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Eur. Phys. J. A 42, 151–157 (2009) DOI: 10.1140/epja/i2009-10870-x
Measurement of Σ beam asymmetry in π0
pho-
toproduction off the neutron in the second and
third resonances region
R. Di Salvo, A. Fantini, G. Mandaglio, F. Mammoliti, O. Bartalini, V.
Bellini, J.P. Bocquet, L. Casano, A. D’angelo, J.P. Didelez, D. Franco,
G. Gervino, F. Ghio, G. Giardina, B. Girolami, A. Giusa, M. Guidal, E.
Hourany, R. Kunne, A. Lapik, P. Levi Sandri, A. Lleres, M. Manganaro,
D. Moricciani, A.N. Mushkarenkov, V. Nedorezov, C. Randieri, D. Re-
breyend, N. Rudnev, G. Russo, C. Schaerf, M.L. Sperduto, M.C. Sutera,
A. Turinge, V. Vegna, A. Fix, S.S. Kamalov and L. Tiator
DOI 10.1140/epja/i2009-10870-x
Regular Article – Experimental Physics
Eur. Phys. J. A 42, 151–157 (2009)
THE EUROPEAN
PHYSICAL JOURNAL A
Measurement of Σ beam asymmetry in π0
photoproduction off
the neutron in the second and third resonances region⋆
R. Di Salvo1
, A. Fantini1,10
, G. Mandaglio2,14
, F. Mammoliti2,11
, O. Bartalini3,10
, V. Bellini4,11
, J.P. Bocquet5
,
L. Casano1
, A. D’angelo1,10
, J.P. Didelez6
, D. Franco1,10
, G. Gervino7,12
, F. Ghio8,13
, G. Giardina2,14
, B. Girolami8,13
,
A. Giusa2,11
, M. Guidal6
, E. Hourany6†
, R. Kunne6
, A. Lapik9
, P. Levi Sandri3,a
, A. Lleres5
, M. Manganaro2,14
,
D. Moricciani1
, A.N. Mushkarenkov9
, V. Nedorezov9
, C. Randieri3,11
, D. Rebreyend5
, N. Rudnev9
, G. Russo2,11
,
C. Schaerf1,10
, M.L. Sperduto2,11
, M.C. Sutera2
, A. Turinge9
, V. Vegna1,10
, A. Fix15
, S.S. Kamalov16,17
, and
L. Tiator16
1
INFN - Sezione di Roma “Tor Vergata”, via della Ricerca Scientifica 1, I-00133 Roma, Italy
2
INFN - Sezione di Catania, via Santa Sofia 64, I-95123 Catania, Italy
3
INFN - Laboratori Nazionali di Frascati, via Enrico Fermi 40, I-00044 Frascati, Italy
4
INFN - Laboratori Nazionali del Sud, via Santa Sofia 64, I-95123 Catania, Italy
5
LPSC, Universit´e Joseph Fourier Grenoble 1, CNRS/IN2P3, Institut National Polytechnique de Grenoble, 53 Avenue des
Martyrs, 38026 Grenoble, France
6
IPNO, Universit´e de Paris-Sud 11, CNRS/IN2P3, 15 rue Georges Cl´emenceau, 91406 Orsay, France
7
INFN - Sezione di Torino, via P. Giuria, I-10125 Torino, Italy
8
INFN - Sezione di Roma, piazzale Aldo Moro 2, I-00185 Roma, Italy
9
Institute for Nuclear Research, 117312 Moscow, Russia
10
Dipartimento di Fisica, Universit`a di Roma “Tor Vergata”, via della Ricerca Scientifica 1, I-00133 Roma, Italy
11
Dipartimento di Fisica e Astronomia Universit`a di Catania, via Santa Sofia 64, I-95123 Catania, Italy
12
Universit`a di Torino, via P. Giuria, I-00125 Torino, Italy
13
Istituto Superiore di Sanit`a, viale Regina Elena 299, I-00161 Roma, Italy
14
Dipartimento di Fisica, Universit`a di Messina, salita Sperone 31, I-98166 Messina, Italy
15
Laboratory of Mathematical Physics, Tomsk Polytechnic University, 634050, Tomsk, Russia
16
Institut f¨ur Kernphysik, Johannes Gutenberg-Universit¨at Mainz, D-55099 Mainz, Germany
17
Laboratory of Theoretical Physics, JINR Dubna, 141980 Moscow region, Russia
Received: 21 April 2009 / Revised: 27 August 2009
Published online: 4 October 2009 – c Societ`a Italiana di Fisica / Springer-Verlag 2009
Communicated by Z.-E. Meziani
Abstract. The Σ beam asymmetry in the photoproduction of neutral pions from quasi-free nucleons in a
deuteron target was measured for the first time between 0.60 and 1.50 GeV, with the GRAAL polarized
and tagged photon beam. The asymmetry values from the quasi-free proton were found equal to the ones
extracted from a pure proton target. The asymmetries from quasi-free proton and quasi-free neutron were
found equal up to 0.82 GeV and substantially different at higher energies. The results are compared with
recent partial-wave analyses.
PACS. 13.60.Le Meson production – 13.88.+e Polarization in interactions and scattering – 25.20.Lj Pho-
toproduction reactions
1 Introduction
The availability over the last decade of high duty-cycle
accelerators coupled with the use of large solid-angle de-
tectors yielded a wealth of experimental information in
⋆
The authors of this work, except A. Fix, S.S. Kamalov and
L. Tiator, belong to The GRAAL Collaboration.
a
e-mail: paolo.levisandri@lnf.infn.it
†
Deceased.
the study of the photo- and electroproduction of mesons
from the proton. The attempt is to extract, from pho-
toproduction, the electromagnetic couplings and further-
more the hadronic properties of the excited nucleon states
that cannot be accessed via pion scattering, either because
the resonances largely overlap, or because of a weak cou-
pling to the single pion-nucleon channel.
In hadronic reactions induced by real photons, the po-
larization degrees of freedom play a crucial role, and offer
152 The European Physical Journal A
a complementary approach to the baryon spectroscopy.
Polarization observables arising from interference mecha-
nisms, are highly sensitive to the details of the interaction
revealing resonance properties that are difficult to extract
from a cross-section measurement, where a single contri-
bution often dominates [1–4].
The detailed description of the photon-nucleon inter-
action requires a complete data set containing, at least,
eight independent observables: the cross-section, the three
single polarization observables (beam, target and recoil
nucleon) and four, appropriately chosen, double polariza-
tion observables [5]. The resonance properties can then be
extracted from the photoproduction data via partial-wave
analysis and multipole decomposition, in the framework
of different approaches [3,6]. The comparison of the cal-
culated observables with the experimental data becomes a
strong constraint to the theoretical models [4,7], to deter-
mine the role and the properties of the resonance included.
The GRAAL Collaboration already provided a large
amount of precise polarization and cross-section data for
various meson photoproduction reactions on the proton.
In particular, the Σ beam asymmetry and the differen-
tial cross-section were measured for π0
photoproduction
in the 0.55–1.50 GeV energy range [8], bringing essential
constraints to the theoretical models and to partial-wave
analysis, and allowing to determine, within the model of
ref. [9] the spin of the new resonance N(2070) D15 in-
troduced in order to fit the large data set (see fig. 18 of
ref. [8]). In order to obtain complementary information,
and towards a full multipole analysis including the isospin
structure, data on meson photoproduction from the neu-
tron are of the utmost importance.
In sect. 2 we give a brief description of the experimen-
tal set-up. In sect. 3 the data analysis procedure is dis-
cussed, while in sect. 4 the Σ beam asymmetries on the
proton bound in the deuterium nucleus are compared with
those of the free proton; the asymmetries from the quasi-
free neutron are presented and are compared with quasi-
free proton results and with theoretical models. The effect
of these data on the multipole expansion is discussed. The
last section contains our conclusions.
2 Experimental set-up
The GRAAL experiment is based on the use of a tagged
and polarized photon beam obtained through the Comp-
ton back-scattering of laser light off the 6.03 GeV electrons
circulating in the ESRF storage ring. A full description of
the beam characteristics can be found in ref. [8]. The cou-
pling of the GRAAL beam with a large acceptance detec-
tor covering 0.95·4π solid angle with cylindrical symmetry
(Lagranγe) is the ideal tool in order to measure polariza-
tion degrees of freedom, in particular Σ beam asymme-
tries, with very small systematic errors. For the purposes
of this paper it is important to remember that the detector
is substantially divided into two parts:
1) a central part based on the BGO Rugby Ball calorime-
ter that covers laboratory angles 25◦
< θlab < 155◦
.
The calorimeter, coupled to a ∆E/∆x segmented scin-
tillation counter (called Barrel) for particle identifica-
tion, has an excellent energy resolution for photons [10]
and a high detection efficiency (> 40% depending on
the energy threshold) for neutrons [11];
2) a forward part (θlab < 25◦
) equipped with two plane
wire chambers, two scintillator walls and a Forward
Shower detector having a good neutron detection ef-
ficiency (∼ 22%) with momentum determination via
time-of-flight (T.O.F.) measurement (∼ 750 ps resolu-
tion for neutrons) [12].
The GRAAL experiment took data with a 6 cm length
deuterium target in six different periods from June 1999
until December 2005. Both the 514 nm green line (giving
rise to a 0.55–1.10 GeV tagged photon beam) and the 333–
368 nm UV line (0.80–1.50 GeV tagged photons) from the
Argon laser were used, with typical intensities of ∼ 106
γ/s.
Data taking was triggered by the coincidence between a
tagging signal (which determines the incident photon en-
ergy with 0.016 GeV FWHM resolution) and the total en-
ergy measured by the Rugby Ball, the latter being required
to be greater than 0.18 GeV. This condition gave rise to a
data acquisition rate ∼ 100 events/s and allowed to record
neutral pion photoproduction events both from quasi-free
neutrons and quasi-free protons. The beam polarization
can easily be changed by rotating the laser polarization.
During data taking the polarization was moved from verti-
cal (V) to horizontal (H) approximately every 20 minutes,
defining two orthogonal polarization states. About 10% of
the beam time was devoted to collect data with the un-
polarized beam (electron Bremsstrahlung on the residual
vacuum of the synchrotron doughnut).
3 Data analysis
Data on the neutral pion photoproduction from quasi-free
protons and from quasi-free neutrons were simultaneously
recorded and analysed in a similar way: two neutral sig-
nals in the BGO Rugby Ball were required to produce the
π0
invariant mass in the range 0.09–0.20 GeV/c2
(initial
preliminary selection see fig. 1).
Together with the two photons in the BGO, a proton
or a neutron signal was required, either in the forward di-
rection or in the BGO Rugby Ball. At forward angles, the
proton was identified via ∆E vs. T.O.F. (both measured
in the two scintillator wall) while a T.O.F. greater than
13.5 ns (measured in the Forward Shower) with no asso-
ciated track in the other detectors was used to select the
neutron. In the central region, the proton was identified
from the E vs. ∆E (measured in the Rugby Ball and in
the Barrel, respectively) whereas a low crystal multiplicity
(less than five) was the selection criterion for the candi-
date neutron. To select quasi-free kinematics (participant-
spectator approach), events with any additional signal(s)
were rejected.
These events were then required to fulfill the two-body
kinematics of the π0
N reaction, where N is the partici-
pating nucleon. Bidimensional cuts were applied on the
following quantities:
R. Di Salvo et al.: Σ beam asymmetry in π0
photoproduction off the neutron 153
Fig. 1. Invariant mass of the two photons from π0
decay before
(full line) and after (dashed line) the kinematical cuts, when
the neutron is detected in the forward direction. The obtained
resolution is typical of the Rugby Ball calorimeter.
Fig. 2. (Colour on-line) The ∆θ vs. ∆φ distribution (see text
for definitions of ∆θ and ∆φ).
– ∆θ vs. ∆φ, where ∆θ = θN − θM is the polar angle
difference between the measured and the theoretical
angle required to fulfill the two-body kinematics cal-
culated from Eγ, the measured energy Eπ0
m and the π0
production angle θπ0
. ∆φ is the difference (−180◦
) of
the measured azimuthal angles of π0
and N;
– the ratio Eπ0
c /Eπ0
m vs. Mx, where Eπ0
c is the π0
energy
calculated from the π0
and N measured angles, and
Mx is the missing mass calculated from Eγ and Eπ0
m .
In fig. 2 an example for a single Eγ energy bin of ∆θ
vs. ∆φ distribution is shown, while the Eπ0
c /Eπ0
m vs. Mx
distribution is displayed in fig. 3.
These two distributions were fitted with bidimensional
Gaussian functions: the mean values µ1, µ2 and the stan-
dard deviations σ1 and σ2 of the generic variables v1
and v2 were thus obtained. If the two Gaussians are
Fig. 3. (Colour on-line) The Eπ0
c /Eπ0
m vs. Mx distribution (see
text for definitions of Eπ0
c , Eπ0
m and Mx).
uncorrelated the cut applied to v1 and v2 is
(v1 − µ1)2
σ2
1
+
(v2 − µ2)2
σ2
2
< σ2
.
If the two variables are correlated, the correlation pa-
rameter C is extracted and the cut is defined as
(v1 − µ1)2
σ2
1
+
(v2 − µ2)2
σ2
2
− 2C
(v1 − µ1)(v2 − µ2)
σ1σ2
< σ2
.
In the event selection a value σ = 3 was used and
was determined by optimizing the signal/background ratio
in a full Monte Carlo simulation including all competing
channels, and based on the GEANT3 [13] package and a
realistic event generator [14].
Since the backgrounds and the detector resolutions
are a function of the energy of the incoming photon, the
cuts are extracted and applied as a function of the energy
bins. Once the events are selected, the beam asymmetry
Σ(Eγ, θcm) is extracted from the ratio
NV /kV
NV /kV + NH/kH
=
1
2
(1 + PΣ cos(2φ)),
where NH, NV are the yields obtained with the two
beam polarization states (horizontal and vertical), kH, kV
are the corresponding beam intensities, P(Eγ) is the de-
gree of linear polarization of the beam at a given energy,
Σ(Eγ, θcm) is the asymmetry as a function of the incom-
ing photon energy and of the polar angle of π0
in the
center-of-mass system, and φ is the π0
azimuthal angle.
For each bin of energy and θcm, the resulting φ distribu-
tion was fitted and the asymmetry Σ(Eγ, θcm) extracted.
A great care was used to determine θcm. The Fermi mo-
tion of the nucleon in the deuteron target is not negligi-
ble and the composition of the Fermi momentum with the
momentum of the incident photon causes a rotation of the
Lorentz boost axis off the direction of the beam. The eval-
uation of the Fermi momentum pF from the momentum
balance of the two-body kinematics
pF = pπ0 + pN − pγ
154 The European Physical Journal A
Fig. 4. The calculated neutron Fermi momentum distribution
before (full line) and after (dashed line) the kinematical cuts.
is affected in particular by the imprecise knowledge of the
momentum of the nucleon. The π0
energy and π0
and the
nucleon emission angles are the more suitable information
to use. Assuming a small Fermi energy (few MeV) for the
nucleon in the deuteron, one can write
Eextr
N = Eγ + MN − Eπ0 ,
pextr
N = (Eextr
N )2 − M2
N ,
where Eextr
N and pextr
N are the extracted energy and mo-
mentum of the outgoing nucleon. The extracted momen-
tum is then combined with the measured outgoing nucleon
angles to determine the three Cartesian components. The
Fermi momentum is then calculated as follows:
pF = pπ0 + pextr
N − pγ.
At this point the θcm can be recalculated and the value
obtained takes into account for the Fermi motion. In fig. 4,
we show the Fermi momentum distribution before and af-
ter the bidimensional cuts are applied.
Data collected with the green laser line and with the
UV laser line were analyzed separately and found com-
patible (at the level of 2 standard deviations at worst) in
the overlap region, where a weighted average of Σ was
performed. At the end of the event selection process, ap-
proximately 2.1·106
quasi-free neutron events and 6.9·106
quasi-free proton events were available for the extraction
of the beam asymmetry Σ(Eγ, θcm), and were grouped in
27 energy bins and 8 angular bins.
The main sources of systematic uncertainties affecting
the cross-section measurement (total photon flux, solid-
angle determination and deuterium density) cancel out
when the Σ beam asymmetry is calculated. The only rel-
evant contributions are related to the beam polarization
and the hadronic background (misidentified reaction chan-
nels). They were estimated to give rise, added in quadra-
ture, to a 3% total systematic uncertainty.
4 Results
4.1 Quasi-free proton
At the first step, the Σ beam asymmetry for the reaction
γ + p → p + π0
for the quasi-free proton was derived and
compared with the existing data collected at GRAAL on
a pure proton target [8]. The same energy binning was
used in order to achieve the best comparison of the two
independent data sets. The results are displayed in fig. 5.
We can see that there is an overall good agreement be-
tween the two independent data sets: the behavior of the
asymmetry as a function of the center-of-mass angle of
the neutral pion is the same for the free proton and for
the quasi-free proton. There are only small differences at
some energies, that can be ascribed to a smearing of the
asymmetry value due to the Fermi motion. A similar ef-
fect was observed recently also in the beam asymmetry
for η photoproduction [15]. Since the bound proton, ade-
quately treated in the quasi-free kinematical regime, be-
haves similarly to the free proton when the beam asymme-
try is measured, we are confident that the measured beam
asymmetries for the π0
photoproduction on the quasi-free
neutron are very similar to the same observable measured
on a free neutron if a free-neutron target were to exist.
4.2 Quasi-free neutron
The values of the Σ beam asymmetry for the quasi-free
neutron are shown in fig. 6, where they are compared with
the predictions of the MAID2007 [16] (dashed lines) and
with the results of the modified MAID2007 version (solid
lines). The last one includes in the fit the results of our
measurement. The comparison with predictions of differ-
ent models [17] is not shown since they are similar to
MAID2007.
MAID2007 is a unitary isobar model which describes
pion photoproduction in terms of background processes
as Born terms and vector meson exchanges and nucleon
resonance excitations.
The background processes are well determined and the
couplings are fixed to the large database of pion photo-
production from protons. This is strictly valid only for
multipoles with isospin 3/2. However, the multipoles with
isospin 1/2 have independent contributions in the proton
and neutron channels. The last one can only be obtained
from data on pion photoproduction reactions from neu-
trons, included in the modified version of MAID2007.
As we can see from fig. 6, the main effects are at back-
ward angles and above 0.9 GeV of the incident photon
energy. The values of the asymmetry are positive at all
energies and angles, in contrast with the results obtained
for the free proton where a change in sign of the asym-
metry occurs around θπ0
cm ≈ 90◦
and for photon energies
between 0.95 and 1.35 GeV. The new version of the fit de-
scribes much better the behavior of the asymmetry: the
negative values predicted by the MAID2007 version are
absent from the modified MAID2007 result, and the over-
all behavior is reproduced.
R. Di Salvo et al.: Σ beam asymmetry in π0
photoproduction off the neutron 155
Fig. 5. The Σ beam asymmetry for the reaction γ + p → p + π0
. Open dots refers to the GRAAL results on free proton [8].
Full dots are the result of this work for proton bound in the deuteron target in the quasi-free kinematic. Only the statistical
uncertainty is shown.
Fig. 6. The Σ beam asymmetry for the reaction γ +n → n+π0
compared with the predictions of MAID2007 (dashed line) and
modified MAID2007 (full line). Where not visible, errors bars lie within the data point spots. Only the statistical uncertainty
is shown.
156 The European Physical Journal A
Fig. 7. MAID2007 [16] (dashed lines) and modified MAID2007
(solid lines) global solutions. Left side: imaginary part; right
side: real part. Upper part of the figure: nM
1/2
1− multipole, cen-
tral part: nE
1/2
1+ multipole, lower part: nE
1/2
0+ multipole (see
text).
In terms of multipoles, the impact of our new data
is clearly visible in fig. 7, where the modified MAID2007
solution is compared with the previous solution. The ef-
fect is particularly striking for the nM
1/2
1− multipole (up-
per plot of fig. 7): here is also the contribution of a sec-
ond P11-resonance with MR = 1.70 GeV, Γtot = 0.07 GeV,
single-pion branching ratio βπ = 0.1 and helicity ampli-
tude A1/2 = −0.076 GeV−1/2
. Note that the indication of
the existence of a state at W ≈ 1.70 GeV was also found
in the reaction γ + p → p + π0
(see fig. 15 in ref. [16]) as
well as in η photoproduction on the neutron [18,19].
The effect of including our data in the fit is also vis-
ible in the nE
1/2
1+ multipole (middle plot of fig. 7). To
have a good description of our data, the photo-couplings
for the P13(1720)-resonance were modified to be An
1/2 =
−0.003 GeV−1/2
and An
3/2 = −0.023 GeV−1/2
while the
original MAID2007 fit assumed An
3/2 = −0.031 GeV−1/2
.
Finally, for Eγ > 1 GeV, the beam asymmetry is also
sensitive to the background contributions from the nE
1/2
0+
and nE
1/2
1+ multipoles, which were also changed in the
modified MAID2007 solution.
In fig. 8, the beam asymmetry for both quasi-free
proton and quasi-free neutron are compared, together
with the modified MAID2007 results. Proton and neu-
tron asymmetries are very similar at small angles and
low energies, while they differ significantly at large angles.
Fig. 8. Σ beam asymmetry for the π0
photoproduction on the
quasi-free proton (full dots) and quasi-free neutron (open dots)
as a function of the photon energy at fixed π0
center-of-mass
angle, compared to the results of partial-wave analysis from
modified MAID2007 (full line: proton, dashed line: neutron).
Where not visible, errors bars lie within the data point spots.
A big discrepancy with the fit results is present around
Eγ = 0.9 GeV, corresponding to a total energy in the
center-of-mass system of ≈ 1.7 GeV where the proton
value is underestimated while the neutron value is over-
predicted. The solution to this problem deserves further
theoretical studies. From the experimental point of view,
the complete determination of the isospin dependence
in the beam asymmetry still requires the measurement
of Σ in the π−
p photoproduction off the neutron (i.e.
γ + n → p + π−
). The analysis of this reaction chan-
nel is underway at GRAAL [20] and the results will soon
be available for theoretical interpretation and for partial-
wave analysis.
5 Conclusions
The Σ beam asymmetry in the π0
photoproduction off the
nucleon bound in deuteron in the quasi-free kinematical
regime was measured between 0.7 and 1.5 GeV photon en-
ergy, covering the second and the third nucleon resonance
region. The results for the proton and for the quasi-free
proton were found to be very similar, justifying a posteri-
ori the participant-spectator approach. In the case of the
quasi-free neutron, the asymmetry was found to be posi-
tive at all energies and center-of-mass angles. A modified
R. Di Salvo et al.: Σ beam asymmetry in π0
photoproduction off the neutron 157
version of the MAID2007 model was able to reproduce the
data when a second P11-resonance with MR = 1.7 GeV
and Γtot = 0.07 GeV was added. Its effect is particularly
visible in the nM
1/2
1− multipole. Further theoretical inves-
tigations are required to fully clarify the contributions to
the transition amplitude in this energy region, and partic-
ularly around 1 GeV of the incident photon energy.
We wish to thank all the technical staff of the collaboration
teams, who gave their full support to the maintenance of the
apparatus and target. We are grateful to the ESRF as a host
institution for the stable operation of the electron beam and
to the members of the CRG support group for the technical
assistance that they provided to the GRAAL Collaboration.
References
1. M. Benmerrouche, N.C. Mukhopadhyay, J.F. Zhang, Phys.
Rev. D 51, 3237 (1995).
2. B. Saghai, F. Tabakin, Phys. Rev. C 55, 917 (1997).
3. D. Drechsel, O. Hanstein, S.S. Kamalov, L. Tiator, Nucl.
Phys. A 645, 145 (1999).
4. T. Feuster, U. Mosel, Phys. Rev. C 59, 460 (1999).
5. W.-T. Chiang, F. Tabakin, Phys. Rev. C 55, 2034 (1997).
6. R.A. Arndt, I.I. Strakowsky, R.L. Workman, Phys. Rev. C
53, 430 (1996).
7. B. Saghai, Z. Li, Eur. Phys. J. A 11, 217 (2001).
8. O. Bartalini et al., Eur. Phys. J. A 26, 399 (2005).
9. A.V. Anisovich et al., Eur. Phys. J. A 25, 427 (2005).
10. P. Levi Sandri et al., Nucl. Instrum. Methods A 370, 396
(1996).
11. O. Bartalini et al., Nucl. Instrum. Methods A 562, 85
(2006).
12. V. Kuznetsov et al., Nucl. Instrum. Methods A 487, 396
(2002).
13. http://wwwasd.web.cern.ch/wwwasd/geant/.
14. P. Corvisiero et al., Nucl. Instrum. Methods A 346, 441
(1994).
15. A. Fantini et al., Phys. Rev. C 78, 015203 (2008).
16. D. Drechsel, S.S. Kamalov, L. Tiator, Eur. Phys. J. A 34,
69 (2007); http://www.kph.uni-mainz.de/MAID/.
17. R.A. Arndt, I.I. Strakovsky, R.L. Workman, Int. J. Mod.
Phys. A 18, 449 (2003); http://gwdac.phys.gwu.edu/.
18. V. Kuznetsov et al., Phys. Lett. B 647, 23 (2007).
19. I. Jaegle et al., Phys. Rev. Lett. 100, 252002 (2008).
20. The GRAAL Collaboration, in preparation.

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36 Measurement of Σ beam asymmetry in π0 photoproduction off the neutron in the second and third resonances region - The European Physical Journal A, November 2009

  • 1. EPJ AHadrons and Nuclei your physics journal EPJ.org Eur. Phys. J. A 42, 151–157 (2009) DOI: 10.1140/epja/i2009-10870-x Measurement of Σ beam asymmetry in π0 pho- toproduction off the neutron in the second and third resonances region R. Di Salvo, A. Fantini, G. Mandaglio, F. Mammoliti, O. Bartalini, V. Bellini, J.P. Bocquet, L. Casano, A. D’angelo, J.P. Didelez, D. Franco, G. Gervino, F. Ghio, G. Giardina, B. Girolami, A. Giusa, M. Guidal, E. Hourany, R. Kunne, A. Lapik, P. Levi Sandri, A. Lleres, M. Manganaro, D. Moricciani, A.N. Mushkarenkov, V. Nedorezov, C. Randieri, D. Re- breyend, N. Rudnev, G. Russo, C. Schaerf, M.L. Sperduto, M.C. Sutera, A. Turinge, V. Vegna, A. Fix, S.S. Kamalov and L. Tiator
  • 2. DOI 10.1140/epja/i2009-10870-x Regular Article – Experimental Physics Eur. Phys. J. A 42, 151–157 (2009) THE EUROPEAN PHYSICAL JOURNAL A Measurement of Σ beam asymmetry in π0 photoproduction off the neutron in the second and third resonances region⋆ R. Di Salvo1 , A. Fantini1,10 , G. Mandaglio2,14 , F. Mammoliti2,11 , O. Bartalini3,10 , V. Bellini4,11 , J.P. Bocquet5 , L. Casano1 , A. D’angelo1,10 , J.P. Didelez6 , D. Franco1,10 , G. Gervino7,12 , F. Ghio8,13 , G. Giardina2,14 , B. Girolami8,13 , A. Giusa2,11 , M. Guidal6 , E. Hourany6† , R. Kunne6 , A. Lapik9 , P. Levi Sandri3,a , A. Lleres5 , M. Manganaro2,14 , D. Moricciani1 , A.N. Mushkarenkov9 , V. Nedorezov9 , C. Randieri3,11 , D. Rebreyend5 , N. Rudnev9 , G. Russo2,11 , C. Schaerf1,10 , M.L. Sperduto2,11 , M.C. Sutera2 , A. Turinge9 , V. Vegna1,10 , A. Fix15 , S.S. Kamalov16,17 , and L. Tiator16 1 INFN - Sezione di Roma “Tor Vergata”, via della Ricerca Scientifica 1, I-00133 Roma, Italy 2 INFN - Sezione di Catania, via Santa Sofia 64, I-95123 Catania, Italy 3 INFN - Laboratori Nazionali di Frascati, via Enrico Fermi 40, I-00044 Frascati, Italy 4 INFN - Laboratori Nazionali del Sud, via Santa Sofia 64, I-95123 Catania, Italy 5 LPSC, Universit´e Joseph Fourier Grenoble 1, CNRS/IN2P3, Institut National Polytechnique de Grenoble, 53 Avenue des Martyrs, 38026 Grenoble, France 6 IPNO, Universit´e de Paris-Sud 11, CNRS/IN2P3, 15 rue Georges Cl´emenceau, 91406 Orsay, France 7 INFN - Sezione di Torino, via P. Giuria, I-10125 Torino, Italy 8 INFN - Sezione di Roma, piazzale Aldo Moro 2, I-00185 Roma, Italy 9 Institute for Nuclear Research, 117312 Moscow, Russia 10 Dipartimento di Fisica, Universit`a di Roma “Tor Vergata”, via della Ricerca Scientifica 1, I-00133 Roma, Italy 11 Dipartimento di Fisica e Astronomia Universit`a di Catania, via Santa Sofia 64, I-95123 Catania, Italy 12 Universit`a di Torino, via P. Giuria, I-00125 Torino, Italy 13 Istituto Superiore di Sanit`a, viale Regina Elena 299, I-00161 Roma, Italy 14 Dipartimento di Fisica, Universit`a di Messina, salita Sperone 31, I-98166 Messina, Italy 15 Laboratory of Mathematical Physics, Tomsk Polytechnic University, 634050, Tomsk, Russia 16 Institut f¨ur Kernphysik, Johannes Gutenberg-Universit¨at Mainz, D-55099 Mainz, Germany 17 Laboratory of Theoretical Physics, JINR Dubna, 141980 Moscow region, Russia Received: 21 April 2009 / Revised: 27 August 2009 Published online: 4 October 2009 – c Societ`a Italiana di Fisica / Springer-Verlag 2009 Communicated by Z.-E. Meziani Abstract. The Σ beam asymmetry in the photoproduction of neutral pions from quasi-free nucleons in a deuteron target was measured for the first time between 0.60 and 1.50 GeV, with the GRAAL polarized and tagged photon beam. The asymmetry values from the quasi-free proton were found equal to the ones extracted from a pure proton target. The asymmetries from quasi-free proton and quasi-free neutron were found equal up to 0.82 GeV and substantially different at higher energies. The results are compared with recent partial-wave analyses. PACS. 13.60.Le Meson production – 13.88.+e Polarization in interactions and scattering – 25.20.Lj Pho- toproduction reactions 1 Introduction The availability over the last decade of high duty-cycle accelerators coupled with the use of large solid-angle de- tectors yielded a wealth of experimental information in ⋆ The authors of this work, except A. Fix, S.S. Kamalov and L. Tiator, belong to The GRAAL Collaboration. a e-mail: paolo.levisandri@lnf.infn.it † Deceased. the study of the photo- and electroproduction of mesons from the proton. The attempt is to extract, from pho- toproduction, the electromagnetic couplings and further- more the hadronic properties of the excited nucleon states that cannot be accessed via pion scattering, either because the resonances largely overlap, or because of a weak cou- pling to the single pion-nucleon channel. In hadronic reactions induced by real photons, the po- larization degrees of freedom play a crucial role, and offer
  • 3. 152 The European Physical Journal A a complementary approach to the baryon spectroscopy. Polarization observables arising from interference mecha- nisms, are highly sensitive to the details of the interaction revealing resonance properties that are difficult to extract from a cross-section measurement, where a single contri- bution often dominates [1–4]. The detailed description of the photon-nucleon inter- action requires a complete data set containing, at least, eight independent observables: the cross-section, the three single polarization observables (beam, target and recoil nucleon) and four, appropriately chosen, double polariza- tion observables [5]. The resonance properties can then be extracted from the photoproduction data via partial-wave analysis and multipole decomposition, in the framework of different approaches [3,6]. The comparison of the cal- culated observables with the experimental data becomes a strong constraint to the theoretical models [4,7], to deter- mine the role and the properties of the resonance included. The GRAAL Collaboration already provided a large amount of precise polarization and cross-section data for various meson photoproduction reactions on the proton. In particular, the Σ beam asymmetry and the differen- tial cross-section were measured for π0 photoproduction in the 0.55–1.50 GeV energy range [8], bringing essential constraints to the theoretical models and to partial-wave analysis, and allowing to determine, within the model of ref. [9] the spin of the new resonance N(2070) D15 in- troduced in order to fit the large data set (see fig. 18 of ref. [8]). In order to obtain complementary information, and towards a full multipole analysis including the isospin structure, data on meson photoproduction from the neu- tron are of the utmost importance. In sect. 2 we give a brief description of the experimen- tal set-up. In sect. 3 the data analysis procedure is dis- cussed, while in sect. 4 the Σ beam asymmetries on the proton bound in the deuterium nucleus are compared with those of the free proton; the asymmetries from the quasi- free neutron are presented and are compared with quasi- free proton results and with theoretical models. The effect of these data on the multipole expansion is discussed. The last section contains our conclusions. 2 Experimental set-up The GRAAL experiment is based on the use of a tagged and polarized photon beam obtained through the Comp- ton back-scattering of laser light off the 6.03 GeV electrons circulating in the ESRF storage ring. A full description of the beam characteristics can be found in ref. [8]. The cou- pling of the GRAAL beam with a large acceptance detec- tor covering 0.95·4π solid angle with cylindrical symmetry (Lagranγe) is the ideal tool in order to measure polariza- tion degrees of freedom, in particular Σ beam asymme- tries, with very small systematic errors. For the purposes of this paper it is important to remember that the detector is substantially divided into two parts: 1) a central part based on the BGO Rugby Ball calorime- ter that covers laboratory angles 25◦ < θlab < 155◦ . The calorimeter, coupled to a ∆E/∆x segmented scin- tillation counter (called Barrel) for particle identifica- tion, has an excellent energy resolution for photons [10] and a high detection efficiency (> 40% depending on the energy threshold) for neutrons [11]; 2) a forward part (θlab < 25◦ ) equipped with two plane wire chambers, two scintillator walls and a Forward Shower detector having a good neutron detection ef- ficiency (∼ 22%) with momentum determination via time-of-flight (T.O.F.) measurement (∼ 750 ps resolu- tion for neutrons) [12]. The GRAAL experiment took data with a 6 cm length deuterium target in six different periods from June 1999 until December 2005. Both the 514 nm green line (giving rise to a 0.55–1.10 GeV tagged photon beam) and the 333– 368 nm UV line (0.80–1.50 GeV tagged photons) from the Argon laser were used, with typical intensities of ∼ 106 γ/s. Data taking was triggered by the coincidence between a tagging signal (which determines the incident photon en- ergy with 0.016 GeV FWHM resolution) and the total en- ergy measured by the Rugby Ball, the latter being required to be greater than 0.18 GeV. This condition gave rise to a data acquisition rate ∼ 100 events/s and allowed to record neutral pion photoproduction events both from quasi-free neutrons and quasi-free protons. The beam polarization can easily be changed by rotating the laser polarization. During data taking the polarization was moved from verti- cal (V) to horizontal (H) approximately every 20 minutes, defining two orthogonal polarization states. About 10% of the beam time was devoted to collect data with the un- polarized beam (electron Bremsstrahlung on the residual vacuum of the synchrotron doughnut). 3 Data analysis Data on the neutral pion photoproduction from quasi-free protons and from quasi-free neutrons were simultaneously recorded and analysed in a similar way: two neutral sig- nals in the BGO Rugby Ball were required to produce the π0 invariant mass in the range 0.09–0.20 GeV/c2 (initial preliminary selection see fig. 1). Together with the two photons in the BGO, a proton or a neutron signal was required, either in the forward di- rection or in the BGO Rugby Ball. At forward angles, the proton was identified via ∆E vs. T.O.F. (both measured in the two scintillator wall) while a T.O.F. greater than 13.5 ns (measured in the Forward Shower) with no asso- ciated track in the other detectors was used to select the neutron. In the central region, the proton was identified from the E vs. ∆E (measured in the Rugby Ball and in the Barrel, respectively) whereas a low crystal multiplicity (less than five) was the selection criterion for the candi- date neutron. To select quasi-free kinematics (participant- spectator approach), events with any additional signal(s) were rejected. These events were then required to fulfill the two-body kinematics of the π0 N reaction, where N is the partici- pating nucleon. Bidimensional cuts were applied on the following quantities:
  • 4. R. Di Salvo et al.: Σ beam asymmetry in π0 photoproduction off the neutron 153 Fig. 1. Invariant mass of the two photons from π0 decay before (full line) and after (dashed line) the kinematical cuts, when the neutron is detected in the forward direction. The obtained resolution is typical of the Rugby Ball calorimeter. Fig. 2. (Colour on-line) The ∆θ vs. ∆φ distribution (see text for definitions of ∆θ and ∆φ). – ∆θ vs. ∆φ, where ∆θ = θN − θM is the polar angle difference between the measured and the theoretical angle required to fulfill the two-body kinematics cal- culated from Eγ, the measured energy Eπ0 m and the π0 production angle θπ0 . ∆φ is the difference (−180◦ ) of the measured azimuthal angles of π0 and N; – the ratio Eπ0 c /Eπ0 m vs. Mx, where Eπ0 c is the π0 energy calculated from the π0 and N measured angles, and Mx is the missing mass calculated from Eγ and Eπ0 m . In fig. 2 an example for a single Eγ energy bin of ∆θ vs. ∆φ distribution is shown, while the Eπ0 c /Eπ0 m vs. Mx distribution is displayed in fig. 3. These two distributions were fitted with bidimensional Gaussian functions: the mean values µ1, µ2 and the stan- dard deviations σ1 and σ2 of the generic variables v1 and v2 were thus obtained. If the two Gaussians are Fig. 3. (Colour on-line) The Eπ0 c /Eπ0 m vs. Mx distribution (see text for definitions of Eπ0 c , Eπ0 m and Mx). uncorrelated the cut applied to v1 and v2 is (v1 − µ1)2 σ2 1 + (v2 − µ2)2 σ2 2 < σ2 . If the two variables are correlated, the correlation pa- rameter C is extracted and the cut is defined as (v1 − µ1)2 σ2 1 + (v2 − µ2)2 σ2 2 − 2C (v1 − µ1)(v2 − µ2) σ1σ2 < σ2 . In the event selection a value σ = 3 was used and was determined by optimizing the signal/background ratio in a full Monte Carlo simulation including all competing channels, and based on the GEANT3 [13] package and a realistic event generator [14]. Since the backgrounds and the detector resolutions are a function of the energy of the incoming photon, the cuts are extracted and applied as a function of the energy bins. Once the events are selected, the beam asymmetry Σ(Eγ, θcm) is extracted from the ratio NV /kV NV /kV + NH/kH = 1 2 (1 + PΣ cos(2φ)), where NH, NV are the yields obtained with the two beam polarization states (horizontal and vertical), kH, kV are the corresponding beam intensities, P(Eγ) is the de- gree of linear polarization of the beam at a given energy, Σ(Eγ, θcm) is the asymmetry as a function of the incom- ing photon energy and of the polar angle of π0 in the center-of-mass system, and φ is the π0 azimuthal angle. For each bin of energy and θcm, the resulting φ distribu- tion was fitted and the asymmetry Σ(Eγ, θcm) extracted. A great care was used to determine θcm. The Fermi mo- tion of the nucleon in the deuteron target is not negligi- ble and the composition of the Fermi momentum with the momentum of the incident photon causes a rotation of the Lorentz boost axis off the direction of the beam. The eval- uation of the Fermi momentum pF from the momentum balance of the two-body kinematics pF = pπ0 + pN − pγ
  • 5. 154 The European Physical Journal A Fig. 4. The calculated neutron Fermi momentum distribution before (full line) and after (dashed line) the kinematical cuts. is affected in particular by the imprecise knowledge of the momentum of the nucleon. The π0 energy and π0 and the nucleon emission angles are the more suitable information to use. Assuming a small Fermi energy (few MeV) for the nucleon in the deuteron, one can write Eextr N = Eγ + MN − Eπ0 , pextr N = (Eextr N )2 − M2 N , where Eextr N and pextr N are the extracted energy and mo- mentum of the outgoing nucleon. The extracted momen- tum is then combined with the measured outgoing nucleon angles to determine the three Cartesian components. The Fermi momentum is then calculated as follows: pF = pπ0 + pextr N − pγ. At this point the θcm can be recalculated and the value obtained takes into account for the Fermi motion. In fig. 4, we show the Fermi momentum distribution before and af- ter the bidimensional cuts are applied. Data collected with the green laser line and with the UV laser line were analyzed separately and found com- patible (at the level of 2 standard deviations at worst) in the overlap region, where a weighted average of Σ was performed. At the end of the event selection process, ap- proximately 2.1·106 quasi-free neutron events and 6.9·106 quasi-free proton events were available for the extraction of the beam asymmetry Σ(Eγ, θcm), and were grouped in 27 energy bins and 8 angular bins. The main sources of systematic uncertainties affecting the cross-section measurement (total photon flux, solid- angle determination and deuterium density) cancel out when the Σ beam asymmetry is calculated. The only rel- evant contributions are related to the beam polarization and the hadronic background (misidentified reaction chan- nels). They were estimated to give rise, added in quadra- ture, to a 3% total systematic uncertainty. 4 Results 4.1 Quasi-free proton At the first step, the Σ beam asymmetry for the reaction γ + p → p + π0 for the quasi-free proton was derived and compared with the existing data collected at GRAAL on a pure proton target [8]. The same energy binning was used in order to achieve the best comparison of the two independent data sets. The results are displayed in fig. 5. We can see that there is an overall good agreement be- tween the two independent data sets: the behavior of the asymmetry as a function of the center-of-mass angle of the neutral pion is the same for the free proton and for the quasi-free proton. There are only small differences at some energies, that can be ascribed to a smearing of the asymmetry value due to the Fermi motion. A similar ef- fect was observed recently also in the beam asymmetry for η photoproduction [15]. Since the bound proton, ade- quately treated in the quasi-free kinematical regime, be- haves similarly to the free proton when the beam asymme- try is measured, we are confident that the measured beam asymmetries for the π0 photoproduction on the quasi-free neutron are very similar to the same observable measured on a free neutron if a free-neutron target were to exist. 4.2 Quasi-free neutron The values of the Σ beam asymmetry for the quasi-free neutron are shown in fig. 6, where they are compared with the predictions of the MAID2007 [16] (dashed lines) and with the results of the modified MAID2007 version (solid lines). The last one includes in the fit the results of our measurement. The comparison with predictions of differ- ent models [17] is not shown since they are similar to MAID2007. MAID2007 is a unitary isobar model which describes pion photoproduction in terms of background processes as Born terms and vector meson exchanges and nucleon resonance excitations. The background processes are well determined and the couplings are fixed to the large database of pion photo- production from protons. This is strictly valid only for multipoles with isospin 3/2. However, the multipoles with isospin 1/2 have independent contributions in the proton and neutron channels. The last one can only be obtained from data on pion photoproduction reactions from neu- trons, included in the modified version of MAID2007. As we can see from fig. 6, the main effects are at back- ward angles and above 0.9 GeV of the incident photon energy. The values of the asymmetry are positive at all energies and angles, in contrast with the results obtained for the free proton where a change in sign of the asym- metry occurs around θπ0 cm ≈ 90◦ and for photon energies between 0.95 and 1.35 GeV. The new version of the fit de- scribes much better the behavior of the asymmetry: the negative values predicted by the MAID2007 version are absent from the modified MAID2007 result, and the over- all behavior is reproduced.
  • 6. R. Di Salvo et al.: Σ beam asymmetry in π0 photoproduction off the neutron 155 Fig. 5. The Σ beam asymmetry for the reaction γ + p → p + π0 . Open dots refers to the GRAAL results on free proton [8]. Full dots are the result of this work for proton bound in the deuteron target in the quasi-free kinematic. Only the statistical uncertainty is shown. Fig. 6. The Σ beam asymmetry for the reaction γ +n → n+π0 compared with the predictions of MAID2007 (dashed line) and modified MAID2007 (full line). Where not visible, errors bars lie within the data point spots. Only the statistical uncertainty is shown.
  • 7. 156 The European Physical Journal A Fig. 7. MAID2007 [16] (dashed lines) and modified MAID2007 (solid lines) global solutions. Left side: imaginary part; right side: real part. Upper part of the figure: nM 1/2 1− multipole, cen- tral part: nE 1/2 1+ multipole, lower part: nE 1/2 0+ multipole (see text). In terms of multipoles, the impact of our new data is clearly visible in fig. 7, where the modified MAID2007 solution is compared with the previous solution. The ef- fect is particularly striking for the nM 1/2 1− multipole (up- per plot of fig. 7): here is also the contribution of a sec- ond P11-resonance with MR = 1.70 GeV, Γtot = 0.07 GeV, single-pion branching ratio βπ = 0.1 and helicity ampli- tude A1/2 = −0.076 GeV−1/2 . Note that the indication of the existence of a state at W ≈ 1.70 GeV was also found in the reaction γ + p → p + π0 (see fig. 15 in ref. [16]) as well as in η photoproduction on the neutron [18,19]. The effect of including our data in the fit is also vis- ible in the nE 1/2 1+ multipole (middle plot of fig. 7). To have a good description of our data, the photo-couplings for the P13(1720)-resonance were modified to be An 1/2 = −0.003 GeV−1/2 and An 3/2 = −0.023 GeV−1/2 while the original MAID2007 fit assumed An 3/2 = −0.031 GeV−1/2 . Finally, for Eγ > 1 GeV, the beam asymmetry is also sensitive to the background contributions from the nE 1/2 0+ and nE 1/2 1+ multipoles, which were also changed in the modified MAID2007 solution. In fig. 8, the beam asymmetry for both quasi-free proton and quasi-free neutron are compared, together with the modified MAID2007 results. Proton and neu- tron asymmetries are very similar at small angles and low energies, while they differ significantly at large angles. Fig. 8. Σ beam asymmetry for the π0 photoproduction on the quasi-free proton (full dots) and quasi-free neutron (open dots) as a function of the photon energy at fixed π0 center-of-mass angle, compared to the results of partial-wave analysis from modified MAID2007 (full line: proton, dashed line: neutron). Where not visible, errors bars lie within the data point spots. A big discrepancy with the fit results is present around Eγ = 0.9 GeV, corresponding to a total energy in the center-of-mass system of ≈ 1.7 GeV where the proton value is underestimated while the neutron value is over- predicted. The solution to this problem deserves further theoretical studies. From the experimental point of view, the complete determination of the isospin dependence in the beam asymmetry still requires the measurement of Σ in the π− p photoproduction off the neutron (i.e. γ + n → p + π− ). The analysis of this reaction chan- nel is underway at GRAAL [20] and the results will soon be available for theoretical interpretation and for partial- wave analysis. 5 Conclusions The Σ beam asymmetry in the π0 photoproduction off the nucleon bound in deuteron in the quasi-free kinematical regime was measured between 0.7 and 1.5 GeV photon en- ergy, covering the second and the third nucleon resonance region. The results for the proton and for the quasi-free proton were found to be very similar, justifying a posteri- ori the participant-spectator approach. In the case of the quasi-free neutron, the asymmetry was found to be posi- tive at all energies and center-of-mass angles. A modified
  • 8. R. Di Salvo et al.: Σ beam asymmetry in π0 photoproduction off the neutron 157 version of the MAID2007 model was able to reproduce the data when a second P11-resonance with MR = 1.7 GeV and Γtot = 0.07 GeV was added. Its effect is particularly visible in the nM 1/2 1− multipole. Further theoretical inves- tigations are required to fully clarify the contributions to the transition amplitude in this energy region, and partic- ularly around 1 GeV of the incident photon energy. We wish to thank all the technical staff of the collaboration teams, who gave their full support to the maintenance of the apparatus and target. We are grateful to the ESRF as a host institution for the stable operation of the electron beam and to the members of the CRG support group for the technical assistance that they provided to the GRAAL Collaboration. References 1. M. Benmerrouche, N.C. Mukhopadhyay, J.F. Zhang, Phys. Rev. D 51, 3237 (1995). 2. B. Saghai, F. Tabakin, Phys. Rev. C 55, 917 (1997). 3. D. Drechsel, O. Hanstein, S.S. Kamalov, L. Tiator, Nucl. Phys. A 645, 145 (1999). 4. T. Feuster, U. Mosel, Phys. Rev. C 59, 460 (1999). 5. W.-T. Chiang, F. Tabakin, Phys. Rev. C 55, 2034 (1997). 6. R.A. Arndt, I.I. Strakowsky, R.L. Workman, Phys. Rev. C 53, 430 (1996). 7. B. Saghai, Z. Li, Eur. Phys. J. A 11, 217 (2001). 8. O. Bartalini et al., Eur. Phys. J. A 26, 399 (2005). 9. A.V. Anisovich et al., Eur. Phys. J. A 25, 427 (2005). 10. P. Levi Sandri et al., Nucl. Instrum. Methods A 370, 396 (1996). 11. O. Bartalini et al., Nucl. Instrum. Methods A 562, 85 (2006). 12. V. Kuznetsov et al., Nucl. Instrum. Methods A 487, 396 (2002). 13. http://wwwasd.web.cern.ch/wwwasd/geant/. 14. P. Corvisiero et al., Nucl. Instrum. Methods A 346, 441 (1994). 15. A. Fantini et al., Phys. Rev. C 78, 015203 (2008). 16. D. Drechsel, S.S. Kamalov, L. Tiator, Eur. Phys. J. A 34, 69 (2007); http://www.kph.uni-mainz.de/MAID/. 17. R.A. Arndt, I.I. Strakovsky, R.L. Workman, Int. J. Mod. Phys. A 18, 449 (2003); http://gwdac.phys.gwu.edu/. 18. V. Kuznetsov et al., Phys. Lett. B 647, 23 (2007). 19. I. Jaegle et al., Phys. Rev. Lett. 100, 252002 (2008). 20. The GRAAL Collaboration, in preparation.