Comment on definition of the naturality basis for
photons.
Adam Szczepaniak, June 30 (somewhere over the Atlantic)
Let
be the GJ amplitude for production
of a resonance of spin
, naturality,
, and spin projection
in the GJ frame,
with
's
referring to helicities of the photon, and the initial and final nucleon.
For a
exchange, the upper (photon coupling)
vertex is invariant under
reflection in the production plane, the
-parity, which leads to
 =
-\tau_...
...u_e (-)^m[J,\tau_X](-\lambda_\gamma ,-m,\lambda_N ,\lambda'_N)
\end{displaymath}](img12.gif) |
(1) |
Here
is the naturality of the exchange. Similarly for the
lower (nucleon) vertex
 =
\tau_...
...ambda_N } [J,\tau_X](\lambda_\gamma ,m-\lambda_N ,-\lambda'_N)
\end{displaymath}](img14.gif) |
(2) |
We want rewrite the spin density matrix
![\begin{displaymath}
\rho^{[J\tau_X],[J'\tau'_X]}_{m,m'}(\lambda_\gamma ,\lambda_...
..._N)
[J',\tau'_X]^*(\lambda_\gamma ',m',\lambda_N ,\lambda'_N)
\end{displaymath}](img15.gif) |
(3) |
in terms of the eigenstates of the reflectivity operator. This
will split up natural from unnatural exchanges.
In the reflectivity basis (for both photon and produced resonance)
the amplitudes are given by (
),
![\begin{displaymath}[J,\tau_X]^{\epsilon_\gamma \epsilon_X }(\vert m\vert,\lambda...
...[J,\tau_X]^{\epsilon_\gamma }(-m,\lambda_N ,\lambda'_N)\right]
\end{displaymath}](img17.gif) |
(4) |
where
for
and
for
and
![\begin{displaymath}[J,\tau_X]^{\epsilon_\gamma }(m,\lambda_N ,\lambda'_N) = {1\o...
...J,\tau_X](\lambda_\gamma =-1,m,\lambda_N ,\lambda'_N)
\right]
\end{displaymath}](img22.gif) |
(5) |
For given
there are
amplitudes. Parity
eliminates half of them and the remaining
amplitudes are
split into noninterfering amplitudes describing natural and unnatural
exchange mechanisms.
Using Eq. 1 one can show that these are given by
The amplitudes
correspond to
photons linearly polarized in the production plane and
to photons polarized
perpendicular to the production plane
Finally,
label the
reflectivity basis of the produced resonance
![\begin{displaymath}
\vert [J_X,\tau_X], \epsilon_X ,\vert m\vert \rangle = \thet...
... \tau_X (-)^m
\vert[J_X,\tau,X],-\vert m\vert \rangle \right]
\end{displaymath}](img39.gif) |
(6) |
In terms of these amplitudes the density matrix is given by
Here
is the orientation of the photon polarization vector
with respect to the direction perpendicular to the production plane
(in the GJ frame). Sum over nucleon helicities is implicit i.e
In this case the nonvanishing amplitudes are :

-
Natural exchange
and
Unnatural exchange
and
![$[a_1]^{-+}(\vert m\vert = 1)$](img52.gif)

-
Natural exchange
and
Unnatural exchange
and
![$[a_2]^{-+}(\vert m\vert = 2,1,0)$](img56.gif)

-
Natural exchange
and
Unnatural exchange
and
![$[\pi_1]^{-+}(\vert m\vert = 1,0)$](img60.gif)

-
Natural exchange
and
Unnatural exchange
and
Here dependence on nucleon spin is implicit, one needs (in
general) a spin-nonflip and a spin flip amplitude. However if
nucleon polarization information is unavailable one will measure a
coherent sum of the two (cf Eq. 10).
In this case
 = A \delta_{\lambda_N ,-\lambda_N '}\tau^3_{\lambda_\gamma ,m}
\end{displaymath}](img65.gif) |
(7) |
(
is the Pauli matrix)
>From Eq. 4 for the only nonvanishing amplitudes one gets
![\begin{displaymath}[a_2]^{+-}(\lambda_\gamma = 1,\lambda_N ,\lambda'_N) = [a_2]^...
...= 1,\lambda_N ,\lambda'_N) =
A\delta_{\lambda_N ,-\lambda'_N}
\end{displaymath}](img67.gif) |
(8) |
i.e. only nucleon helicity flip contributes.
The spin density matrix are then given by
In the helicity basis the photon density matrix is given by
where
is the degree of linear polarization and
 |
(11) |
In the basis of linearly polarized photons :
this gives (
)
 |
(13) |
This is diagonal in the basis given by two orthogonal vectors
corresponding to eigenvalues
and
respectively.
It s now straightforward to generalize resonance production spin
density matrix
to the
case when
Curtis A. Meyer
2000-07-28