Bled Workshops in Physics Vol. 13, No. 1 p. 55

Bled, Slovenia, July 1 - 8, 2012
Complete Experiments for Pion Photoproduction
Institut fur Kernphysik, Johannes Gutenberg-Universitat, D-55099 Mainz, Germany
Abstract. The possibilities of a model-independent partial wave analysis for pion, eta or kaon photoproduction are discussed in the context of 'complete experiments'. It is shown that the helicity amplitudes obtained from at least 8 polarization observables including beam, target and recoil polarization can not be used to analyze nucleon resonances. However, a truncated partial wave analysis, which requires only 5 observables will be possible with minimal model assumptions.
1	Introduction
Around the year 1970 people started to think about how to determine the four complex helicity amplitudes for pseudoscalar meson photoproduction from a complete set of experiments. In 1975 Barker, Donnachie and Storrow [1] published their classical paper on 'Complete Experiments'. After reconsiderations and careful studies of discrete ambiguities [2-4], in the 90s it became clear that such a model-independent amplitude analysis would require at least 8 polarization observables which have to be carefully chosen. There are plenty of possible combinations, but all of them would require a polarized beam and target and in addition also recoil polarization measurements. Technically this was not possible until very recently, when transverse polarized targets came into operation at Mainz, Bonn and JLab and furthermore recoil polarization measurements by nucleon rescattering has been shown to be doable. This was the start of new efforts in different groups in order to achieve the complete experimental information and a model-independent partial wave analysis [5-8].
2	Complete experiments
A complete experiment is a set of measurements which is sufficient to predict all other possible experiments, provided that the measurements are free of uncertainties. Therefore it is first of all an academic problem, which can be solved by mathematical algorithms. In practise, however, it will not work in the same way and either a very high statistical precision would be required, which is very unlikely, or further measurements of other polarization observables are necessary. Both problems, first the mathematical problem but also the problem for a physical experiment can be studied with the help of state-of-the-art models like MAID or partial wave analyses (PWA) like SAID. With high precision calculations the complete sets of observables can be checked and with pseudo-data, generated from models and PWA, real experiments can be simulated under realistic conditions.
L. Tiator
2.1 Coordinate Frames
Experiments with three types of polarization can be performed in meson photoproduction: photon beam polarization, polarization of the target nucleon and polarization of the recoil nucleon. Target polarization will be described in the frame {x,y,z}, see Fig. 1, with the z-axis pointing into the direction of the photon momentum k, the y-axis perpendicular to the reaction plane, y = k x ^/ sin 6, and the x-axis is given by X = y x Z. For recoil polarization, traditionally the frame {x',y ', z'} is used, with the z'-axis defined by the momentum vector of the outgoing meson ^, the y '-axis is the same as for target polarization and the x '-axis given by x' = y ' x z'.
The photon polarization can be linear or circular. For a linear photon polarization (PT = I ) in the reaction plane (X, Z), cp = 0. Perpendicular, in direction y, the polarization angle is cp = n/2. Finally, for right-handed circular polarization,
P© =+1.
N'(-q)
Fig. 1. Frames for polarization vectors in the CM.
The polarized differential cross section can be classified into three classes of double polarization experiments: polarized photons and polarized target (types (S, BT)
^ = (j0{l -PTIcos2<p + Px(-PTHsin2<p+PmF) dO
+Py(T - Pt P cos 2^) + Pz (Pt G sin 2^ - P©E)},	(1)
polarized photons and recoil polarization (types (S, BR)
= cr0{1 -PTIcos2<p + PX'(-PTCVsin2<p-PmCx0
dO
+Py' (P - PtT cos 2^) + Pz' (-PtOz' sin 2^ - P©Cz')}, (2) polarized target and recoil polarization (types (S, TR)
^ = ao{1+PyT + Py'P + PX'(PxTx'-PzLx0 + Py'PyI-l-PZ'(PxTZ'-l-PzLz0}. (3)
In these equations cr0 denotes the unpolarized differential cross section, I, T, P are single-spin asymmetries (S), E, F, G,H the beam-target asymmetries (BT),
0x', 0z', Cx', Cz' the beam-recoil asymmetries (BR) and Tx' ,Tz' ,Lx' ,Lz' the target-recoil asymmetries (TR). The polarization quantities are described in Fig. 1. The signs of the 16 polarization observables of Eq. (1,2,3) are in principle arbitrary, except for the cross section do, which is naturally positive. For the 15 asymmetries we use the sign convention of Barker et al. [1], which is also used by the MAID and SAID partial wave analysis groups. For other sign conventions, see Ref. [9].
2.2 Amplitude analysis
Pseudoscalar meson photoproduction has 8 spin degrees of freedom, and due to parity conservation it can be described by 4 complex amplitudes of 2 kinemat-ical variables. Possible sets of amplitudes are: Invariant amplitudes At, CGLN amplitudes Ft, helicity amplitudes Ht or transversity amplitudes bt. All of them are linearly related to each other and further combinations are possible. Most often in the literature the helicity basis was chosen and the 16 possible polarization observables can be expressed in bilinear products
4
ot(w,e) = ^ Y. «k,£ Hk(w,e)Ht(w,e),	(4)
k,«=1
where 01 is the unpolarized differential cross section d0 and all other observables are products of asymmetries with d0, for details see Table 1.
From a complete set of 8 measurements {0t(W, 6)} one can determine the moduli of the 4 amplitudes and 3 relative phases. But there is always an unknown overall phase, e.g. (W, 6), which can not be determined by additional measurements. This is, however, not a principal problem as with the principally undetermined phase of a quantum mechanical wave function. Already in 1963 Goldberger et al. [10] discussed a method using the idea of a Hanbury-Brown and Twiss experiment, and very recently in 2012, Ivanov [11] discussed another method using vortex beams to measure the phase of a scattering amplitude. Both methods, however, are highly impractical for a meson photoproduction experiment.
Therefore, the complete information is contained in a set of 4 reduced amplitudes,
Hi(W,6)= Ht(W,6) e-i*l(W'e)	(5)
of which H is a real function, the others are complex, resulting in a total of 7 real values for any given W and 6.
Figure 2 shows two of such amplitude analyses with a complete set of 8 observables and an overcomplete set of 10 observables. The data used for this analysis has been generated as pseudo-data from Monte-Carlo events according to the Maid2007 solution, see Sect. 3. The figure shows the real parts of two out of four reduced helicity amplitudes, ReH 1 and ReH4. While the solution with the complete set of 8 observables results in a rather bad description of the true amplitudes, the solution of the overcomplete set gives a satisfactory result.
Table 1. Spin observables for pseudoscalar meson photoproduction involving beam, target and recoil polarization in 4 groups, S, BT, BR, TR. A phase space factor q/k has been omitted in all expressions and the asymmetries are given by A = A/ao. In column 2 the observables are expressed in terms of the Walker helicity amplitudes [12] and in column 3 in sin 0 and x = cos 0 with the leading terms for an S, P wave truncation.
Spin Obs	Helicity Representation	Partial Wave Expansion	
oo	j(|Hi 2 + H2 2 + H3 2 + H4 2)		Ao + A^x + AJ x2 + • • •
t t P^	Re(Hi H4 — H2H3)		sin2 0(Aq + • • • )
	Im(Hi + H3H4) —Im(Hi H3 + H2H4)		sin 0( AJ + Ajx H----) sin 0( Aq + AJ'x H----)
é	—Im(Hi H4 + H2H3)		sin2 0( Aq + • • • )
A Ê	—Im(Hi H3 — H2H4) IÎ-IHtI2 +|H2|2-IH3I2 + IH4I2)		sin0(A^ + A^xH----) Ao + Afx + Af x2 + • • •
t	Re(HiH| + H3H4)		sin 0( Ao + A^x H----)
ol,	—Im(Hi Hj - H3H4)	sin	0(Ao^' +A^'x + A^'x2 + •••)
ó:,	Im(Hi HJ — H2H3)		sin2 0(A°z' + A°z'xH----)
cl,	—RefHiH^ +H2H4)	sin	0(A^' +A^'x + A2c-'x2 + ---)
Cl,	1(-|H1|2-|H2|2 + |H3|2 + |H4|2)	a cz' A0	„ c / -»c/9 -»c/î + A-, z x + A2 z x2 + A3 z x H----
t'	Re(Hi HJ + H2H3)		sin 0(AOV' + A^'xH----)
t'	Re(Hi H2 — H3H4)	sin0(A0Z' + A^'x + A^'x2 H----)	
o	—RefHiH^ — H2H4)	sin	0(Aq ' + A^'x + A^'x2 + •••)
O	Hi 2 — H2 2 — H3 2 + H4 2)	a Lz ao	+ A^z ' x + A2 z ' x2 + A3z ' x3 H----
2.3 Truncated partial wave analysis
Even with the help of unitarity in form of Watson's theorem, the angle-dependent phase (W, 6) cannot be provided. This has very strong consequences, namely a partial wave decomposition would lead to wrong partial waves, which would be useless for nucleon resonance analysis. It becomes obvious in the following schematic formula
f«(W)= 2
21 +1
H(W,e)ei*(W'0)Pi(cos0) dcos0,	(6)
where the desired partial wave f (W) cannot be obtained from the reduced helicity amplitudes H(W, 0) alone, as long as the angle dependent phase $(W, 0) is unknown.
Our main goal in the data analysis of photoproduction is the search for nucleon resonances and their properties. To better reach this goal, one can directly perform a partial wave analysis from the observables without going through the underlying helicity amplitudes. Such an analysis would be a truncated partial wave analysis (TPWA) with a minimal model dependence (i) from the truncation of the series at a maximal angular momentum £max and (ii) from an overall unknown phase as in the case of the amplitude analysis in the previous paragraph. However, in the TPWA the overall phase would be only a function of energy and with additional theoretical help it can be constrained without strong model as-
Fig. 2. Comparison of the reduced helicity amplitudes ReH 1 and ReH4 between a pseudodata analysis with a complete dataset of 8 observables: do, I, T, P, E, G, 0x', Cx' (left 2 panels) and with an overcomplete dataset of 10 observables with additional F, H (right 2 panels) for Yp ^ n0p at E = 320 MeV as a function of the c.m. angle 6. The solid red curves show the MAID2007 solutions. Amplitudes are in units of 10_3 /mn+.
sumptions. Such a concept was already discussed and applied for y, n in the 80s by Grushin [13] for a PWA in the region of the A(1232) resonance.
Formally, the truncated partial wave analysis can be performed in the following way. All observables can be expanded either in a Legendre series or in a cos 6 series
Oi(W,9) = £ sinai9 Y Aj.(W) cosk9,	(7)
k k=0
lmax	4
Ak (W)=	T_	(W) M¡'' (W),	(8)
1,1'=0 k,k' = 1
where k, k' denote the 4 possible electric and magnetic multipoles for each nN angular momentum I > 2, namely Ml>k = {El+, , Ml+, }. For an S,P truncation (lmax = 1) there are 4 complex multipoles E0+, E1 +, M1 +, M1_ leading to 7 free real parameters and an arbitrary phase, which can be put to zero for the beginning. In Table 1 we list the expansion coefficients for all observables that appear in an S, P wave expansion. Already from the 8 observables of the first two groups (S, BT) one can measure a set of 16 coefficients, from which we only need 8 well selected ones for a unique mathematical solution. This can be achieved by a measurement of the angular distributions of only 5 observables, e.g. d0,1, T, P, F or d0,1, T, F, G. In the first example one gets even 10 coefficients, from which e.g.
AP and AF can be omitted. In the second case, there are 9 coefficients, of which A0 can be omitted. In practise one can select those coefficients, which have the smallest statistical errors, and therefore, the biggest impact for the analysis by keeping in mind that all discrete ambiguities are resolved.
As has been shown by Omelaenko [14] the same is true for any PWA with truncation at lmax. For the determination of the 8£max — 1 free parameters one has the possibility to measure (8£max, 8£max, 8£max + 4, 8£max + 4) coefficients for types (S, BT, BR, TR), respectively.
3 Partial wave analysis with pseudo-data
In a first numerical attempt towards a model-independent partial wave analysis, a procedure similar to the second method, the TPWA, described above, has been applied [6], and pseudo-data, generated for y, n0 and y, have been analyzed.
Events were generated over an energy range from Elab = 200 — 1200 MeV and a full angular range of 6 = 0 — 180° for beam energy bins of AEY = 10 MeV and angular bins of A6 = 10°, based on the MAID2007 model predictions [15]. For each observable, typically 5 • 106 events have been generated over the full energy range. For each energy bin a single-energy (SE) analysis has been performed using the SAID PWA tools [16].
Fig. 3. Real and imaginary parts of (a) the Sn partial wave amplitude E0+2 and (b) the Pi 1 partial wave amplitude M1}-2. The solid (dashed) line shows the real (imaginary) part of the MAID2007 solution, used for the pseudo-data generation. Solid (open) circles display real (imaginary) single-energy fits (SE6p) to the following 6 observables without any recoil polarization measurement: da/dO, two single-spin observables Z, T and three beam-target double polarization observables E, F, G. Multipoles are in millifermi units.
A series of fits, SE4p, SE6p and SE8p have been performed [6] using 4,6 and 8
observables, respectively. Here the example using 6 observables (a0, Z, T, E, F, G)
is demonstrated, where no recoil polarization has been used. As explained before,
such an experiment would be incomplete in the sense of an 'amplitude analysis',
1 /2
but complete for a truncated partial wave analysis. In Fig. 3 two multipoles E0+ 1 /2
and M1- for the S11 and P11 channels are shown and the SE6p fits are compared to the MAID2007 solution. The fitted SE solutions are very close to the MAID
solution with very small uncertainties for the Si i partial wave. For the Pi i partial wave we obtain a larger statistical spread of the SE solutions. This is typical i /2
for the M^- multipole, which is generally much more difficult to obtain with good accuracy [15], because of the weaker sensitivity of the observables to this magnetic multipole. But also this multipole can be considerably improved in an analysis with 8 observables [6].
4 Summary and conclusions
It is shown that for an analysis of N* resonances, the amplitude analysis of a complete experiment is not very useful, because of an unknown energy and angle dependent phase that can not be determined by experiment and can not be provided by theory without a strong model dependence. However, the same measurements or even less will be very useful for a truncated partial wave analysis with minimal model dependence due to truncations and extrapolations of Watson's theorem in the inelastic energy region. A further big advantage of such a PWA is a different counting of the necessary polarization observables, resulting in very different sets of observables. While it is certainly helpful to have polarization observables from 3 or 4 different types, for a mathematical solution of the bilinear equations one can find minimal sets of only 5 observables from only 2 types, where either a polarized target or recoil polarization measurements can be completely avoided.
I would like to thank R. Workman, M. Ostrick and S. Schumann for their contributions to this ongoing work. I want to thank the Deutsche Forschungsgemeinschaft for the support by the Collaborative Research Center 1044.
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Bled Workshops in Physics Vol. 13, No. 1 p. 62

Bled, Slovenia, July 1 - 8, 2012
News from Belle: Recent Spectroscopy Results
M. Bracko*
University of Maribor, Smetanova ulica 17, SI-2000 Maribor, Slovenia and Jozef Stefan Institute, Jamova cesta 39, SI-1000 Ljubljana, Slovenia
Abstract. This paper reports on some of the latest spectroscopic measurements performed with the experimental data collected by the Belle spectrometer, which has been operating at the KEKB asymmetric-energy e+ e- collider in the KEK laboratory in Tsukuba, Japan.
1	Introduction
The Belle detector [1] at the asymmetric-energy e+ e- collider KEKB [2] has accumulated about 1 ab-1 of data by the end of its operation in June 2010. The KEKB collider, called a B-factory, most of the time operated near the Y(4S) resonance, but it has accumulated substantial data samples also at other Y resonances, like Y(1S), Y(2S) and Y(5S), as well as in the nearby continuum. In particular, the data samples at the Y(4S) and Y(5S) resonances are by far the largest available in the world, corresponding to integrated luminosities of 798 fb-1 and 123 fb-1, respectively. Large amount of collected experimental data and excellent detector performance enabled many interesting spectroscopic results, including discoveries of new hadronic states and studies of their properties. This report covers most recent and interesting spectroscopic measurements—performed with either charmonium(-like) and bottomonium(-like) states.
2	Bottomonium and Bottomonium-like States
The Belle collaboration used a data sample at the CM energy around the Y(5S) mass 10.89 GeV, and found large signals for decays into n-Y(1 S), n-Y(2S) and n+n-Y(3S) final states [3]. If these transitions are only from the Y(5S) resonance, then the corresponding partial widths are more than two orders of magnitude larger than the corresponding partial widths for Y(4S), Y(3S) and Y(2S) decays to n+n-Y(1S). These results motivate a search for the hb (mP) resonances in the Y(5S) data. hb (1P) and hb (2P) states are observed in the missing mass spectrum of n+n- pairs for the Y(5S) decays, with significances of 5.5ct and 11 .2ct, respectively [4]. This is the first observation of the hb(1P) and hb(2P) spin-singlet bottomonium states in the reaction e+ e- —» hb(mP)n+n- at the Y(5S) energy. Later hb (1P) and hb (2P) were studied in the Y(5S) —» hbn+n- —» ynb (1S)n+ n-
* Representing the Belle Collaboration.
Decay mode	Branching fraction in %
hb(lP) -> yrib(lS)	49.2±5.7^j
hb(2P) -> yrib(lS)	22.3±3.8l|;^
hb (2P) —> yr|b (2S)	47.5±10.5+f;S
Table 1. The branching fractions for hb ^ yr|b decays, as measured by Belle.
decay [5]. In the same final state, Belle observes [5] also the first evidence for a nb(2S) in Y(5S) —» hb(2P)n+ n— —» ynb(2S)n:+ n— decay. The width of nb(2S) is small, with r = (4±8) MeV. Branching fractions for observed radiative hb decays are summarized in Table 1.
Comparable rates of hb (1P) and hb (2P) production indicate a possible exotic process that violates heavy quark spin-flip and this motivates a further study of the resonant structure in Y(5S) —» hb(mP)n+n— and Y(5S) —» Y(nS)n+ n— decays [6]. Due to the limited statistics, only the study of M(hb (mP)n) distribution is possible for hb(mP)n+ n—, while in the case of Y(nS)n+n— decay modes the Dalitz plot analysis can be performed. As a result, two charged bottomonium-like resonances, Zb (10610) and Zb (10650), are observed with signals in five different decay channels, Y(nS)n± (n = 1,2,3) and hb(mP)n± (m = 1,2). The averaged values for the mass and widths of the two states are calculated to be: M(Zb(10610)) = (10607.2 ± 2.0) MeV, r(Zb(10610)) = (18.4 ± 2.4) MeV and M.(zb(10650)) = (10652.2 ± 1.5) MeV, r(Zb(10650)) = (11.5 ± 2.2) MeV. The measured masses are only a few MeV above the thresholds for the open beauty channels B*B (10604.6 MeV) and B*B* (10650.2 MeV) [9], which could indicate a molecular nature of the two observed states. Angular analysis of charged pion distributions favours the JP = 1 + spin-parity assignment for both Zb (10610) and Zb (10650).
3 Charmonium and Charmonium-like States
There has been a renewed interest in charmonium spectroscopy since 2002. The attention to this field was drawn by the discovery of the two missing cc states below the open-charm threshold,nc(2S) and hc(1P) [7,8] with JPC=0—+ and 1+ , respectively, but even with the discoveries of new new charmonium-like states (so called "XYZ" states).
3.1 The X(3872) news
The storyabout the so called "XYZ" states began in 2003, when Belle reported on B+ —} K+J/^n+ n— analysis, where a new state decaying to J/^n+n— was discovered [10]. The new state, called X(3872), was soon confirmed and also intensively studied by the CDF, D0 and BABAR collaborations [11-19]. So far it has been established that this narrow state (r = (3.0—1 '4 ± 0.9) MeV) has a mass of
(3872.2 ± 0.8) MeV, which is very close to the D°D*° threshold [9]. The intensive studies of several X(3872) production and decay modes suggest two possible JPC assignments, 1++ and 2 h, and establish the X(3872) as a candidate for a loosely bound D°D*° molecular state. However, results provided substantial evidence that the X(3872) state must contain a significant cc component as well.
Recently, Belle performed a study of B —> (ccy)K using the final data sample with 772 million of BB pairs collected at the T(4S) resonance [20]. Pure D°D*° molecular model [21] predicts B(X(3872) -> ^'y) to be less than B(X(3872) -> J/^y). Results by the BABAR collaboration [19] show that B(X(3872) -> ^'y) is almost three times that of B(X(3872) —> J/^y), which is inconsistent with the pure molecular model, and can be interpreted as a large cc — D°D*° admixture. We observe X(3872) —» J/^y together with an evidence for Xc2 —> J/^y in B± —> J/^yK± decays, while in our search for X(3872) —» ^'y no significant signal is found. We also observe B —> Xci K decays in both, charged as well as neutral B decays. The obtained results suggest that the cc-D°D*° admixture in X(3872) may not be as large as discussed above.
New results for the X(3872) ->J/^n+n- decay modes in B+—>K+X(3872) and B°^K° (^7t+7t~)X(3872) decays are obtained with the complete Belle data set of 772 million BB pairs collected at the T(4S) resonance [22], The results for the X(3872) mass and width are obtained by a 3-dimensional fit to distributions of the three variables: beam-constrained-mass Mbc= v^beSiJ2 — (p™8)2 (with the beam energy Ebmsm and the B-meson momentum pBms both measured in the centre-of-mass system), the invariant mass Minv(J/^n+n-) and the energy difference AE=EBms-Ebmfm (where EBms is the B-meson energy in the centre-of-mass system). As a first step, the fit is performed for the reference channel ^'—»J/^n+n-, and the resolution parameters are then fixed for the fit of the X(3872). The mass, determined by the fit, is (3871.84±0.27±0.19) MeV. Including the new Belle result, the updated world-average mass of the X(3872) is mx=(3871.67±0.17) MeV. If the X(3872) is an S-wave D*°D° molecular state, the binding energy Eb would be given by the mass difference m(X)-m(D*°)-m(D°). With the current value of m(D0)+m(D*°)=(3871.79 ± 0.30) MeV [9], a binding energy of Eb=(-0.12±0.35) MeV can be calculated, which is surprisingly small and would indicate a very large radius of the molecular state.
The best upper limit for the X(3872) width was 2.3 MeV (with 90% C.L.), obtained by previous Belle measurement [10]. The 3-dimensional fits are more sensitive to the natural width, which is smaller than the detector resolution (ct -4 MeV). Due to the fit sensitivity and the calibration performed on the reference channel ^'—»J/^n+n-, the updated upper limit for the X(3872) width is about 1/2 of the previous value: r(X(3872)) < 1.2 MeV at 90% C.L.
Previous studies performed by several experiments suggested two possible JPC assignments for the X(3872), 1++ and 2 h. In the recent Belle analysis [20], the X(3872) quantum numbers were also studied with the full available data sample collected at the Y(4S) resonance. At the current level of statistical sensitivity it is not possible to distinguish completely between the two possible quantum number assignments, so both hypotheses are still allowed. Possible C-odd neu-
tral partners of X(3872) are also searched, but no signal is found for this type of states.
4 Summary and Conclusions
Many new particles have already been discovered during the operation of the Belle experiment at the KEKB collider, and some of them are mentioned in this report. Some recent Belle results also indicate that analogs to exotic charmonium-like states can be found in bb systems. Although the operation of the experiment has finished, data analyses are still ongoing and therefore more interesting results on charmonium(-like) and bottomonium(-like) spectroscopy can still be expected from Belle in the near future.
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