PHYSICAL REVIEW D 66, 034012 ~2002! Muon transverse polarization in the Kl2g decay in the standard model V. V. Braguta and A. E. Chalov Moscow Institute of Physics and Technology, Moscow, 141700 Russia A. A. Likhoded* Instituto de Fı´sica Teo´rica–UNESP, Rua Pamplona, 145, 01405-900 Sa˜o Paulo, SP, Brazil ~Received 26 March 2002; published 15 August 2002! The muon transverse polarization in theK1→m1ng process induced by the electromagnetic final state interaction is calculated in the framework of the standard model. It is shown that one loop contributions lead to a nonvanishing muon transverse polarization. The value of the muon transverse polarization averaged over the kinematical region ofEg>20 MeV is equal to 5.6331024. DOI: 10.1103/PhysRevD.66.034012 PACS number~s!: 13.88.1e, 13.20.Eb, 13.40.Ks ly th s bo re u- a - f - It co he ion m y is n fi th o ia st - in s- as cs I. INTRODUCTION The study of the radiativeK-meson decays is extreme interesting in searching for new physics effects beyond standard model~SM!. One of the most appealing possibilitie is to probe new interactions, which could lead toCP viola- tion. Contrary to the SM, whereCP violation is caused by the presence of the complex phase in the Cabib Kobayashi-Maskawa~CKM! matrix, theCP violation in ex- tended models~for instance, in models with three and mo Higgs doublets! can naturally arise due to the complex co plings of new Higgs bosons to fermions@1#. Such effects can be detected by using experimental observables, which essentially sensitive toT-odd contributions. These observ ables, for instance, are theT-odd correlation $T 5(1/MK 3 )pW g•@pW p3pW l #% in theK6→p0m6ng decay@2# and muon transverse polarization (PT) in K6→m6ng. The search for new physics effects using theT-odd correlation analysis in theK6→p0m6ng decay will be done in the proposed OKA experiment@3#, where an event sample o 7.03105 for the K1→p0m1ng decay is expected to be ac cumulated. At the moment the E246 experiment at KEK@4# performs the analysis of the data on theK6→m6ng process to put bounds on theT-violating muon transverse polarization. should be noted that the expected value of new physics tribution to PT can be of the order of.7.031023–6.0 31022 @5,6#, depending on the type of model beyond t SM. Thus, when one searches for new physics contribut to PT , it is extremely important to estimate the effects co ing from so called ‘‘fake’’ polarization, which is caused b the SM electromagnetic final state interactions and which natural background for the new interaction contributions. In this paper we calculate muon transverse polarizatio the K6→m6ng process, induced by the electromagnetic nal state interaction in the one-loop approximation of minimal quantum electrodynamics. In next section we present the calculations of the mu transverse polarization taking into account one-loop d *On leave of absence from Institute for High Energy Physi Protvino, 142284 Russia. Email address: andre@ift.unesp.br 0556-2821/2002/66~3!/034012~8!/$20.00 66 0340 e - re n- s - a in - e n - grams with final state interactions within the SM. The la section summarizes the results and conclusions. II. MUON TRANSVERSE POLARIZATION IN THE K¿\µ¿ng PROCESS IN SM The K1→m1ng decay at the tree level of SM is de scribed by the diagrams shown in Fig. 1. The diagrams Figs. 1~b! and 1~c! correspond to the muon and kaon brem strahlung, while the diagram in Fig. 1~a! corresponds to the structure radiation. This decay amplitude can be written follows: M5 ie GF A2 Vus* «m* F f Kmmū~pn!~11g5!S pK m ~pKq! 2 ~pm!m ~pmq! 2 q̂gm 2~pmq! D v~pm!2Gmnl nG , ~1! where l m5ū~pn!~11g5!gmv~pm!, Gmn5 iF v«mnabqa~pK!b2Fa~gmn~pKq!2pK mqn!, ~2! , FIG. 1. Feynman diagrams for theK6→m6ng decay at the tree level of SM. ©2002 The American Physical Society12-1 t, ur s. uc b pe on po tri o er n uo ol he is on e of ia- ion. an r- e on y V. V. BRAGUTA, A. E. CHALOV, AND A. A. LIKHODED PHYSICAL REVIEW D 66, 034012 ~2002! GF is the Fermi constant,Vus is the corresponding CKM matrix element, f K is the K-meson leptonic constan pK ,pm ,pn ,q are the kaon, muon, neutrino, and photon fo momenta, correspondingly, and«m is the photon polarization vector.Fv andFa are the kaon vector and axial form factor In Eq. ~2! we use the following definition of Levi-Civita tensor:e0123511. The part of the amplitude which corresponds to the str ture radiation and kaon bremsstrahlung and which will used further in one-loop calculations, has the form MK5 ie GF A2 Vus* «m* F f Kmmū~pn!~11g5! 3S pK m ~pKq! 2 gm m mD v~pm!2Gmnl nG . ~3! The partial width of theK1→m1ng decay in theK-meson rest frame can be expressed as dG5 ( uM u2 2mK ~2p!4d~pK2pm2q2pn! 3 d3q ~2p!32Eq d3pm ~2p!32Em d3pn ~2p!32En , ~4! where summation over muon and photon spin states is formed. Introducing the unit vector along the muon spin directi in muon rest framesW whereeW i ( i 5L,N,T) are the unit vec- tors along the longitudinal, normal and transverse com nents of muon polarization, one can write down the ma element squared for the transition into the particular mu polarization state in the following form: uM u25r0@11~PLeWL1PNeWN1PTeWT!•sW#, ~5! wherer0 is the Dalitz plot probability density averaged ov polarization states. The unit vectorseW i can be expressed i terms of the three-momenta of final particles eWL5 pW m upW mu , eWN5 pW m3~qW 3pW m! upW m3~qW 3pW m!u , eWT5 qW 3pW m uqW 3pW mu . ~6! With such definition ofeW i vectors,PT , PL , andPN denote transverse, longitudinal, and normal components of the m polarization, correspondingly. It is convenient to use the f lowing variables: x5 2Eg mK , y5 2Em mK , l5 x1y212r m x , r m5 mm 2 mK 2 , ~7! whereEg and Em are the photon and muon energies in t kaon rest frame. The Dalitz plot probability density, as a function of thex andy variables, has the form 03401 - - e r- - x n n - r05 1 2 e2GF 2 uVusu2H 4mm 2 u f Ku2 lx2 ~12l!Fx212~12r m!S 12x 2 r m l D G1mK 6 x2~ uFau21uFvu2!~y22ly2lx12l2! 14 Re~ f KFv* !mK 4 r m x l ~l21! 14 Re~ f KFa* !mK 4 r mS 22y1x12 r m l 2 x l 12l D 12 Re~FaFv* !mK 6 x2~y22l1xl!J . ~8! Calculating the muon transverse polarizationPT we follow the original paper@7# and assume that the decay amplitude CP invariant, and form factorsf K , Fv , andFa are real. In this case the tree level muon polarizationPT50. When one- loop contributions are incorporated, the nonvanishing mu transverse polarization can arise due to the interferenc tree-level diagrams and imaginary parts of one-loop d grams, induced by the electromagnetic final state interact To calculate the imaginary parts of formfactors one c use theS-matrix unitarity S1S51 ~9! and, usingS511 iT, one gets Tf i2Ti f* 5 i( n Tn f* Tni , ~10! wherei , f ,n indices correspond to the initial, final, and inte mediate states of the particle system. Further, using thT invariance of the matrix element one has Im Tf i5 1 2 ( n Tn f* Tni , ~11! Tf i5~2p!4d~Pf2Pi !M f i . ~12! One-loop diagrams of the SM, which contribute to the mu transverse polarization in theK1→m1ng decay, are shown in Fig. 2. Using Eq.~3! one can write down the imaginar parts of these diagrams. For the diagrams in Figs. 2~a!, 2~c! one has Im M15 iea 2p GF A2 Vus* ū~pn!~11g5! 3E d3kg 2vg d3km 2vm d~kg1km2P!Rm~ k̂m2mm!gm 3 q̂1 p̂m2mm ~q1pm!22mm 2 gd«d* v~pm!. ~13! For the diagrams in Figs. 2~b!, 2~d! one has 2-2 s - e wn ters ry - le- gi- n nd s rs MUON TRANSVERSE POLARIZATION IN . . . PHYSICAL REVIEW D66, 034012 ~2002! ImM25 iea 2p GF A2 Vus* ū~pn!~11g5!E d3kg 2vg d3km 2vm 3d~kg1km2P!Rm~ k̂m2mm!gd«d* k̂m2q̂2mm ~km2q!22mm 2 3gmv~pm!, ~14! where Rm5 f KmmS ~pK!m ~pKkg! 2 gm mm D2 iF v«mnab~kg!a~pK!bgn 1Fa@gm~pKkg!2~pK!mk̂g#. ~15! To write down the contributions of diagrams shown in Fig 2~e!, 2~f!, one should substituteRm by Rm5 f KmmS gm mm 2 ~km!m ~kmkg! 2 k̂ggm 2~kmkg! D ~16! FIG. 2. Feynman diagrams contributing to the muon transve polarization at the one-loop level of SM. 03401 . in expressions~13!,~14!. Using thex PT Lagrangian@8#, one can derive decay am plitudes for theK1→p0m1n andp0→gg processes, which contribute to the imaginary part of the diagram in Fig. 2~g!: T~K1→p0m1n!52 GF 2 ū~pn!~11g5!~ p̂K1 p̂p!v~pm!, T~p0→gg!5 aA2 pF emnlsk1 me1 nk2 ae2 s , ~17! whereF5132 MeV. It should be noted thatT(p0→gg) is written at O(p2) level. In addition, the amplitude differs from the one in Ref.@8# by the sign, since we used th opposite sign of pseudoscalar octet of mesons. From Eq.~17! one can write down the imaginary part of the diagram sho in Fig. 2~g!: Im M35 GFa 8A2p3F eE d3kp 2vp d3km 2vm d~kp1km2P! 3 ersabqaeb* kr p kg 2 ū~pn!~11g5!~ p̂K1 k̂p! 3~ k̂m2mm!gsv~pm!. ~18! The details of the calculations of integrals entering Eqs.~13!, ~14!, ~18!, and their dependence on kinematical parame are given in Appendix A. The expression for the amplitude including the imagina one-loop contributions can be written as M5 ie GF A2 Vus* «m* F f̃ Kmmū~pn!~11g5!S pK m ~pKq! 2 ~pm!m ~pmq! D 3v~pm!1F̃nū~pn!~11g5!q̂gmv~pm!2G̃mnl nG , ~19! where G̃mn5 i F̃ v«mnabqa~pK!b2F̃a@gmn~pKq!2pK mqn#. ~20! The f̃ K , F̃v , F̃a , andF̃n form factors include one-loop con tributions from diagrams shown in Figs. 2~a!–2~f!. The choice of the form factors is determined by the matrix e ment expansion into set of gauge-invariant structures. As long as we are interested in the contributions of ima nary parts of one-loop diagrams only~since they lead to a nonvanishing value of the transverse polarizatio!, we neglect the real parts of these diagrams a assume that Ref̃ K ,ReF̃v ,ReF̃a coincide with their tree-level valuesf K ,Fv ,Fa , correspondingly, and ReF̃n 52 f Kmm/2(pmq). Explicit expressions for imaginary part of the form factors are given in Appendix B. The muon transverse polarization can be written as PT5 rT r0 , ~21! e 2-3 n nt ig rm on e po is tr , s e n e. po r- i e oin- - gi- s. u- s. our po- n ar- the hor on se V. V. BRAGUTA, A. E. CHALOV, AND A. A. LIKHODED PHYSICAL REVIEW D 66, 034012 ~2002! where rT52mK 3 e2GF 2 uVusu2xAly2l22r mFmmIm~ f̃ KF̃a* ! 3S 12 2 x 1 y lxD1mmIm~ f̃ KF̃v* !S y lx 2122 r m lxD 12 r m lx Im~ f̃ KF̃n* !~12l!1mK 2 x Im~ F̃nF̃a* !~l21! 1mK 2 xIm~ F̃nF̃v* !~l21!G . ~22! It should be noted that Eq.~20! disagrees with the expressio for rT in Ref. @9#. In particular, the terms containing ImFn are missing in therT expression given in Ref.@9#. Moreover, calculating the muon transverse polarization we took i account the diagrams shown in Figs. 2~e!–2~g!, which have been neglected in Ref.@9#, and which give the contribution comparable with the contribution from other diagrams in F 2. III. RESULTS AND DISCUSSION For the numerical calculations we use the following fo factor values: f K50.16 GeV, Fv5 0.095 mK , Fa52 0.043 mK . The f K form factor is determined from experimental data kaon decays@10#, and theFv ,Fa ones are calculated at th one loop-level in the chiral perturbation theory@11#. It should be noted that our definition forFv differs by a sign from that in Ref.@11#. With this choice of form factor values the decay branching ratio Br(K6→m6ng), with the cut on photon energyEg>20 MeV, is equal to53.331023, which is in good agreement with the PDG data. The three-dimensional distribution of muon transverse larization, calculated in the one-loop approximation of SM shown in Figs. 3 and 4.PT , as function of thex and y parameters, is characterized by the sum of individual con butions of diagrams in Figs. 2~a!–2~f!, while the contribu- tions from diagrams 2~a!–2~d! @12# and 2~e!–2~f! are com- parable in absolute value, but they are opposite in sign that the totalPT(x,y) distribution is the difference of thes group contributions and in absolute value it is about o order of magnitude less than each individual one of thos It should be noted that the value of muon transverse larization is positive in the whole Dalitz plot region. Ave aged value of transverse polarization can be obtained by tegrating the function 2rT /G(K1→m1ng) over the physical region, and with the cut on photon energyEg .20 MeV it is equal to ^PT SM&55.6331024. ~23! Let us note that the obtained numerical value of the av aged transverse polarization andPT(x,y) kinematical depen- dence in Dalitz plot differ from those given in Refs.@9,13#. 03401 o . - i- o e - n- r- Note that in Ref.@13# only the diagram shown in Fig. 2~g! was calculated and the result for that diagram does not c cide with ours. As it was calculated in Ref.@9#, thePT value varies in the range of (20.1–4.0)31023 for cuts on the muon and pho ton energies 200,Em,254.5 MeV, 20,Eg,200 MeV. We have already mentioned above that~1! the authors of Ref. @9# did not take into account terms containing the ima nary part of theFn form factor ~contributing torT), which, in general, are not small being compared with others, and~2! the authors of Ref.@9# omitted the diagrams, shown in Fig 2~e!–2~f!, though, as was mentioned above, their contrib tion to PT is comparable with the one of diagrams in Fig 2~a!–2~d!, and ~3! the authors of Ref.@9# did not take into account the diagram shown in Fig. 2~g!. All these points lead to serious disagreement between results and results obtained in Ref.@9#. In particular, our calculations show that the value of the muon transverse larization has positive sign in the whole Dalitz plot regio and its absolute value varies in the range of~0.0–1.5) 31023, and thePT dependence on thex,y parameters is different from that in Ref.@9#. We would like to remark that the muon transverse pol ization for the same process was calculated in Ref.@14#, where the contributions from diagrams 2~e!, 2~f!, and 2~g! were taken into account. However, our result differs from one obtained in Ref.@14#: PT value has opposite sign in comparison to ours and in numerical calculation the aut of Ref. @14# used constantf p instead off K in Eq. ~1!. Since FIG. 3. The 3D Dalitz plot for the muon transverse polarizati as a function ofx52Eg /mK andy52Em /mK in the one-loop ap- proximation of SM. FIG. 4. Level lines for the Dalitz plot of the muon transver polarizationPT5 f (x,y). 2-4 e ru . he fo is fo 64 n y te th ng hich MUON TRANSVERSE POLARIZATION IN . . . PHYSICAL REVIEW D66, 034012 ~2002! the calculation is produced atO(p4) level, one needs to us f K , as have been done in our paper. The kinematical st tures for diagrams Figs. 2~a!–2~g! in Ref. @14# coincide with ours. ACKNOWLEDGMENTS The authors thank Dr. V. V. Kiselev and Dr. A. K Likhoded for fruitful discussion and valuable remarks. T authors are also grateful to F. Bezrukov and D. Gorbunov their remarks on the sign of the form factorFv in our previ- ous results and R. Rogalyov for fruitful discussion. Th work was in part supported by the Russian Foundation Basic Research, Grants Nos. 99-02-16558 and 00-15-96 Russian Education Ministry, Grants No. RF E00-33-062 a CRDF MO-011-0. The work of A. A. Likhoded was partiall funded by a FapesP Grant No. 2001/06391-4. APPENDIX A For the integrals, which contribute to Eqs.~14! and ~15!, we use the following notations: P5pm1q, ~A1! dr5 d3kg 2vg d3km 2vm d~kg1km2P!. We present below either the explicit expressions for in grals, or the set of equations, which being solved, give parameters, entering the integrals: J115E dr5 p 2 P22mm 2 P2 , J125E dr 1 ~pKkg! 5 p 2I lnS ~PpK!1I ~PpK!2I D , where I 25~PpK!22mK 2 P2, E dr kg a ~pKkg! 5a11pK a1b11P a. The a11 andb11 parameters are determined by the followi equations: a1152 1 ~PpK!22mK 2 P2 S P2J112 J12 2 ~PpK!~P22mm 2 ! D , b115 1 ~PpK!22mK 2 P2 S ~PpK!J112 J12 2 mK 2 ~P22mm 2 ! D , E drkg a5a12P a, 03401 c- r r 5, d - e E drkg akg b5a13g ab1b13P aPb, where a125 ~P22mm 2 ! 2P2 J11, a1352 1 12 ~P22mm 2 !2 P2 J11, b135 1 3 S P22mm 2 P2 D 2 J11. J15E dr 1 ~pKkg!@~pm2kg!22mm 2 # 52 p 2I 1~P22mm 2 ! lnS ~pKpm!1I 1 ~pKpm!2I 1 D , J25E dr 1 ~pm2kg!22mm 2 52 p 4I 2 lnS ~Ppm!1I 2 ~Ppm!2I 2 D , where I 1 25~pKpm!22mm 2 mK 2 , I 2 25~Ppm!22mm 2 P2. E dr kg a ~pm2kg!22mm 2 5a1Pa1b1pm a , a152 mm 2 ~P22mm 2 !J21~Ppm!J11 2~~Ppm!22mm 2 P2! , b15 ~Ppm!~P22mm 2 !J21P2J11 2@~Ppm!22mm 2 P2# , The integrals below are determined by the parameters, w can be obtained by solving the sets of equations: E dr kg a ~pKkg!@~pm2kg!22mm 2 # 5a2Pa1b2pK a1c2pm a , 2-5 ppendix V. V. BRAGUTA, A. E. CHALOV, AND A. A. LIKHODED PHYSICAL REVIEW D 66, 034012 ~2002! a2~PpK!1b2mK 2 1c2~pKpm!5J2 , a2~Ppm!1b2~pKpm!1c2mm 2 52 1 2 J12, a2P21b2~PpK!1c2~Ppm!5~pmq!J1 , E dr kg akg b ~pKkg!@~pm2kg!22mm 2 # 5a3gab1b3~PapK b1PbpK a !1c3~Papm b1Pbpm a !1d3~pK apm b1pK bpm a ! 1e3pm apm b1 f 3PaPb1g3pK apK b , 4a312b3~PpK!12c3~Ppm!12d3~pKpm!1g3mK 2 1e3mm 2 1 f 3P250, c3~pKpm!1b3mK 2 1 f 3~PpK!2a150, c3~PpK!1d3mK 2 1e3~pKpm!2b150, a31b3~PpK!1d3~pKpm!1g3mK 2 50, b3~pKpm!1c3mm 2 1 f 3~Ppm!52 1 2 b11, b3~Ppm!1d3mm 2 1g3~pKpm!52 1 2 a11, a3P212b3P2~PpK!12c3P2~Ppm!12d3~Ppm!~PpK!1e3~Ppm!21 f 3~P2!21g3~PpK!25~pmq!2J1 , E dr kg akg b ~pm2kg!22mm 2 5a4gab1b4~Papm b1Pbpm a !1c4PaPb1d4pm apm b , a41d4mm 2 1b4~Ppm!50, b4mm 2 1c4~Ppm!52 1 2 a12, 4a412b4~Ppm!1c4P21d4mm 2 50, a4P212b4P2~Ppm!1c4~P2!21d4~Ppm!25 ~P22mm 2 !2 4 J2 , E dr kg akg bkg d ~pm2kg!22mm 2 5a5~gabpm d 1gdapm b1gbdpm a !1b5~gabPd1gdaPb1gbdPa!1c5pm apm bpm d 1d5PaPbPd 1e5~Papm bpm d 1Pdpm apm b1Pbpm d pm a !1 f 5~PaPbpm d 1PdPapm b1PbPdpm a !, 2a51c5mm 2 1e5~Ppm!50, a5mm 2 1b5~Ppm!52 1 2 a13, b51e5mm 2 1 f 5~Ppm!50, d5~Ppm!1 f 5mm 2 52 1 2 b13, 6a51c5mm 2 12e5~Ppm!1 f 5P250, 3a5P2~Ppm!13b5~P2!21c5~Ppm!31d5~P2!313e5P2~Ppm!213 f 5~P2!2~Ppm!5 ~P22mm 2 !3 8 J2 . For the rest of the integrals the following notations are used: Pkp5 1 2 ~P21mp 2 2mm 2 !, dr5 d3kp 2vp d3km 2vm d~kp1km2P!. In terms of this notation the integrals can be rewritten as follows: J35E dr kg 2 52 p 4Pq LnU2~Pq!Pkp12~Pq!APkp 2 2mp 2 P22mp 2 P2 2~Pq!Pkp22~Pq!APkp 2 2mp 2 P22mp 2 P2U , J45E dr5 p P2 A~Pkp!22mp 2 P2. APPENDIX B Here we present the expressions for imaginary parts of form factors as the functions of parameters, calculated in A A. 034012-6 MUON TRANSVERSE POLARIZATION IN . . . PHYSICAL REVIEW D66, 034012 ~2002! Im f̃ K5 a 2p f K@24a3~pKq!14a2mm 2 ~pKq!22b3mm 2 ~pKq!14c2mm 2 ~pKq!24c3mm 2 ~pKq!22d3mm 2 ~pKq!22e3mm 2 ~pKq! 22 f 3mm 2 ~pKq!14a2~pKq!~pmq!24b3~pKq!~pmq!24c3~pKq!~pmq!24 f 3~pKq!~pmq!#1 a 2p Fa@8a4~pKq! 28a5~pKq!28b5~pKq!18b4mm 2 ~pKq!14c4mm 2 ~pKq!22c5mm 2 ~pKq!14d4mm 2 ~pKq!22d5mm 2 ~pKq! 26e5mm 2 ~pKq!26 f 5mm 2 ~pKq!112b4~pKq!~pmq!18c4~pKq!~pmq!14d4~pKq!~pmq!24d5~pKq!~pmq! 24e5~pKq!~pmq!28 f 5~pKq!~pmq!#1 a 2p Fv@8a4~pKq!28a5~pKq!28b5~pKq!18b4mm 2 ~pKq!14c4mm 2 ~pKq! 22c5mm 2 ~pKq!14d4mm 2 ~pKq!22d5mm 2 ~pKq!26e5mm 2 ~pKq!26 f 5mm 2 ~pKq!112b4~pKq!~pmq!18c4~pKq!~pmq! 14d4~pKq!~pmq!24d5~pKq!~pmq!24e5~pKq!~pmq!28 f 5~pKq!~pmq!#, Im F̃a5 a 2p f KS a2mm 2 12c2mm 2 2c3mm 2 22d3mm 2 2e3mm 2 2 a1mm 2 ~pmq! 2 b1mm 2 ~pmq! 1 2b4mm 2 ~pmq! 1 c4mm 2 ~pmq! 1 d4mm 2 ~pmq! D 1 a 2p Fv@8a424a5 212b522a1mm 2 14b4mm 2 15c4mm 2 2c5mm 2 2d4mm 2 23d5mm 2 25e5mm 2 27 f 5mm 2 12a1~pKpm!24b4~pKpm! 24c4~pKpm!12d5~pKpm!12e5~pKpm!14 f 5~pKpm!12a1~pKq!22b4~pKq!24c4~pKq!12d5~pKq!12 f 5~pKq! 24a1~pmq!16b4~pmq!110c4~pmq!26d5~pmq!22e5~pmq!28 f 5~pmq!#1 a 2p Fa@26a412a51c4mm 2 2d4mm 2 2d5mm 2 2e5mm 2 22 f 5mm 2 12a1~pKpm!24b4~pKpm!24c4~pKpm!12d5~pKpm!12e5~pKpm!14 f 5~pKpm! 12a1~pKq!22b4~pKq!24c4~pKq!12d5~pKq!12 f 5~pKq!12c4~pmq!22d5~pmq!22 f 5 ~pmq!#. Im F̃n5 a 2p f KF4a1mm12a3mm12b1mm1b11mm22b4mm22c4mm2J12mm22J2mm2b2mK 2 mm1g3mK 2 mm22a2mm 3 2c2mm 3 1c3mm 3 1 f 3mm 3 22a2mm~pKpm!22b2mm~pKpm!12b3mm~pKpm!22c2mm~pKpm!12d3mm~pKpm! 12J1mm~pKpm!12b3mm~pKq!2 a12mm 3 ~pmq!2 2 J11mm 3 ~pmq!2 2 a12mm ~pmq! 2 2a4mm ~pmq! 1 J11mm ~pmq! 2 a11mK 2 mm 2~pmq! 1 3a1mm 3 ~pmq! 1 3b1mm 3 ~pmq! 1 b11mm 3 2~pmq! 2 2J2mm 3 ~pmq! 2 b11mm~pKpm! ~pmq! 1 J12mm~pKpm! ~pmq! 2 b11mm~pKq! ~pmq! 1 J12mm~pKq! ~pmq! 22a2mm~pmq!12c3mm~pmq! 12 f 3mm~pmq!G1 a 2p FvS 2a4mm24a5mm12b13mm24b5mm22a1mm 3 1c4mm 3 2c5mm 3 2d4mm 3 2d5mm 3 23e5mm 3 23 f 5mm 3 12a1mm~pKpm!22c4mm~pKpm!12d4mm~pKpm!12d5mm~pKpm!12e5mm~pKpm!14 f 5mm~pKpm! 22c4mm~pKq!12d5mm~pKq!12 f 5mm~pKq!1 3a13mm ~pmq! 1 b13mm 3 ~pmq! 2 b13mm~pKpm! ~pmq! 2 b13mm~pKq! ~pmq! 22a1mm~pmq! 12c4mm~pmq!22d4mm~pmq!22d5mm~pmq!22e5mm~pmq!24 f 5mm~pmq! D 1 a 2p FaS 26a4mm18a5mm2b13mm 18b5mm24b4mm 3 22c4mm 3 1c5mm 3 22d4mm 3 1d5mm 3 13e5mm 3 13 f 5mm 3 12a1mm~pKpm!22c4mm~pKpm! 12d4mm~pKpm!12d5mm~pKpm!12e5mm~pKpm!14 f 5mm~pKpm!22c4mm~pKq!12d5mm~pKq!12 f 5mm~pKq! 2 3a13mm ~pmq! 2 b13mm 3 2~pmq! 2 b13mm~pKpm! ~pmq! 2 b13mm~pKq! ~pmq! 26b4mm~pmq!24c4mm~pmq!22d4mm~pmq!12d5mm~pmq! 12e5mm~pmq!14 f 5mm~pmq! D , 034012-7 V. V. BRAGUTA, A. E. CHALOV, AND A. A. LIKHODED PHYSICAL REVIEW D 66, 034012 ~2002! Im F̃v5 a 2p f KS a2mm 2 1c3mm 2 1e3mm 2 1 a1mm 2 ~pmq! 1 b1mm 2 ~pmq! 2 2b4mm 2 ~pmq! 2 c4mm 2 ~pmq! 2 d4mm 2 ~pmq! D 1 a 2p Fa@6a422a528b51c4mm 2 2d4mm 2 2d5mm 2 2e5mm 2 22 f 5mm 2 22a1~pKpm!14b4~pKpm!14c4~pKpm!22d5~pKpm!22e5~pKpm!24 f 5~pKpm! 22a1~pKq!12b4~pKq!14c4~pKq!22d5~pKq!22 f 5~pKq!12c4~pmq!22d5~pmq!22 f 5~pmq!#1 a 2p Fv@28a4 14a514b512a1mm 2 24b4mm 2 23c4mm 2 1c5mm 2 2d4mm 2 1d5mm 2 13e5mm 2 13 f 5mm 2 22a1~pKpm!14b4~pKpm! 14c4~pKpm!22d5~pKpm!22e5~pKpm!24 f 5~pKpm!22a1~pKq!12b4~pKq!14c4~pKq!22d5~pKq!22 f 5~pKq! 14a1~pmq!26b4~pmq!26c4~pmq!12d5~pmq!12e5~pmq!14 f 5~pmq!#. The contribution to imaginary parts coming from the diagram shown in Fig. 2~g! may be written as follows: Im f̃ K50, Im F̃v52 a 8p3F S 3J4mm 2 4P2 2 J4mm 4 mp 2 8~pmq!2P2 1 J3mm 4 mp 4 8~pmq!2P2 2 3J4mm 2 mp 2 8~pmq!P2 1 J3mm 2 mp 4 4~pmq!P2 1 2J4~pmq! P2 D u@P22~mm1mp!2#, ImF̃a52ImF̃v , Im f̃ n52 a 8p3F S 23J4mmmp 2 2P2 1 J3mmmp 4 P2 2 J4mm 5 mp 2 4~pmq!2P2 1 J3mm 5 mp 4 4~pmq!2P2 2 5J4mm 3 mp 2 4~pmq!P2 1 J3mm 3 mp 4 ~pmq!P2D u@P22~mm1mp!2#. , P @1# S. Weinberg, Phys. Rev. Lett.37, 651 ~1976!. @2# V. Braguta, A. Likhoded, and A. Chalov, Phys. Rev. D65, 054038~2002!. @3# V. F. Obraztsov and L. G. Landsberg, Nucl. Phys. B~Proc. Suppl.! 99B, 257 ~2001!. @4# See, for example, M. Abeet al., Phys. Rev. Lett.83, 4253 ~1999!; Yu. G. Kudenko, Yad. Fiz.65, 269 ~2002! @Phys. Atom. Nucl. 65, 244 ~2002!#. @5# J. F. Donoghue and B. Holstein, Phys. Lett.113B, 382~1982!; L. Wolfenstein, Phys. Rev. D29, 2130~1984!; G. Barenboim et al., ibid. 55, 4213 ~1997!; M. Kobayashi, T.-T. Lin, and Y. Okada, Prog. Theor. Phys.95, 361 ~1996!; S. S. Gershtein et al., Z. Phys. C24, 305 ~1984!; R. Garisto and G. Kane Phys. Rev. D44, 2038~1991!. 03401 @6# G. Belanger and C. Q. Geng, Phys. Rev. D44, 2789~1991!. @7# L. B. Okun and I. B. Khriplovich, Sov. J. Nucl. Phys.6, 821 ~1967!. @8# A. Pich, Rep. Prog. Phys.58, 563 ~1995!. @9# V. P. Efrosinin and Yu. G. Kudenko, Phys. Atom. Nucl.62, 987 ~1999!. @10# Particle Data Group, R. Groomet al., Eur. Phys. J. C15, 1 ~2000!. @11# J. Bijnens, G. Ecker, and J. Gasser, Nucl. Phys.B396, 81 ~1993!. @12# A. Likhoded, V. Braguta, and A. Chalov, Report No. IHE 2000-57, 2000. @13# G. Hiller and G. Isidori, Phys. Lett. B459, 295 ~1999!. @14# R. N. Rogalyov, Phys. Lett. B521, 243 ~2001!. 2-8