# Eta-meson production in the resonance energy region.
^{1}^{1}1Supported by Transregio SFB/TR16, project B.7

###### Abstract

We perform an updated coupled-channel analysis of eta-meson production including all recent photoproduction data on the proton. The dip observed in the differential cross sections at c.m. energies W=1.68 GeV is explained by destructive interference between the and states. The effect from is found to be small but still important to reproduce the correct shape of the differential cross section. For the scattering we suggest a reaction mechanism in terms of the , , and states. Our conclusion on the importance of the , , and resonances in the eta-production reactions is in line with our previous results. No strong indication for a narrow state with a width of 15 MeV and the mass of 1680 MeV is found in the analysis. scattering length is extracted and discussed.

###### pacs:

11.80.-m,13.75.Gx,14.20.Gk,13.30.Gk## I Introduction

The discovery of nucleon resonances in the first pion-nucleon scattering experiments provided first indications for a complicated intrinsic structure of the nucleon. With establishing the quark picture of hadrons and developments of the constituent quark models the interest in the study of the nucleon excitation spectra was renewed. The major question was the number of the excited states and their properties. This problem was attacked both experimentally and theoretically. On the theory side constituent quark (CQM) models, lattice QCD and Dyson-Schwinger approaches have been developed to describe and predict the nucleon resonance spectra (see e.g. Aznauryan:2009da () for a review). The main problem remains, however, a serious disagreement between the theoretical calculations and the experimentally observed baryon spectra. This concerns both the number and the properties of excited states.

On the experimental side pion-induced reactions have been studied to establish resonance spectra. However, due to difficulties in detecting neutral particles most experiments were limited to pion-nucleon elastic scattering with charged particles in the final state. Being the lightest non-strange particle next to the pion the -meson also becomes an interesting probe to study nucleon excitations. A few experiments have been made in the past to investigate -production. The first near-threshold measurements Jones:1966zza (); Richards:1970cy (); Bulos:1970zk () demonstrated that the reaction proceeds through a strong -wave resonance excitation which was later identified with . An extensive study of the reaction above W1.7 GeV has been made in Brown:1979ii (); Baker:1979aw (). Both differential cross section and asymmetry data have been obtained. However, due to possible problems with the energy-momentum calibration Clajus:1992dh () the use of these data might lead to wrong conclusions on the reaction mechanism. Note that these problems are present not only in the -measurements Brown:1979ii (); Baker:1979aw () but also in the charge-exchange data obtained in the same experiment.

Presently the development of the high-duty electron facilities (ELSA, JLAB, MAMI, SPring) offers new possibilities to study the -photoproduction both on the proton () and on the neutron (). The first measurement of the -photoproduction on the neutron reported an indication for a resonance-like structure in the reaction cross section at W=1.68 GeV Kuznetsov:2006 (); Kuznetsov:2006kt (). Independent experimental studies Jaegle:2008ux (); Jaegle:2011sw () confirmed the existence of this effect in the reaction. This phenomenon was predicted in Azimov:2005jj () as a signal from a narrow state - a possible non-strange partner of the pentaquark Diakonov:1997mm (). Another explanation has been suggested in Shklyar:2006xw () where the observed effect was described by the contributions from the or states. Due to the lack of knowledge of the and resonance couplings to a clean separation of the relative contributions from these states is difficult. The general conclusion made in Shklyar:2006xw () is that both states might be good candidates to explain the observed structure.

By fitting to the cross sections and beam asymmetry the Bonn-Gatchina group provided an explanation Anisovich:2008wd () for the second peak in terms of the state. Another contribution to the field has been made by the authors of Doring:2009qr (). There the peak in the cross section ratio was explained by a cusp effect from the and rescattering channel. All these studies have been done assuming scattering on a quasi-free nucleon. At the same time a realistic analysis of meson photoproduction on the quasi-free neutron should include the nucleon-nucleon and meson-nucleon correlations (FSI-effect) which were shown to be very important Tarasov:2011ec () and take into account corresponding experimental cuts applied by the extraction of the quasi-free neutron data from -scattering. The later issue might be crucial for the unambiguous identification of the narrow resonance contribution as discussed in MartinezTorres:2010zzb ().

If it is granted that the signal observed in the scattering Kuznetsov:2006 (); Kuznetsov:2006kt (); Jaegle:2008ux (); Jaegle:2011sw () is due to the narrow (exotic) state one may expect to observe a similar effect in other eta-production reactions at the same energies, e.g in gamma-proton scattering. The experimental investigations of the -production on the proton made by the CLAS, GRAAL, and CB-ELSA/TAPS collaborations Dugger:2002ft (); Crede:2009zzb (); Bartholomy:2007zz (); Bartalini:2007fg () have found an indication of the dip structure around W=1.68 GeV in the differential cross section but not a resonance-like structure. This effect was also accompanied by the change in the angular distribution of the differential cross section. However, despite of extensive theoretical studies of the -production the reaction mechanism is still under discussion PhysRevC.84.045207 (); Chiang:2002vq (); Bartholomy:2007zz (); Feuster:1998b (); An:2011sb (); Anisovich:2011ka (); Shyam:2008fr (); Nakayama:2008tg (); Choi:2007gy (); Zhong:2007fx (); Fix:2007st (); Gasparyan:2003fp (); Ruic:2011wf ().

Recently the -photoproduction on the proton has been measured with high-precision by the Crystal Ball collaboration at MAMI McNicoll:2010qk (). These high-resolution data provides a new step forward in understanding the reaction dynamics and in the search for a signal from the ’weak’ resonance states. The main result reported in McNicoll:2010qk () is a very clean signal of a dip structure around W=1.68 GeV. It is interesting to note that the old measurements of the reaction Richards:1970cy () also give an indication for the second structure in the differential cross section at W=1.7 GeV. This raises a question whether the dip reported in the reaction, the resonance-like signal observed in and the possible structure in the cross section are originating from the same degrees of freedom or not. The second question is whether one of these phenomena can be attributed to the signal from a narrow (exotic) resonance state as discussed in Azimov2 (); Azimov:2005jj (); Azimov:2005hv ().

In our previous coupled-channel PWA study Shklyar:2006xw () we proposed an explanation of the possible dip in the -proton cross section in terms of the destructive interference of the and states. The result was based on the photoproduction data taken before 2006 Dugger:2002ft (); Crede:2003ax (). The aim of the present study is to extend our previous coupled-channel analysis of the reaction by including the data from the high-precision measurements McNicoll:2010qk (). The main question is whether the reaction dynamics can be understood in terms of the established resonance states. We emphasize that for reliable identification of the resonance contributions the calculations should maintain unitarity. Another complication comes from the fact that the most contributions to the resonance self-energy (total decay width) is driven by its hadronic couplings. Therefore the analysis of the photoproduction data requires the knowledge of the hadronic transition amplitudes. Hence the simultaneous analysis of all open channels (both hadronic and electromagnetic ) is inevitable for the identification of the resonances and extraction of their properties. In the present study we concentrate on the combined description of the scattering taking also the , , , channels into account. The results on the reaction will be reported elsewhere.

First, we corroborate our previous findings Penner:2002a (); Penner:2002b (); Shklyar:2006xw () where the important contributions from the , and resonances to the reaction have been found. The major effect comes from the and partial waves. The interference between the and states produces a dip in the amplitude. The amplitude is influenced by the contributions from the state. The interference between the and partial waves leads to the forward peak in the differential cross section around W=1.7 GeV. We stress that the interference between two nearby states also includes rescattering and coupled-channel effects which are hard to simulate by the simple sum of two Breit-Wigner forms.

We also confirm our previous finding that the interference between and is responsible for the dip seen in the data. The effect from the threshold is found to be relatively small which is also in line with the conclusion of Shklyar:2006xw (). Opposite to Anisovich:2011ka () we do not find any strong indications for a narrow state in the Crystal Ball/Taps data around W=1.68 GeV. We have also checked our results for the reaction above W=2 GeV where a number of new experimental data are available. Note that we do not use Reggezied channel exchange but include all -channel contributions consistently into our unitarization procedure. Because of the normalization problem Sibirtsev:2010yj (); Dey:2011rh () between the CLAS Williams:2009yj () and the CB-ELSA Crede:2009zzb () datasets the simultaneous description of these data is not possible. Above W=2 GeV our calculations are found to be in closer agreement with the CLAS measurements Williams:2009yj (). The CB-ELSA data Crede:2009zzb () demonstrates a step rise around W=1.925 GeV for the scattering angles . It is not clear whether this phenomenon could be related to a threshold effect (e.g. , , , or ) or attributed to other reaction mechanisms.

We conclude that further progress in understanding of the -meson production dynamics would be hardly possible without new measurements of the reaction.

## Ii Database

Here we present a short overview of the experimental database relevant for the present calculations. The details on the , , channels will be given elsewhere.

: The thorough overview of the experimental data (except the recently published Crystal Ball measurements Prakhov ()), is given in Clajus:1992dh (). As already mentioned in Introduction only few measurements of the -production have been made with pion beams: except for Danburg:1971 () where the eta-meson was produced in collisions, all the data have been taken from the scattering Prakhov (); Baker:1979aw (); Brown:1979ii (); Bulos:1970zk (); Richards:1970cy (); Jones:1966zza (); Debenham (); Deinet:1969cd (). Unfortunately due to numerous problems with the experimental data from Baker:1979aw (); Brown:1979ii () (see discussion in Clajus:1992dh () and references therein) the use of these measurements in the analysis might lead to wrong conclusions for the reaction mechanism. Therefore, opposite to Shrestha:2012va () we do not include these data in the analysis. Another measurement available above W=1.65 GeV is the data from Richards et al Richards:1970cy (). In the first resonance energy region this cross section tends to be lower than results from other experiments. Since the old measurements quote only statistical uncertainties the reason for these differences is unclear. In their study the authors of Batinic:1995 () added systematical errors to all differential cross sections. We do not follow this procedure and include only quoted uncertainties in the analysis.

: a number of experimental studies have been performed in the resonance energy region McNicoll:2010qk (); Williams:2009yj (); GRAAL:2002 (); Dugger:2002ft (); Krusche:1995nv (); Bartalini:2007fg (); Nakabayashi:2006ut (); Crede:2009zzb (); Crede:2003ax (); Bartholomy:2007zz (); Elsner:2007hm (); Bock:1998rk (); Ajaka:1998zi (). Most of these measurement are differential cross sections. The target asymmetry has been studied in Bock:1998rk (). It has been observed that close to the production threshold the asymmetry changes the sign at moderate scattering angles. The previous calculations of the Giessen Model Penner:2002a (); Shklyar:2006xw () and the Mainz group PhysRevC.60.035210 () could not explain this feature. The description of this data would require an unexpected phase shift between the and resonances as noted in PhysRevC.60.035210 (). One may hope that the upcoming new measurements of the target asymmetry at the ELSA facility will solve this puzzle Hartmann:2011uv ().

For the beam asymmetry we use the recent data from the GRAAL Bartalini:2007fg () and CB-ELSA/TAPS Elsner:2007hm () collaborations which cover the energy region up to W=1.91 GeV. For the differential cross section we use the recent high-quality Crystal Ball data McNicoll:2010qk (). Above W=1.89 GeV our calculations are constrained by the amalgamated data set from experiments Williams:2009yj (); Crede:2009zzb (); Crede:2003ax (); Bartholomy:2007zz (). Since the experimental uncertainties of the data Williams:2009yj (); Crede:2009zzb (); Crede:2003ax (); Bartholomy:2007zz () are much larger than those in McNicoll:2010qk () we reduce them by factor of 2.

In the channels our calculations are constrained by the single-energy solutions from the GWU (former SAID) analysis Workman:2011vb (); Arndt:2006bf (); Arndt:2008zz (). For the transitions we follow the procedure described in Penner:2002a (); Penner:2002b (); Feuster:1998a (); Feuster:1998b (). We continue to parameterize the channel in terms of the effective state, where is an isovector scalar meson of two pion mass: . The final state is only allowed to couple to nucleon resonances. Therefore the decay stands for the sum of transitions , , etc. This procedure allows for the good description of the partial wave cross sections extracted in Manley:1984 (). However of case of the the same agreement cannot be expected. This is because of the enhanced role of the background contributions (due to e.g. the contact interaction in the transitions). After fixing the database a minimization is performed to fix the model parameters.

## Iii Giessen Model

Here we briefly outline the main ingredients of the model. More details can be found in Feuster:1998a (); Feuster:1998b (); Penner:2002a (); Penner:2002b (); shklyar:2004a (); shklyar:2005c (). The Bethe-Salpeter equation is solved in the -matrix approximation to obtain multi-channel scattering -matrix:

(1) |

where () and () are the incoming and outgoing baryon (meson) four-momenta, is a coupled-channel scattering amplitude, is a meson-nucleon propagator and is an interaction kernel. The quantities , , and are in fact multidimensional matrices where the elements of the matrix stand for the different scattering reactions.

To solve the coupled-channel scattering problem with a large number of inelastic channels, we apply the so-called K-matrix approximation by neglecting the real part of the BSE propagator . After the integration over the relative energy, Eq. (1) reduces to

(2) |

where is a scattering matrix and () stands for the quantum numbers of initial(final) states , , , , , , . Using the partial-wave decomposition of , in terms of Wigner d-functions the angular integration can be easily carried out and the equation is further simplified to the algebraic form

(3) |

The validity of this approximation was demonstrated by Pearce and Jennings in Pearce:1990uj () by studying different approximations to the BSE for scattering. Considering different BSE propagators they concluded that an important feature of the reduced intermediate two particle propagator is the on-shell part of . It has been argued that there is no much difference between physical parameters obtained using the -matrix approximation and other schemes. It has also been shown in Goudsmit:1993cp (); Oset:1997it () that for and scattering the main effect from the off-shell part is a renormalization of the couplings and the masses.

Due to the smallness of the electromagnetic coupling the dominant contributions to the self energy stem from the hadronic part. Therefore we treat the photoproduction reactions perturbatively. This is equivalent to neglecting in the sum over intermediate states in Eq. (2). Thus, for a photoproduction process the equation (3) can be rewritten as follows Penner:2002b (); Feuster:1998b ()

(4) |

where the summation in Eq.(4) is done over all hadronic intermediate states. Here the matrix stems only from the hadronic transitions: indices and run over , , , , , channels. The sum in Eq. (4) reflects the importance of the hadronic part of the transition amplitude in the description of photoproduction reactions. In other words, the amplitudes for the , , etc. transitions should always be included in the calculation of the photoproduction amplitudes.

### iii.1 Interaction kernel and resonance parameters

Here we present the main ingredients of the interaction kernel to the BSE Eq.(1) relevant for -production. More details on other reactions can be found in shklyar:2004a (); Penner:2002a (); Penner:2002b (); Feuster:1998a (); Feuster:1998b (); shklyar:2004b (). The interaction potential (-matrix) of the BSE is built up as a sum of -, -, and -channel contributions corresponding to the tree level Feynman diagrams shown in Fig. (1).

In the isospin channel we checked for the contributions from the , , , , , , , , , resonances. The resonance and background contributions are consistently generated from the same effective interaction. The Lagrangian densities are given in shklyar:2004a (); Penner:2002a (); Penner:2002b (); Feuster:1998a (); Feuster:1998b (); shklyar:2004b () and respect the chiral symmetry in low-energy regime. The properties of the -channel mesons important for production are given in Table 1.

mass [GeV] | final state | |||
---|---|---|---|---|

0.783 | ||||

0.769 | ||||

0.983 | ||||

1.02 |

Using the interaction Lagrangians and values of the corresponding meson decay widths taken from the PDG pdg () the following coupling constants are obtained:

(5) |

All other coupling constants were allowed to be varied during the fit. The obtained values are given in Table 2. For the interaction we use pseudoscalar coupling , which has been also utilized in our previous studies Feuster:1998b (); Feuster:1998a (); Penner:2002a (); Penner:2002b (); Shklyar:2006xw (). The derived constant is found to be small which is in line with our previous results Shklyar:2006xw (); Penner:2002b (). To check the dependence of our results on the choice of the interaction we have also performed calculations with the pseudovector coupling. However also in the latter case only a small coupling constant has been found.

Since the PDG gives only the upper limit for the decay branching ratio R we allowed this constant to be varied during fit. However due to lack of experimental constraints this coupling cannot be fully fixed in the present calculation. We find a small overall contribution from the -channel -meson exchange to the reaction. The coupling is calculated from using the relation

where is a deviation from the ideal - mixing angle. Taking from pdg () one gets for the ratio . Using this value a very small contribution from the - channel -meson exchange to the -photoproduction has been found.

12.85 | 0.133 | 4.98 | 2.18 | ||||

0.31 | -44.37 | 7.23 | -1.50 |

To take into account the finite size of mesons and baryons each vertex is dressed by a corresponding form factor:

(6) |

where is a c.m. four-momentum of an intermediate particle and is a cutoff parameter. The cutoffs in Eq. (6) are treated as free parameters being varied during the calculation. However, we keep the same cutoffs in all channels for a given resonance spin : etc., (). This significantly reduces the number of free parameters; i.e. for all spin- resonances there is only one cutoff for all decay channels. However for the photoproduction reactions we use different cutoffs at the - and -channel electromagnetic vertices. All values are given in Table 3. Except for the spin- states, the - and -channel cutoffs almost coincide.

[GeV] | [GeV] | [GeV] | [GeV] | [GeV] | [GeV] | [GeV] | [GeV] |
---|---|---|---|---|---|---|---|

0.952 | 3.0 | 0.97 | 1.13 | 1.69 (1.69) | 4.20 (2.9) | 1.17 (1.25) | 0.7 |

The use of vertex form factors requires special care for maintaining the current conservation when the Born contributions to photoproduction reactions are considered. Since the resonance and intermediate meson vertices are constructed from gauge invariant Lagrangians they can be independently multiplied by the corresponding form factors. For the nucleon contributions to meson photoproduction we apply the suggestion of Davidson and Workman Davidson:2001rk () and use the crossing symmetric common form factor:

(7) |

The extracted resonance parameters given in Table 4 are very close to the values deduced in our previous calculations shklyar:2004b (); Shklyar:2006xw () which indicates the stability of the obtained solution. However some values changed upon inclusion of the new MAMI data McNicoll:2010qk (). The total width of tends to be larger than that deduced in our previous calculations shklyar:2004b (). The helicity amplitude is also modified but still is in good agreement with the parameter range provided by PDG pdg (). The opposite effect is found for the state where the total width is reduced once the data of McNicoll:2010qk () are included. The remaining resonance parameters are only slightly modified as compared to our previous results.

The mass and width of the Roper resonance is found to be larger than deduced in other analyses pdg (). However the authors of Vrana:2000 () give MeV for the total width. The large decay width MeV has also been deduced by Cutkosky and Wang Cutkosky:1990 (). Note that properties of this state are strongly influenced by its decay into the final state. Arndt et al Arndt:1990bp () found a second pole structure for the Roper resonance which might be attributed to the coupling to the subchannel. Since we use a simplified prescription for the reaction this effect cannot be properly described in the present calculations.

The recent GWU(SAID) study of the data shows no evidence for the resonance. An indirect indication for the existence of this state can be concluded from the analysis of the inelasticity and cross section in the partial wave, see discussion in Section IV. We find a small coupling of this resonance to the final state. Since a clear signal from this state is not seen in the recent GWU solution, the determination of the total width turns out to be difficult. In our calculations we assume that this resonance has a large decay branching ratio to the . However the quality of the data does not allow for an unambiguous determination of the properties of this state.

The mass and width of the is more close to the values obtained by Arndt et al Arndt:1995ak (): MeV and MeV respectively. It is interesting to note that the mass of this resonance deduced from the pion photoproduction tends to be 10 MeV lower that the values derived from the pion-induced reactions pdg (). The second has a very large decay width. We associate this state with as suggested in PDG. This resonance is rated with two stars and its existence is still under discussion. In our updated coupled-channel calculation of the -production shklyar:2004b () a large and decay branching ratios have been obtained.

The properties of other resonances are very close to the values given in PDG. Except for and we find only small resonance couplings to which is in accordance with our previous conclusions. One needs to stress that the smallness of the resonance coupling does not necessarily mean that the contribution from the state is negligible. The state produces for example a sizable effect in the eta-production due to overlapping with . Another example is the effect from the state in -photoproduction on the proton. Here the smallness of the branching ratio is compensated by the strong electromagnetic coupling of this resonance. Therefore the effect from this state could be seen in the and multipoles, see Section IV.5. However in most cases the resonance contributions with small branching ratios to the eta are hard to resolve unambiguously.

### iii.2 Pole parameters

It is interesting to compare the poles positions and elastic residues with the results from other studies, see Table 5. The calculated pole masses are very close to the values obtained in other analyses, see pdg (). The agreement between imaginary parts and elastics residues is also good, though some differences exist between the present values and the results from other groups.

For the state we obtain a smaller elastic residue (for definition of see pdg ()) MeV which is almost identical to the result of the GWU group =16 MeV Arndt:2006bf (). Both values seem to be out of the range given in PDG pdg () 5020 MeV. It is interesting to note that the elastic residue from Arndt:2006bf () is included into the estimation made in pdg () but still does not fit to the provided range. The value MeV for the state is also comparable with the result from Arndt:2006bf (): MeV which are again less than the lower bound given in pdg ().

Though the derived pole mass of is very close to the values deduced in other calculations we obtain a significantly larger pole width. As a result the elastic pole residue turns out to be also large =126 MeV. We note, that the extraction of the properties of in the complex energy plane might require a proper treatment of the isobar decay channel where the overlap of the self-energies of the and states might be important for the determination of the properties of . This question will be addressed in shklyar:2012 ().

As we already mentioned the results for are controversial. We find 159 MeV for the pole width. Somewhat greater value of 189 MeV has been obtained in Tiator:2010rp (); Batinic:2010zz (). The recent issue of PDG pdg () summarizes results for the pole parameters taken from four different analyses. Whereas the calculations Anisovich:2011fc (); Hoehler:1993 () give 200 MeV for the pole width, Cutkosky obtains a significantly lower value =80 MeV Cutkosky:1990zh (); Cutkosky:1979fy (). This results in a large spread of the resonance width given by PDG, see Table 5. The elastic residue is found to be small which is in accordance with the small decay branching ratio to . The similar conclusion has also been drawn in Tiator:2010rp ().

Investigation of the - wave inelasticity Arndt:2006bf () shows that the state could have a strong decay flux into the channel Manley:1984 (). Therefore the calculation of its pole width might be affected by deficiencies in description of this channel. PDG estimations are based on several studies where by Cutkosky Cutkosky:1979fy () is the lower limit. The upper bound MeV is given by the recent Bonn-Gatchina analysis Anisovich:2011fc (). Neither of these calculations includes the channel explicitely.

The situation with the second state is even more complicated. This resonance is rated by two stars in PDG and supposed to be rather broad. The latest GWU analysis Arndt:2006bf () does not find any indication for this state. The present information about the pole parameters in PDG is based solely on the result of the Bonn-Gatchina calculations Anisovich:2011fc () which deduce the pole mass MeV and the pole width MeV. These values are very close to those derived in the present work.

The pole width of the state ( 94 MeV) turns out to be 10 MeV less than the lower limit given in PDGpdg (). The similar value of 95 MeV has also been obtained in the Jülich model Doring:2009yv (). Some analyses find additional poles associated with the and states pdg (). We do not find any indication for . The pole position for the second resonance is close to the results of other calculation pdg ().

Though the elastic residues for the and states are comparable with the values given in PDG their pole widths are somewhat lower than those obtained in other studies pdg (). We also find an indication for the second state N(2000) with the pole mass of 1900 MeV and the width of MeV, see Table 5. This resonance has a small coupling to the final state what is in agreement with results from other calculations.

mass (MeV) | R | R | R | R | ||||
---|---|---|---|---|---|---|---|---|

(1535) | 1526(2) | 131(12) | 35(3) | — | 91(4) | — | ||

1526 | 136 | 34.4 | — | 92 | — | |||

1536(10) | 150(25) | 45(10) | — | 90(30) | — | |||

(1650) | 1665(2) | 147(14) | 74(3) | — | 63(6) | — | ||

1664 | 131 | 72.4 | — | 57 | — | |||

1657(13) | 150(30) | 70(20) | — | 53(16) | — | |||

(1440) | 1515(15) | 605(90) | 56(2) | — | — | -85(3) | — | |

1517 | 608 | 56.0 | — | — | -84 | — | ||

1445(25) | 300(150) | 65(10) | — | — | -60(4) | — | ||

(1710) | 1737(17) | 368(120) | 2(2) | 3(2) | -50(1) | — | ||

1723 | 408 | 1.7 | 0.2 | -50 | — | |||

1710(30) | 150(100) | 13(7) | 13(2) | 24(10) | — | |||

(1720) | 1700(10) | 152(2) | 17(2) | — | -65(2) | 35(2) | ||

1700 | 152 | 17.1 | — | -65 | 35 | |||

1725(24) | 225(125) | 11(3) | — | 50(60) | -19(20) | |||

(1900) | 1998(3) | 359(10) | 25(1) | 10(3) | -8(1) | 0(1) | ||

1998 | 404 | 22.2 | 14.9 | -8 | 0 | |||

1900(-) | 250(-) | 10(-) | — | 39(-) | 26(15) | -65(30) | ||

(1520) | 1505(4) | 100(2) | 57(2) | — | -15(1) | 146(1) | ||

1505 | 100 | 56.6 | 1.2 | — | -13 | 145 | ||

1520(5) | 112(12) | 60(5) | 2.3 | — | -24(8) | 150(15) | ||

(1875) | 1934(10) | 857(100) | 11(1) | 20(5) | 11(1) | 26(1) | ||

1934 | 859 | 10.5 | 20.1 | 11 | 26 | |||

1875(45) | 220(100) | 12(10) | 21(7) | 18(10) | -9(5) | |||

(1675) | 1666(2) | 148(1) | 41(1) | — | 9(1) | 21(1) | ||

1666 | 148 | 41.1 | — | 9 | 20 | |||

1675(5) | 150(15) | 40(5) | — | 19(8) | 15(9) | |||

(1680) | 1676(2) | 115(1) | 68(1) | — | 3(1) | 116(1) | ||

1676 | 115 | 68.3 | — | 3 | 115 | |||

1685(5) | 130(10) | 67(3) | — | -15(6) | 132(13) | |||

(2000) | 1946(4) | 198(2) | 10(1) | 1(1) | 11(1) | 25(1) | ||

1946 | 198 | 9.9 | 0.4 | 10 | 25 | |||

2050(100) | 350(200) | 15(7) | — | — | — | 35(15) | 50(14) | |

Re (GeV) | -2Im (MeV) | R(MeV) | ||
---|---|---|---|---|

1.49 | 100 | 15 | -51 | |

1.49-1.53 | 90-250 | 30…70 | -1…-30 | |

1.65 | 89 | 19 | -46 | |

1.64-1.67 | 100-170 | 20-50 | -50…-80 | |

1.386 | 277 | 126 | -60 | |

1.35-1.38 | 160-220 | 40-52 | -75…-100 | |

1.67 | 159 | 11 | 9 | |

1.67-1.77 | 80-380 | 2-15 | -160…+190 | |

1.67 | 118 | 12 | -45 | |

1.66-1.69 | 150-400 | 7-23 | -90…-160 | |

1.91 | 173 | 10 | -64 | |

1.870-1.93 | 140-300 | 1-5 | 45…-25 | |

1.492 | 94 | 27 | -35 | |

1.505-1.515 | 105-120 | 32-38 | -5…-15 | |

1.81 | 98 | 3 | -76 | |

1.8-1.95 | 150-250 | 2-10 | 20…180 | |

1.64 | 108 | 20 | -49 | |

1.655-1.665 | 125-150 | 22-32 | -21…40 | |

1.66 | 98 | 33 | -32 | |

1.665-1.68 | 110-135 | 35-45 | 0…-30 | |

1.90 | 123 | 11 | -6 | |

1.92-2.15 | 380-580 | 20-115 | -60…-140 |

## Iv Results and discussion

The lack of the experimental data for the pion-induced reactions does not provide enough constraints on the resonance parameters. Also the discrepancy among various measurements (see Section (II)) does not allow for a consistent description of the data in a full kinematical region. While the contribution from the state is well established the reaction dynamics above W=1.6 GeV is still under discussion. One of the early Giessen coupled-channel calculations Penner:2002a (); Penner:2002b (); Shklyar:2006xw () found a destructive interference between and states. The second suggestion is a strong contribution from the -resonance excitation above W=1.68 GeV. This resonance was established in the early single-channel Karlsruhe-Helsinki and Carnegie Mellon-Berkeley analyses (see PDG pdg () and references therein). The independent study of the reactions by the Zagreb group Ceci:2006ra () provides an additional evidence for the existence of . The result of Ceci:2006ra () confirm the assumption made in Penner:2002a (); Penner:2002b () on the important contribution from this state to the -production. However the recent analysis from the GWU group Arndt:2006bf () finds no evidence for this state. The absence of a clear signal in the partial wave of the elastic scattering does not necessarily mean that this state does not exist. If the coupling to the final state is small, the effect from this state might not be seen in scattering. The evidence for the signal from the resonance has also been reported from the study of the reaction Ceci:2005vf (). On the other hand the result of the Bayestian analysis performed by the Gent group DeCruz:2012bv () demonstrates that is not needed to describe the photoproduction. An opposite conclusion was drawn by the Bonn-Gatchina group which finds decay branching ratio of % of this state to Anisovich:2011fc ().

Another indication for this state comes from the analysis of an inelastic flux in the partial wave. In Fig. (2) the total inelasticity from the GWU analysis vs. the total cross section extracted in Manley:1984 () is compared. The difference between the total inelasticity and the total cross section at W=1.7 GeV in the -wave can be attributed to the sum of inelastic channels like , , etc. We assume here that the observed difference is due to the production channel dominated by the state. As is assumed to be small this raises the question about the magnitude of the contribution in the reaction. However the situation in -production is different from the elastic scattering. Here the contribution from is proportional to the product , where is the coupling constant at the transition vertex. It follows that the contribution from the can be significant provided that is large enough. The interplay with background and coupled-channel rescattering would further increase this effect.

### iv.1

The results of our calculations are presented in Fig. (3) in comparison with the world data. The first peak at W=1.54 GeV is related to the well established resonance contribution.

Though the effect from the state is hardly visible in the differential cross section this state plays an important role leading to the destructive interference between and as it has been pointed out in our previous calculations Penner:2002a (); Penner:2002b ().

The second rise is due to the resonance. This state has a small branching ratio to the system but due to the large -coupling this resonance affects the production cross section at W=1.7 GeV. The coupled-channel effects and interference with other partial waves further enlarge the overall contribution from this state.

The total partial wave cross sections are shown in Fig. 4. The destructive interference between the and leads to the dip in the total -partial wave cross section around W=1.64 GeV (dotted line). The effect from the state is shown by the dashed line, Fig. 4. The contributions from other partial waves are found to be small. We also corroborate our previous results shklyar:2004a () where only minor contributions from spin resonance states were obtained. Both t-channel and meson exchange and channel graphs give small effects. The inclusion of the higher spin state into the calculations is still important to reproduce the correct shape of the cross section. This feature is also found in many other calculations, e.g.Penner:2002a (); Batinic:1995 (). It is interesting to note that importance of the resonance contribution has recently been found in Shrestha:2012va () which is in line with our previous results Shklyar:2006xw (); Penner:2002b ().

Since the main contributions in our calculations come mainly from the and partial waves it is interesting to trace back the interference effect between them. Neglecting the higher partial waves the differential cross section can be written in the form

(8) |

where is a scattering angle and only depends on the c.m. energy. Then the angular distribution should have a maximum (minimum) at forward angles depending on the relative phase between the nonvanishing and amplitudes. In our calculation the interference between and partial waves produces a peak at forward scattering angles and energies above W=1.67 GeV, see Fig. (3). As a result the signal from the resonance becomes more transparent for forward scattering. This is in line with the data of Richards et al Richards:1970cy () confirming our guess about the production mechanism. The inclusion of higher partial waves would modify Eq. (8). However these contributions are relatively small (see Fig.(4)) thus producing only minor deviations from the distribution Eq. (8).

Note, that due to numerous problems with the experimental data our calculations above W=1.6 GeV are only partly constrained by experiment. Indeed, once the data Baker:1979aw (); Brown:1979ii () are neglected there are only 30 datapoints from experiment Richards:1970cy (). This data has relatively large error bars and seems not to be fully consistent with other measurements Clajus:1992dh (). Therefore, the results for the differential cross section might be regarded as a prediction rather than an outcome of the fit. This demonstrates an urgent need for new measurements of the reactions above W=1.6 GeV. This would be a challenge for the the upcoming pion-beams experiment carried out by the HADES collaboration at GSI.

### iv.2 amplitude and scattering lengths

The result for the transition amplitude in the partial wave is presented in Fig. 5. Close to threshold the elastic scattering is completely determined by the contribution of the resonance. At higher energies the excitation of also becomes important. The interference between those two -states produces an excess structure in the imaginary part of the amplitude at W=1.65 GeV.

The rapid variation of the -amplitude close to threshold indicates that this energy dependence should be taken into account when the scattering length is calculated. Here we use the definition for the effective range expansion from PhysRevC.55.R2167 ():

(9) |

where is an elastic partial S-wave amplitude, and , and are scattering length, effective range, and effective volume respectively. The results are shown in Table 6 in comparison with values deduced from other coupled-channel calculations ( results published before 1997 are discussed in PhysRevC.55.R2167 () ). The obtained value of is very close to our previous results Penner:2002a (). The values for the real part deduced in Batinic:1996me () and PhysRevC.55.R2167 () are lower than in this work. The study Batinic:1996me () gives 1.550 GeV for the mass and 204 MeV for the width of the state which are somewhat greater than in the present calculation. This could be one of the reasons for the differences in .

In PhysRevC.55.R2167 () only the state is taken into account to calculate transition amplitudes to the channel. Since the parameters of in PhysRevC.55.R2167 () are close to the values obtained in the present study the observed difference in might be attributed to the different treatment of background contributions which have been assumed in PhysRevC.55.R2167 () to be energy-independent. The second piece of uncertainty is related to the quality of the world data of scattering. Hence, precise measurements of this reaction would provide an additional constraint on scattering length.

The non-vanishing imaginary part of is mostly driven by rescattering in the channel. Since the largest contributions to the scattering length are produced by the state the imaginary part of is strongly influenced by the decay branching ratio of this resonance to . Only a minor effect is found from the rescattering induced by background contributions and inelastic flux to the channel. Since the coupling is well fixed an agreement in between various model calculations can be expected provided that unitarity is maintained.

The obtained value of the scattering length should be taken with care when in-medium properties of the -meson are considered. As it has already been pointed out in PhysRevC.55.R2167 () the amplitude has a strong energy dependence - a feature which might affect the -potential. The second reason is that properties of the resonance might also be subjected to in-medium modifications Lehr:2003km (). Both effects should be taken into account when -meson properties in nuclei are studied.

Reference | (fm) | (fm) |
---|---|---|

present work | 0.990.08 + i0.250.06 | -1.980.1 - i0.430.15 |

Penner:2002a () | 0.99 + i0.34 | -2.08 - i0.81 |

Batinic:1996me () |
0.7340.026 + i0.269 | |

PhysRevC.55.R2167 () | 0.75 + i0.27 | -1.50.13 - i0.240.04 |

Lutz:2001 () | 0.43+ i0.21 |

### iv.3 below 1.89 GeV

The results of our calculation of the differential cross section in comparison with the recent Crystal Ball/MAMI measurements are shown in Fig. (6). Our calculations demonstrate a nice agreement with the experimental data in the whole kinematical region. The first peak is related to the resonance contribution. Similar to the reaction the and states interfere destructively producing a dip around W=1.68 GeV. Though the effect from the state is only minor, the contribution from this resonance produces a rapid change in the photoproduction multipole, see Section IV.5. The coherent sum of all partial waves leads to the more pronounced effect from the dip at forward angles. Note that the resonance contribution to the photoproduction reaction stems from two sources: the first is related to the direct electromagnetic excitation of the nucleon resonance and the second comes from rescattering e.g. , Eq. (4). At this stage the hadronic transition amplitudes e.g. become an important part of the production mechanism. The sum of these contributions in the wave turns out to be destructive which reduces the overall contribution from the state. We also corroborate our previous findings Shklyar:2006xw () where a small effect from the threshold was found.

We also do not find any strong indication for contributions from a hypothetic narrow state with a width of 15-20 MeV around W=1.68 GeV. It is natural to assume that the contribution from this state would induce a strong modification of the beam asymmetry for energies close to the mass of this state. This is because the beam asymmetry is less sensitive to the absolute magnitude of the various partial wave contributions but strongly affected by the relative phases between different partial waves. Thus even a small admixture of a contribution from a narrow state might result into a strong modification of the beam asymmetry in the energy region of W=1.68 GeV.

In Fig. (8) we show the calculation of the photon-beam asymmetry in comparison with the GRAAL measurements Bartalini:2007fg (). One can see that even close to the threshold where our calculations exhibit a dominant production mechanism (see Fig. (7) ) the beam asymmetry is nonvanishing for angles . This shows that this observable is very sensitive to very small contributions from higher partial waves. At W=1.68 GeV and forward angles the GRAAL measurements show a rapid change of the asymmetry behavior. We explain this effect by a destructive interference between the and resonances which induces the dip at W=1.68 GeV in the partial wave. The strong drop in the partial wave modifies the interference between and other partial waves and changes the asymmetry behavior. Note that the interference between and and the interference between different partial waves are of different nature. The overlapping of the and resonances does not simply mean a coherent sum of two independent contributions, but also includes rescattering (coupled-channel effects). Such interplay is hard to simulate by the simple sum of two Breit-Wigner forms since it does not take into account rescattering due to the coupled-channel treatment.

The GRAAL collaboration finds no evidence for a narrow state around W=1.68 GeV. We also find no strong need for the narrow resonance contribution to describe the asymmetry data. Taking contributions from the established states into account our results are in close agreement with the experimental data Bartalini:2007fg ().

### iv.4 above 1.89 GeV

Since the MAMI measurements are available up to W=1.89 GeV the calculations in the region W=1.89 …2.GeV are constrained by the combined data set constructed out of the recent CLAS and CB-ELSA/TAPS Williams:2009yj (); Crede:2009zzb () data. Due to some inconsistencies between these two experiments Dey:2011rh (); Sibirtsev:2010yj () we did not try to fit the data above W=2.GeV but instead extrapolate our calculation into the higher energies. In this region the -channel exchange starts to play a dominant role. One of the accepted prescriptions is to use a Reggeized -channel meson exchange as suggested in Chiang:2002vq (). We do not follow this procedure here but include all -channel exchanges into the interaction kernel. This allows for a consistent unitary treatment of resonance and background contributions. The calculated differential cross section is presented in Fig. (9) as a function of the scattering angle. Except for the energy bin W = 2.097 GeV our results are found to be in close agreement with the CLAS measurements. The major contribution to the differential cross section at forward angles comes from - and -meson exchanges. The effect from the -meson is small due to the weakness of the coupling as dictated by the OZI rule Okubo:1963fa (); Zweig:1964jf (); Iizuka:1966fk (). We also checked for the contributions from the Primakoff effect which is found to be negligible at these energies.

It is interesting to compare our calculations with the data Williams:2009yj (); Crede:2009zzb () at forward angles plotted as a function of the c.m. energy, see Fig. (10). The cusp due to the production threshold is clearly seen in our calculations around W=1.72 GeV. The quality of the data is still not good enough to unambiguously resolve the cusp induced by the threshold in the experimental data. Note, that the calculations are done assuming a stable -meson. Taking into account the final -width would smear out this effect. Since the threshold lies 45 MeV above the dip position ( W=1.68 GeV) we conclude that this effect cannot explain the dip in the differential cross section. This conclusion is opposite to that drawn in Anisovich:2011ka ().

The discrepancy between the CLAS Williams:2009yj () and CB-ELSA/TAPS data is better seen at whereas for the measurements are found to be in better agreement. One of the interesting features observed in the recent CB-ELSA data is a sudden rise of the differential cross section at W=1.92 GeV. The effect is more pronounced at and is absent at other scattering angles. This phenomena might be attributed to sidefeeding from of one of the inelastic channels (e.g. , , , or ). However the problem with normalization inconsistencies between the CLAS and CB-ELSA data should be solved first before any physical interpretation can be given.

### iv.5 eta-photoproduction multipoles

The extracted multipoles are presented in Fig. 11. The major contribution to the multipole comes from the resonance. The second plays an important role in the region W=1.6…1.7 GeV. We corroborate our previous results Shklyar:2006xw () where only a small effect from the spin- states has been found. A very small signal from the resonance is seen in the and amplitudes at W=1.68 GeV.

It is interesting to note that the effect of is clearly seen in the and though the overall contribution from this state turns out to be small. The multipole is affected by the Roper and resonances leading to the rapid change in both real and imaginary parts of the amplitude at W=1.7 GeV. In the region W=1.48…1.6 GeV both the imaginary and the real parts of all multipoles with are of the order of magnitude smaller than due to the strong dominant contribution from . However for higher energies the influence of amplitudes with becomes also important.

## V Conclusion

We have performed a coupled-channel analysis of pion- and photon-induced reactions including the recent eta-photoproduction data from the Crystal Ball/MAMI collaboration. In the region W=1.89…2.0 GeV our solution is constrained by the combined dataset built from the recent CLAS and CB-ELSA/TAPS measurements. The dip in the differential cross-sections at W=1.68 GeV reported in McNicoll:2010qk () is described in terms of an interference of the and states. We stress that such an interference also includes coupled-channel effects and rescattering which is hard to simulate by a simple sum of two Breit-Wigner contributions. The additional contribution at W=1.68 GeV comes from the multipole where the excitation of the leads to a rapid change of the real and imaginary parts of the amplitude. We conclude that the cusp due to the threshold seen at 1.72 GeV is not important for the explanation of the dip at W=1.68 GeV. However the quality of the data is still not sufficient to resolve the threshold effect completely.

Above W=1.9 GeV the -channel - and -exchanges start to play a dominant role in the calculations. The effect from the -meson exchange is less important because of the smallness of the coupling. We have also checked for the contribution from the Primakoff-effect which is found to be negligible. In the region W=1.9…2.2 GeV our calculations tend to be in closer agreement with the CLAS data.

It is interesting to note that above W=1.92 GeV the cross sections of the CB-ELSA/TAPS collaboration indicate a sudden rise from 0.2 b up to 0.3 b. The effect is observed only for scattering angles . This phenomenon might be attributed to sidefeeding from of one of the inelastic channels (e.g. , , , or ). However the origin of the normalization discrepancies between the CLAS and CB-ELSA/TAPS data should first be understood before any physical interpretation can be given.

In the reaction the main effect comes from three resonances , , and . Similar to eta-photoproduction on the proton the overlap of the and states produces a dip around W=1.68 GeV. For energies GeV the contribution from is found to be important. The above reaction mechanism for the reaction is in line with our early findings Shklyar:2006xw () where the resonance like-structure in -photoproduction at W=1.68 GeV on the neutron was explained by the excitations of the , and resonances.

We conclude that further progress in understanding of -meson production would be hardly possible without new measurements of the reaction. The experimental investigation of this reaction would help to establish the resonance contributions to the -photoproduction above GeV. Finally, the study of the -channel with pion beams would solve the question whether the observed phenomena in photoproduction have their counterparts in scattering.

## References

- (1) I. Aznauryan et al., (2009), nucl-th/0907.1901.
- (2) W. Jones, D. Binnie, A. Duane, J. Horsey, and D. Mason, Phys.Lett. 23, 597 (1966).
- (3) W. Richards et al., Phys.Rev. D1, 10 (1970).
- (4) F. Bulos et al., Phys.Rev. 187, 1827 (1969).
- (5) R. M. Brown et al., Nucl.Phys. B153, 89 (1979).
- (6) R. Baker et al., Nucl.Phys. B156, 93 (1979).
- (7) M. Clajus and B. Nefkens, PiN Newslett. 7, 76 (1992).
- (8) V. Kuznetsov et al., (2006), hep-ex/0601002.
- (9) GRAAL, V. Kuznetsov, Phys. Lett. B647, 23 (2007), hep-ex/0606065.
- (10) CBELSA Collaboration, TAPS Collaboration, I. Jaegle et al., Phys.Rev.Lett. 100, 252002 (2008).
- (11) I. Jaegle et al., Eur.Phys.J. A47, 89 (2011).
- (12) Y. I. Azimov, V. Kuznetsov, M. Polyakov, and I. Strakovsky, Eur.Phys.J. A25, 325 (2005), hep-ph/0506236.
- (13) D. Diakonov, V. Petrov, and M. V. Polyakov, Z.Phys. A359, 305 (1997), hep-ph/9703373.
- (14) V. Shklyar, H. Lenske, and U. Mosel, Phys.Lett. B650, 172 (2007), nucl-th/0611036.
- (15) A. Anisovich et al., Eur.Phys.J. A41, 13 (2009).
- (16) M. Döring and K. Nakayama, Phys.Lett. B683, 145 (2010).
- (17) V. Tarasov, W. Briscoe, H. Gao, A. Kudryavtsev, and I. Strakovsky, Phys.Rev. C84, 035203 (2011).
- (18) A. Martinez Torres and E. Oset, Phys.Rev.Lett. 105, 092001 (2010).
- (19) CLAS Collaboration, M. Dugger et al., Phys.Rev.Lett. 89, 222002 (2002).
- (20) CBELSA/TAPS Collaboration, V. Crede et al., Phys.Rev. C80, 055202 (2009).
- (21) CB-ELSA Collaboration, O. Bartholomy et al., Eur.Phys.J. A33, 133 (2007).
- (22) The GRAAL collaboration, O. Bartalini et al., Eur.Phys.J. A33, 169 (2007).
- (23) X.-H. Zhong and Q. Zhao, Phys. Rev. C 84, 045207 (2011).
- (24) W.-T. Chiang, S. N. Yang, L. Tiator, M. Vanderhaeghen, and D. Drechsel, Phys.Rev. C68, 045202 (2003), nucl-th/0212106, 24 pages, 15 figures, modified version to appear in Phys. Rev. C.
- (25) T. Feuster and U. Mosel, Phys. Rev. C59, 460 (1999), nucl-th/9803057.
- (26) C. An and B. Saghai, Phys.Rev. C84, 045204 (2011).
- (27) A. Anisovich et al., (2011), hep-ph/1108.3010.
- (28) R. Shyam and O. Scholten, Phys.Rev. C78, 065201 (2008).
- (29) K. Nakayama, Y. Oh, and H. Haberzettl, J.Korean Phys.Soc. 59, 224 (2011).
- (30) K.-S. Choi, S.-i. Nam, A. Hosaka, and H.-C. Kim, J.Phys.G G36, 015008 (2009).
- (31) X.-H. Zhong, Q. Zhao, J. He, and B. Saghai, Phys.Rev. C76, 065205 (2007).
- (32) A. Fix, L. Tiator, and M. Polyakov, Eur.Phys.J. A32, 311 (2007), nucl-th/0702034.
- (33) A. Gasparyan, J. Haidenbauer, C. Hanhart, and J. Speth, Phys.Rev. C68, 045207 (2003), nucl-th/0307072.
- (34) D. Ruic, M. Mai, and U.-G. Meissner, Phys.Lett. B704, 659 (2011), 1108.4825.
- (35) Crystal Ball at MAMI, E. F. McNicoll et al., Phys. Rev. C82, 035208 (2010).
- (36) R. A. Arndt, Y. I. Azimov, M. V. Polyakov, I. I. Strakovsky, and R. L. Workman, Phys. Rev. C 69, 035208 (2004).
- (37) Y. I. Azimov, R. Arndt, I. Strakovsky, R. Workman, and K. Goeke, Eur.Phys.J. A26, 79 (2005), hep-ph/0504022.
- (38) CB-ELSA Collaboration, V. Crede et al., Phys.Rev.Lett. 94, 012004 (2005), hep-ex/0311045.
- (39) G. Penner and U. Mosel, Phys. Rev. C66, 055211 (2002), nucl-th/0207066.
- (40) G. Penner and U. Mosel, Phys. Rev. C66, 055212 (2002), nucl-th/0207069.
- (41) A. Sibirtsev, J. Haidenbauer, S. Krewald, and U.-G. Meissner, Eur.Phys.J. A46, 359 (2010).
- (42) B. Dey and C. A. Meyer, (2011), arXiv:1106.0479 [hep-ph].
- (43) CLAS Collaboration, M. Williams et al., Phys.Rev. C80, 045213 (2009).
- (44) Crystal Ball Collaboration, S. Prakhov et al., Phys. Rev. C 72, 015203 (2005).
- (45) J. S. Danburg et al., Phys. Rev. D2, 2564 (1970).
- (46) N. C. Debenham et al., Phys. Rev. D 12, 2545 (1975).
- (47) W. Deinet et al., Nucl.Phys. B11, 495 (1969).
- (48) M. Shrestha and D. Manley, (2012), arXiv:1205.5294.
- (49) M. Batinic, I. Slaus, A. Svarc, and B. M. K. Nefkens, Phys. Rev. C51, 2310 (1995), nucl-th/9501011, Erratum-ibid. C57:1004,(1998).
- (50) GRAAL, F. Renard et al., Phys. Lett. B528, 215 (2002), hep-ex/0011098.
- (51) B. Krusche et al., Phys.Rev.Lett. 74, 3736 (1995).
- (52) T. Nakabayashi et al., Phys.Rev. C74, 035202 (2006).
- (53) CBELSA Collaboration, TAPS Collaboration, D. Elsner et al., Eur.Phys.J. A33, 147 (2007), nucl-ex/0702032.
- (54) A. Bock et al., Phys.Rev.Lett. 81, 534 (1998).
- (55) J. Ajaka et al., Phys.Rev.Lett. 81, 1797 (1998).
- (56) L. Tiator, D. Drechsel, G. Knöchlein, and C. Bennhold, Phys. Rev. C 60, 035210 (1999).
- (57) CBESLA/TAPS Collaboration, J. Hartmann, (2011), arXiv:1108.3459 [nucl-ex].
- (58) R. L. Workman, W. J. Briscoe, M. W. Paris, and I. I. Strakovsky, Phys.Rev. C85, 025201 (2012), 9 pages, 6 figures, 3 tables.
- (59) R. Arndt, W. Briscoe, I. Strakovsky, and R. Workman, Phys.Rev. C74, 045205 (2006), nucl-th/0605082.
- (60) R. Arndt, W. Briscoe, I. Strakovsky, and R. Workman, Eur.Phys.J. A35, 311 (2008).
- (61) T. Feuster and U. Mosel, Phys. Rev. C58, 457 (1998), nucl-th/9708051.
- (62) D. M. Manley, R. A. Arndt, Y. Goradia, and V. L. Teplitz, Phys. Rev. D30, 904 (1984).
- (63) V. Shklyar, G. Penner, and U. Mosel, Eur. Phys. J. A21, 445 (2004), nucl-th/0403064.
- (64) V. Shklyar, H. Lenske, and U. Mosel, Phys. Rev. C72, 015210 (2005), nucl-th/0505010.
- (65) B. C. Pearce and B. K. Jennings, Nucl. Phys. A528, 655 (1991).
- (66) P. F. A. Goudsmit, H. J. Leisi, E. Matsinos, B. L. Birbrair, and A. B. Gridnev, Nucl. Phys. A575, 673 (1994).
- (67) E. Oset and A. Ramos, Nucl. Phys. A635, 99 (1998), nucl-th/9711022.
- (68) V. Shklyar, H. Lenske, U. Mosel, and G. Penner, Phys. Rev. C71, 055206 (2005), nucl-th/0412029.
- (69) Particle Data Group, J. Beringer et al., Phys.Rev. D86, 010001 (2012).
- (70) R. M. Davidson and R. Workman, Phys. Rev. C63, 025210 (2001).
- (71) T. P. Vrana, S. A. Dytman, and T. S. H. Lee, Phys. Rept. 328, 181 (2000), nucl-th/9910012.
- (72) R. E. Cutkosky and S. Wang, Phys. Rev. D42, 235 (1990).
- (73) R. A. Arndt, Z.-J. Li, L. D. Roper, R. L. Workman, and J. M. Ford, Phys.Rev. D43, 2131 (1991).
- (74) R. Arndt, I. Strakovsky, and R. Workman, Phys.Rev. C53, 430 (1996), nucl-th/9509005.
- (75) V. Shklyar, H. Lenske, and U. Mosel, in preparation .
- (76) L. Tiator et al., Phys.Rev. C82, 055203 (2010), 1007.2126.
- (77) M. Batinic, S. Ceci, A. Svarc, and B. Zauner, Phys.Rev. C82, 038203 (2010).
- (78) A. Anisovich et al., Eur.Phys.J. A48, 15 (2012), 1112.4937.
- (79) G. Hoehler, PiN Newslett. 9, 1 (1993).
- (80) R. Cutkosky and S. Wang, Phys.Rev. D42, 235 (1990).
- (81) R. Cutkosky, C. Forsyth, R. Hendrick, and R. Kelly, Phys.Rev. D20, 2839 (1979).
- (82) M. Doring, C. Hanhart, F. Huang, S. Krewald, and U.-G. Meissner, Nucl.Phys. A829, 170 (2009), 0903.4337.
- (83) S. Ceci, A. Svarc, and B. Zauner, Phys.Rev.Lett. 97, 062002 (2006), hep-ph/0603144.
- (84) S. Ceci, A. Svarc, and B. Zauner, Few Body Syst. 39, 27 (2006), hep-ph/0512337.
- (85) L. De Cruz, J. Ryckebusch, T. Vrancx, and P. Vancraeyveld, Phys.Rev. C86, 015212 (2012), 1205.2195.
- (86) T. W. Morrison, Ph.D. Thesis, George Washington University, UMI-99-55477, 2000 (2000).
- (87) A. M. Green and S. Wycech, Phys. Rev. C 55, R2167 (1997).
- (88) M. Batinic et al., Phys.Scripta 58, 15 (1998).
- (89) J. Lehr, M. Post, and U. Mosel, Phys.Rev. C68, 044601 (2003), nucl-th/0306024.
- (90) M. F. M. Lutz, G. Wolf, and B. Friman, Nucl. Phys. A706, 431 (2002), nucl-th/0112052.
- (91) S. Okubo, Phys.Lett. 5, 165 (1963).
- (92) G. Zweig, (1964), Published in ’Developments in the Quark Theory of Hadrons’. Volume 1. Edited by D. Lichtenberg and S. Rosen. Nonantum, Mass., Hadronic Press, 1980. pp. 22-101.
- (93) J. Iizuka, Prog.Theor.Phys.Suppl. 37, 21 (1966).