application/xmlTwo new sum rules for octet-baryon magnetic moments (μ) and constraints on QCD sum rules from new experimental determination of μ-s for the decupletMonika SinhaAshik IqubalMira DeyJishnu DeyQCD sum rulesMagnetic moments of octet and decuplet baryonsMagnetic moment sum rulesPhysics Letters B 562 (2003) 63-67. doi:10.1016/S0370-2693(03)00545-8journalPhysics Letters BCopyright © unknown. Published by Elsevier B.V.Elsevier B.V.0370-26935621-25 June 20032003-06-0563-67636710.1016/S0370-2693(03)00545-8http://dx.doi.org/10.1016/S0370-2693(03)00545-8doi:10.1016/S0370-2693(03)00545-8http://vtw.elsevier.com/data/voc/oa/OpenAccessStatus#Full2014-01-01T00:14:32ZSCOAP3 - Sponsoring Consortium for Open Access Publishing in Particle Physicshttp://vtw.elsevier.com/data/voc/oa/SponsorType#FundingBodyhttp://creativecommons.org/licenses/by/3.0/JournalsS300.2PLB19786S0370-2693(03)00545-810.1016/S0370-2693(03)00545-8PhenomenologyTable 1The experimental values of magnetic moments in unit of μNpnΞΞ0Σ+ΣΩΔ+Δ++2.793−1.913−0.6507−1.252.458−1.162.0192.7−2.8+2.56.14±0.51Table 2The values of magnetic moments and sum rules in unit of μN for [16] and [15]. Note that the values of ΔSR should be zeropnΞΞ0Σ+ΣΔSR1ΔSR2ΔCGRef.2.744−1.955−0.598−1.2782.461−1.0690.8300.6750.489[16]2.800−1.990−0.560−1.2401.430−1.2001.1480.7390.480[15]Table 3The values of parameters and their corresponding magnetic momentsχμΩμΔ++ξ=−1−2−3−1−2−311.0−1.945−1.955−1.9665.845.875.9011.1−1.956−1.966−1.9775.895.925.9511.2−1.967−1.977−1.9885.945.975.9911.3−1.978−1.988−1.9985.996.026.0511.4−1.988−1.999−2.0096.046.076.0911.5−1.999−2.010−2.0206.096.116.1411.6−2.010−2.020−2.0316.146.166.1911.7−2.021−2.032−2.0426.186.216.2411.8−2.032−2.042−2.0536.236.266.29Two new sum rules for octet-baryon magnetic moments (μ) and constraints on QCD sum rules from new experimental determination of μ-s for the decupletMonikaSinhaa14AshikIqubalbMiraDeya24JishnuDeya23deyjm@giascl01.vsnl.net.inaAbdus Salam ICTP, Trieste, ItalybTheory Division, TIFR, Mumbai, India1CSIR Research fellow, Government of India.4On leave from Department of Physics, Presidency College, Kolkata 700 073, India.2Work supported in part by DST grant No. SP/S2/K03/01, Government of India. Permanent address: 1/10 Prince Golam Md. Road, Kolkata 700 026, India.3On leave from Department of Physics, Maulana Azad College, Kolkata 700 013, India.Editor: H. GeorgiAbstractRecently the μΔ++ was found from a fit to π+p scattering [G.L. Castro, A. Mariano, Phys. Lett. B 517 (2002) 339]. This enable us to pinpoint condensate parameters more precisely in the context of QCD sum rules (QCDSR). In the octet sector, the Coleman–Glashow sum rule (CGSR) [S. Coleman, S.L. Glashow, Phys. Rev. Lett. 6 (1961) 423] is violated by the experimental μ-s. QCDSR allows us to write down two sum rules similar to the CGSR, which are obeyed by the experimental magnetic moments, whereas they rule out a specific model using the Wilson loop approach and a particular chiral quark model. It is amusing to note that the QCDSR allows us to write down the quark and gluon condensates in terms of measurables like the μ-s of the nucleons and the Σ±.KeywordsQCD sum rulesMagnetic moments of octet and decuplet baryonsMagnetic moment sum rules1IntroductionMagnetic moments of baryons depend very sensitively on model parameters. So accurately measured values of baryon magnetic moments are very useful to constrain the validity of modeling.In the decuplet sector μΩ was measured accurately and differs from most of the theoretical estimates, thus posing a challenge to the latter. It was shown [3] that this can be explained from QCDSR and QCD condensate parameters are thereby constrained.Recently there has been much experimental and theoretical studies, seemingly a little isolated, with different groups not conscious of each other's work. But these studies of magnetic moments can be correlated to evolve a picture of the QCD vacuum which is very rich. Correlations between μB should also be interesting to experimentalists. Thus for example Kotulla et al. [4], during their determination of μΔ+ should have found the QCDSR relation μΔ++ = 12μΔ+ interesting, in view of the earlier determination of μΔ++ by Castro and Mariano [1]. We write down two other sum rules involving octet baryon μB, hoping to stimulate more studies of these objects.QCDSR enables us to write down the quark and gluon condensates in terms of the octet magnetic moments, for example μp, μn and μΣ±.We also find that the magnetic susceptibility needs to be very large to fit the determination of the magnetic moment of Δ++, made in [1], from the most sensitive observables in radiative π+p scattering.Iqubal et al. [3] used the QCDSR to fit the Ω magnetic moment. μΩ has been the subject of many studies [5–10]. The magnetic moment was unknown, when the large colour Fock approximation paper [5] was published. But on hindsight, the value predicted there, within the acceptable parameter range, agrees with the presently determined experimental result [11].55The methods of this calculation are now used for strange star matter [12,13]. The results of Lee [6] using QCDSR and those from the lattice calculation [8] underestimated it whereas the light-cone relativistic quark model [9] and the chiral quark soliton model [10] overestimated it. This intriguing situation was investigated by looking at the calculations of Lee using a slightly different point of view advocated in [14] and it was found that one indeed gets good agreement with experiment [3].Further, it was pointed out in [3,6] the μΔ++ depend sensitively on the magnetic susceptibility. This moment is now obtained in [1]. They have determined the μ of the Δ++ resonance by using a full dynamical model which consistently describes the elastic and radiative π+p scattering data. It also reproduce very well the total and differential cross-sections for elastic π+p scattering close to the resonance region. It provides an amplitude for radiative π+p scattering that satisfies electro magnetic gauge invariance when finite width effects of Δ++ resonance are taken into account. From their determination we can fix the magnetic susceptibility parameter of QCDSR.As already mentioned, very recently Kotulla et al. have investigated the reaction γpπ0γp. Through the reaction channel they arrived at the magnetic dipole moment of the Δ+ (1232) resonance [4]. Their measured value is also consistent with QCDSR.We have summarized the values of experimentally determined magnetic moments [1,4,11] in the Table 1.The Coleman and Glashow sum rule CGSR [2] is given by (1)ΔCGp−μnΣΣ+Ξ0−μΞ=0.Experimental numbers give ΔCG=0.49μN.From the experimental values of octet magnetic moments we can get the values of the quark and gluon condensates respectively: (2)a=−2π2q̄q〉=−0.4618(μp+2μn)−1.8382(μΣ++2μΣ),(3)b=gs2G2=−4.4545(μp+2μn)−21.2651(μΣ++2μΣ).Putting the values of the experimental moments one gets numerical values a=0.472 and b=1.667. The former matches with the value we use, the latter differs in the last figure, we use 1.664.We have two new sum rules, SR1 and SR2, resulting from the scaling of the baryonic coupling to its current [14]. These are as follows: (4)ΔSR1=(μp+2μn)+6.7096(μΣ++2μΣ)−3.4484(μΞ−μΞ0)+2.1741=0,(5)ΔSR2=(μp+2μn)+4.7738(μΣ++2μΣ)−0.9988(μΞ−μΞ0)+0.9781=0.Using the experimental values of magnetic moments [11] the left-hand side of these two sum rules (Eqs. (4) and (5)) give ΔSR1=4.4929×10−4μN and ΔSR2=5.3175×10−3μN. These sum rules are very powerful. For example, the chiral quark model for octet baryon magnetic moments of Dahiya and Gupta [15] becomes questionable, although it satisfies the ΔCG while fitting the experimental moments approximately. The agreement to ΔCG obtained in this paper is clearly accidental; the small departures from the experimental moments cancel for CGSR, but do not for ΔSR1 and ΔSR2 (see Table 2). However, it is possible that with more judicious choice of parameters the chiral quark model may be able to satisfy the new sum rules given by us.The same comments apply to the model of Ha and Durand [16] in Table 2. They fit the ΔCG fairly well but their model fails for ΔSR1 and ΔSR2. The decomposition of the magnetic moments in terms of the parameters of Table VI of their paper may perhaps be used effectively to satisfy the new sum rules.2QCDSR for decuplet μBAs is widely known, QCDSR is a very powerful tool in revealing a deep connection between hadron phenomenology and vacuum structure [17] via a few condensates like a, b, related to the quark (q) and gluon (G) vacuum expectation values. These can be used for evaluating μB[18,19], where some new parameters enter, for example, χ, κ and ξ, defined through the following equations: (6)q̄σμνqF=eqχ〈q̄q〉Fμν,(7)q̄gGμνqF=eqκ〈q̄q〉Fμν,(8)q̄ϵμνργGργγ5qF=eqξ〈q̄q〉Fμν, where the F denotes the usual external electromagnetic field tensor. Lee [6] very carefully evaluated the contributions of these operators to the magnetic moments of the Ω and Δ++, the latter emerging from the former when the quark mass ms, is put equal to zero, the parameter f and φ are put equal to 1 and the quark charge es=−1/3 is replaced by eu=2/3. The parameter f and φ measure the ratio of values for quark condensates and quark spin-condensates with strange and ud quarks. (9)f=s̄s〉ūu〉,(10)φ=s̄σμνs〉ūσμνu〉.For the expression for the μΩ and Δ++ sum rules we refer the expressions derived in Lee [6] which we reproduce here for the sake of completeness, in terms of the Borel parameter M and the intermediate state contribution A: (11)928esL4/27E1M4157esfφmsχaL−12/27E0M2+356esbL4/27187esfmsaL4/27928esfφ(2κ+ξ)msaL4/2767esf2φχa2L12/2747esf2κva2L28/271M2114esf2φ(4κ+ξ)a2L28/271M2+14esf2φχm20a2L−2/271M2928esfmsm20aL−10/271M2+112esf2m20a2L14/271M4=λ̃2ΩμΩM2+Ae−M2Ω/M2. Here (12)En(x)=1−e−xnxnn!,x=wB2MB2, where wB is the continuum, and (13)L=ln(M22QCD)ln22QCD). For evaluating the magnetic moment we use the above equation and divide by the equation for the mass sum rule given earlier by Lee [20]. Thus we eliminate the parameter λΩ in the spirit of [14] and we get an excellent fit to the resulting numbers in the form μΩ+A/M2. We find that the results are not very sensitive to κv, the so-called factorization violation parameter, defined through (14)ūuūu〉=κvūu〉2. Neither are the results very sensitive to the parameters κ and ξ. We use the crucial parameters a and b from [14], since they must fit the octet baryon moment-differences (μpμn) and (μΣ+μΣ). It was shown in [14] that by using the empirical scaling of the λ̃ with the (baryon mass)3—these differences depend only of a and b, and one gets a=0.475 GeV3 and b=1.695 GeV4. In this Letter we have used slightly different values 0.472 and 1.664 for a and b. Further, to fit the difference (μΞ0μΞ), ms was set to be 170 MeV in [14] and we use this value.Table 3 shows the dependence of the magnetic moments on the parameters. Clearly, the agreement with experiment is very good both for μΔ++ and μΩ. Obviously, the former does not depend on f and φ. It is found that χ∼11 is the best choice for the μΔ++. For such a χ one should take φ∼0.35 and f∼0.564 to get the experimental value of μΩ=(−2.019±0.054)μN[11]. The μΔ++ is known only approximately, (6.14±0.51)μN[1] and a better determination will enable us to pinpoint χ. As such the experimental determination is very important since it gives us a very large magnetic susceptibility χ.Dahiya and Gupta [21], in their paper on decuplet μB, seem to be unaware of the 2001 publication of [1] and their fit to μΔ++ is poor.3Results and discussionWe find that using the constrained values of the parameters a and b[14] one can get a good fit to the known decuplet magnetic moments. The moments may be used to pinpoint (1) the susceptibility χ, (2) f and (3) φ, the ratios of the condensate and spin condensate for strange and ud quarks.For octet magnetic moments two sum rules are written down from QCDSR (Eqs. (4) and (5)). These two sum rules are used to rule out some specific quark model calculation which claim to have fitted experimental magnetic moments satisfactorily but are obviously in contradiction with QCDSR. It is just that the sum rules highlight the discrepancies in the particular combination of the moments, to point out the inadequacy of the models. We hope future theoretical models will try to accommodate these new sum rules in their fitting while the new experimental data will continue to satisfy them.It is interesting that the quark and gluon condensates can be written out directly in terms of octet magnetic moments (Eqs. 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