\over {4\pi}}$
decay channel      
a1      
$\;\;\;\;\;\;\rho\pi$ S 26.28 1.03
  D 32.54 1.04 x 10-2
a2      
$\;\;\;\;\;\;\rho\pi$ D 442.4 2.37
$\;\;\;\;\;\;\eta\pi$ D 57.08 72.71
$\pi_2$      
$\;\;\;\;\;\;\rho\pi$ P 20.01 1.74
  F 20.15 4.01 x 10-2
$\;\;\;\;\;\;f_2\pi$ S 13.72  
$\hat\rho$      
$\;\;\;\;\;\;\rho\pi$ P 24.59 1.51
$\;\;\;\;\;\;b_1\pi$ S 7.12  



Footnotes

... values [*]
See caption for Table.1



1999-09-17