# Complex-Mass Definition and the Structure of Unstable Particle’s Propagator

Authors: Vladimir Kuksa
Journal: Advances in High Energy Physics
 (2015)

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## Abstract

The propagators of unstable particles are considered in framework of the convolution representation. Spectral function is found for a special case when the propagator of scalar unstable particle has Breit-Wigner form. The expressions for the dressed propagators of unstable vector and spinor fields are derived in an analytical way for this case. We obtain the propagators in modified Breit-Wigner forms which correspond to the complex-mass definition.


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## Body

## 1. Introduction

Two standard definitions of the mass and width of unstable particles (UP), which are usually considered in the literature, have different nature. The on-mass-shell (OMS) scheme defines the massM and width Γ of UP by the renormalization of the self-energy amplitude. In the pole scheme (PS), the definitions of mass and width are based on the complex-valued position of the propagator pole sR-M02-Π(sR)=0. There has been considerable discussion concerning definition of the vector-boson mass [1–11]. It was shown that OMS scheme contains spurious higher-order gauge-dependent terms. Moreover, at one loop in the conventional OMS, the problem of threshold singularity arises which originates from the wave-function renormalization constant Z-1=1-RA′(M2) [6]. The PS provides gauge invariant definition and make it possible to solve the problem of threshold singularity [6, 7]. However, it does not define the mass and width in unique way [12]. One of the PS definitions, where mass Mρ and width Γρ follow from the parametrization sR=Mρ2-iMρΓρ [12], is known as complex-mass definition. It should be noted that the PS definition of the mass and width is connected with the structure of the dressed propagator. Some aspects of the abovementioned problems are considered further in more detail.Traditional way to construct the dressed propagator of UP is the Dyson summation which introduces the width and redefines the mass of UP. This procedure runs into some problems which are widely discussed in the literature. One of such problems follows from the d’Alembert convergence criterion|z|<1 of the series(1)11-z=∑k=0∞zk=1+z+z2+⋯,z<1, where z=Π(1)(q)/(q2-M02) and Π(1)(q) is the one-particle-irreducible self-energy. The variable z should be correctly redefined before summation; that is, we have to perform the renormalization of the Π(1)(q) at Lagrangian level. This procedure must be consistent with the infinite Dyson summation and we cannot use it after the redefinition at z>1. For instance, in the resonant-part approximation we can define z=IΠ(1)(q)/(q2-M2)≈MΓ/(q2-M2). So, the peak range q2-M2<MΓ or q-M<Γ/2 (at Γ≪M) is excluded by d’Alembert convergence criterion. There are, also, the difficulties in the scheme of sequential fixed-order calculations which exhibit themselves in the violation of the gauge invariance. Moreover, using different decompositions of self-energy tensor in the Dyson summation leads to different expressions for vector dressed propagator [13–15]. Then, the renormalization procedure is connected with the truncation of a Laurent series expansion at the resonance range. So, the renormalized propagator is an approximation of the full one which corresponds to exact two-point function.The peculiarities of Dyson summation lead to the lack of uniqueness in constructing the propagators of unstable particles. There are several different expressions for the numerator of vector-boson propagatorgμν-qμqν/f(q,M,Γ), which are exploited in practical calculations and give almost the same numerical results. The denominator f(q,M,Γ) has the following forms (in the unitary gauge): M2, M2-iMΓ, (M-iΓ/2)2, q2, and other combinations with q-dependent M,Γ. So, we need in an additional argumentation concern these semiphenomenological definitions. It is known that the commonly used Breit-Wigner (BW) expressions for bosonic and fermionic propagators, respectively,(2)DμνVq2=-gμν+qμqν/MV2q2-MV2+iMVΓV,DFq^=q^+MFq2-MF2+iMFΓFdo not satisfy the electromagnetic Ward identity [3]. It was shown in [3, 13, 14] that the modified BW propagators,(3)DμνVq2=-gμν+qμqν/MV2-iMVΓVq2-MV2-iMVΓV,DFq^=q^+MF-iΓF/2q2-MF-iΓF/22,satisfy the electromagnetic Ward identity which provides the gauge invariant description of processes with UP participation. Note, here we deal with the resonant part of the full propagator which follows from Dyson summation. The correctness of this propagator should be understood in the context of resonant processes where the usage of the modified BW propagator leads consistently to gauge invariant results [3, 13, 14]. It was also noted in [13] that, in this case, we have to make the modification MV2→MV2-iMVΓV not only in the qμqν term of the propagator, but in the vertexes also. Thus, we get the so-called complex-mass definition which was developed in the framework of the complex-mass scheme (CMS) [16–20]. Recently, BW parametrization of the resonance lines has been developed in the works [21–23]. In particular, a new parameter has been introduced into this parametrization which describes a fundamental property of a resonance [23].All abovementioned definitions are connected with the structure of dressed propagators which follows from Dyson summation. As was noted above, this procedure runs into some problems which are widely discussed in literature. An alternative approach is based on the spectral representation of the propagator of UP. It has a long history [24–34] and treats UP as a nonperturbative state or effective field (asymptotic free field [30, 31]). For the first time, the hypothesis of continuous (smeared) mass of UP was suggested by Matthews and Salam [27]. In this paper, they have formulated “…a very direct interpretation to the spectral function introduced by Kallen [26] and Lehmann [24].” The authors interpreted the spectral function as “…distribution of mass values, with a spread, δm, related to the mean life δτ(=1/λ), by uncertainty relation δmδτ~1” (see Introduction in [27]). In [30, 31], UP is described by the so-called asymptotic free field as the state with indefinite (not fixed) mass. The hypothesis of continuous (smeared, indefinite) mass of UP was developed in a series of works, where a quantum field model of UP was presented (see, e.g., review articles [35, 36] and references therein). In this approach, the physical values of the mass and width are related to the parameters of continuous mass distribution. It should be noted that the definition of the spectral function does not follow from the first principles. So, it was constructed in phenomenological ways and has a different form in abovementioned papers. Moreover, the spectral function is sensible to the “tails” of distribution.In this work, we consider the structure of the propagators in the framework of the spectral-representation approach and on account of the Dyson procedure. As was noted early, Dyson summation is not well-defined at peak range, while the spectral approach cannot be applied far from the peak. So, we have used the information which follows from both approaches in the domains of their validity. We suppose that the propagator of scalar UP in spectral representation coincides with the BW one in the intersection of their domains of definition. Using this assumption we define the spectral function of boson UP and apply it for the case of the vector UP’s propagator. We show that this strategy strictly leads to the propagators which have the structure of the modified Breit-Wigner ones (3) under the condition that the spectral function is defined for both positive and negative values of its parameter (see Section 2).The paper is organized as follows. In Section2 we present the principal elements of the approach and analyze the general structure of the scalar propagator. The expressions for vector and fermionic propagators are derived in Sections 3 and 4, respectively. Some aspects of Lagrangian formalism with unstable field ingredient and respective conclusions concerning the physical status of the results are made in Sections 5 and 6.


## 2. Propagator of Scalar Unstable Particle

The structure of propagator for the case of scalar UP can be represented in the following convolution form:(4)Dq=i∫s0∞ρm2dm2q2-m2+iϵ=i∫s0∞D0q2,m2ρm2dm2,where ρ(m2) is spectral function of the parameter m2, D0(q2,m2) is “bare” scalar propagator, and the limit of integration s0 will be determined further. Note that the symbolic expression (4) has different explicit form in various approaches. One can get a traditional Lehmann-Kallen representation for the case ρ(m2)=δ(M2-m2)+ρLK(m2), where ρLK(m2)=0 below the threshold m2<4M2. In the framework of the asymptotic free field approaches (indefinite mass) [30, 31] or the model with continuous mass [35, 36] the expression (4) can be derived directly. In these cases, the field function of scalar UP can be represented in the following convolution form:(5)ϕx=12π3/2∬ϕp,m2eipxdpωm2dm2,where p=(p,p0), ϕ(p,m2) is defined in standard way at fixed mass p2=m2 and ω(m2) is model weight function. Note that the value m is not a conventional observed mass of UP. It is continuous mass parameter which cuts out three-dimensional surface in the four-momentum space according to equality p2=m2. The canonical commutation relations contain an additional delta-function δ(m2-m′2). Starting from the standard definition of Green’s function Dq=i∫dxexp⁡-iqx0T^ϕxϕ00, where ϕ(x) is defined by (5), by straightforward calculations we get convolution representation of the model propagator (4), where ρ(m2)=ωm22.The principal problem of the approach under consideration is to define the spectral functionρ(m2). In this connection we should note the general peculiarity of the spectral approaches. From expression (4) the problem with threshold value of the spectral parameter s0 follows. Propagator of UP near the threshold q2≈s0 contains divergent at q2→s0 contributions which are compensated far from the threshold. This threshold effect is explicitly described with the help of the known integration rule(6)∫abfxdxx±iϵ=∓iπf0+P∫abfxxdx,which follows from the Sokhotski-Plemelj formula when x=0∈(a,b). In (6) P∫‍ stands for the Cauchy principal value of the integral. The threshold effect is caused by the pole at q2=s0 and will be described further in more detail.Here, we consider the special case of the spectral function for scalar UP in the assumption that the scalar propagator has a conventional BW form:(7)DBWq=1q2-M2+iMΓ.In (7), we use q-independent scheme of the width insertion and omit general factor i for simplicity. Scalar propagator in this form can be derived by Dyson summation too, if we use renormalization conditions M02=M2-RΠM2, Z-1=1+RΠ′(M2), and unitary condition ZIΠ(M2)=-M2Γ(M2) [2, 14] (note that the definitions of the Π(M2) in these references have different sign). Taking into account the abovementioned peculiarities of summation procedure, we use expression (7) as phenomenological postulate which was verified by the experiments with good accuracy. Note also that expression (7) has the same status in the framework of CMS which does not rely on the Dyson procedure. Starting from the BW expression (7) for scalar propagator, we will define the corresponding spectral function ρ(m2) and apply it to derive the expressions for the propagators of vector and spinor UP.To defineρ(m2) we rewrite (4) with the help of the integration rule (6). Then, (4) takes the form:(8)Dq=-iπρq2+P∫ρm2q2-m2dm2.The condition D(q)=DBW(q) leads to a following equalities:(9)IDq=-πρq2=-MΓq2-M22+M2Γ2,RDq=P∫ρm2dm2q2-m2=q2-M2q2-M22+M2Γ2,where the first equalities follow from (8) and the second ones from (7). From the upper equality in (9) it follows that(10)ρm2=1πMΓm2-M22+M2Γ2.Thus, the condition ID(q)=IDBW(q) uniquely defines the form of the function ρ(m2) for the case under consideration (q-independent M and Γ). In [29] the definition of the function ρ(m2) was given in close analogy with above consideration and was finished at this stage. Here, we take into consideration the lower equality of (9) which gives an additional information about the limits of integration. By straightforward calculation we can check that the lower equality of (9) and normalization of the function (10) are fulfilled exactly if (-∞<m2<∞). Inserting the expression (10) into the lower equality of (9) we get(11)RDq=MΓπP∫s0∞dm2q2-m2m2-M22+M2Γ2=MΓπQπp2d+12ln⁡q2-s02q2-s02-pq2-s0+Q+pdarctan⁡M2-s0MΓ,where Q=(q2-M2)2+M2Γ2, p=2(q2-M2), and d=2MΓ. From expression (11) it follows that the lower equality (9) is exact when s0=-∞. So, the parameter m2 can take a negative value and we have to consider an analytic continuation of the traditional spectral approach. On the other hand, the expression (11) explicitly describes abovementioned threshold effect. The second term gives a logarithmic singularity at q2→s0, where the point q2=s0 is cut out by the integration rule (6). The nature of this singularity differs from the one of the conventional threshold singularity, which takes place in OMS renormalization scheme [6, 7]. In the framework of the traditional Lehmann-like spectral approach, threshold effect is absent from the very beginning, because of ρ(m2≤s0)=0. At the same time, BW form of scalar propagator cannot be reproduced exactly in this case. In our approach, ρ(m2)>0 on the whole real axis, the threshold effect disappears at s0→-∞, and BW form is reproduced exactly. It should be noted that this effect has rather unphysical artificial nature (see, also, comments in Section 5).Let us consider the theoretical status of the result and possible consequences of the presence of negative mass parameterm2<0 in the integral representations (4) and (5). The condition D(q)=DBW(q) defines the integral equation which contains the unknown function ρ(m2) and was solved exactly. The form of the spectral function is defined strictly by the choice of the dressed scalar propagator as input condition. It should be noted that appearance of the negative component can be caused by the choice of the BW approximation. However, we do not know correct (exact) expression for the input propagator and evaluate the error of approximation. In the framework of the approaches with continuous mass, the negative component m2<0 leads to the states with imaginary mass parameters which are usually interpreted as tachyons. The problem of existence of tachyons is under considerable discussion in the last decades. The main attention is paid to the principal problems such as violation of causality, tachyon vacuum, and radiation instability. It should be noted that these problems are related to UP as an observable object with fixed imaginary mass. In the framework of the effective model [36] UP is described by the positive mass square M2 and we have no tachyons in the set of physical states.Now we evaluate the contribution of the negative component. The spectral functionρ(m2) is normalized and can be interpreted as the probability density of parameter m2. So, the probability of the negative component is as follows:(12)Pm2<0=∫-∞0ρm2;M,Γdm2≈ΓπM,ΓM≪1.From (12) it follows that this probability is proportional to the factor Γ/M which defines the finite-width effects in the processes with UP’s participation. This fact can lead to an interesting possible conclusions: tachyon instability is intrinsic property of UP; it can be interpreted as the cause of unstable particle decay. Now, we evaluate the relative contribution of the negative component to the full propagator which we define as the following relation:(13)ϵq2=∫-∞0D0q2,m2ρm2dm2∫-∞+∞D0q2,m2ρm2dm2.In expression (13) denominator is full BW propagator (7) and the integration in numerator can be performed directly at q2>0. As a result, we get(14)ϵq2;M,Γ=1πΓMq2-M2-iΓM12ln⁡q4M2M2+Γ2+πq2-M2ΓM,where we used the approximation arctan⁡(M/Γ)≈π/2 in the second term. From (14) strong q2-dependence of the relative contribution ϵ(q2;M,Γ) follows. In particular, at the peak range ϵ(M2;Γ,M)≈-iΓ2/2πM2, at q2≫M2 it has asymptotic ϵ(q2)→1, and at q2≪M2 from (13) it follows that(15)ϵq2;M,Γ=ΓπM12ln⁡M2M2+Γ2q4+πMΓ.So, at small q2, the value ϵ(q2;M,Γ) is large and we cannot cut off the negative component. At q2<0, an upper integral in (13) can be calculated with the help of the integration rule (6) and calculation gives the same effect. This effect is a direct consequence of the integration rule (6) and connected with the above-described threshold effect. Thus, the account of the negative component is essential for the case of deep virtual states of UP, that is, far from the peak range. This conclusion arises in any quantum field model with spectral representation of the propagator in form (4) and scalar propagator in BW form (7). It should be noted, however, that the status of the above given evaluations and conclusions crucially depends on the difference between the BW approximation and exact finite propagator (which, unfortunately, is unknown).


## 3. Propagator of Vector Unstable Particles

In this section, the result (10) is applied to determine the structure of vector UP’s propagator. Here, we suggest that the function ρ(m2) for boson UP (scalar and vector) is universal. Such suggestion is in accordance with the mass redefinition scheme M2=M02+RΠ(M) and relation MΓ=IΠ(M) for the case of both scalar and vector UP. First of all, we demonstrate the consistency of expression (10) for ρ(m2) and input condition D(q)=DBW(q) with the help of contour integration, which will be used in further considerations. According to (4) and (10) the propagator of scalar UP can be written as follows:(16)Dq=1π∫-∞+∞MΓdm2q2-m2+iϵm2-M22+M2Γ2.This expression can be represented in the form(17)Dq=-1π∫-∞+∞MΓdm2m2-z0m2-z+m2-z-,where z0=q2+iϵ and z±=M2±iMΓ. Analytic continuation of the integrand function in (17), where m2→z, has three poles z0, z+, and z- in the complex plane. It decreases as 1/|z|2 for z→∞; that is, it satisfies the condition fz<N/|z|1+δ for z>R0, where N and δ are positive numbers and R0→∞. So, we can apply the method of contour integration and rearrange D(q) as follows:(18)Dq=∓MΓπ∮C±dzz-z0z-z+z-z-=2πi∑kRes⁡fz,zk.In (18) k is number of the poles, Res(f(z),zk) is the residue at the pole zk, and C± is a contour in the upper (C+) or lower (C-) half of the complex z-plane. The simplest way to perform the integration is to go along the contour C- which encloses only one pole z-:(19)Dq=MΓπ∮C-dzz-z-1z-z+z-z0=2iMΓz--z+z--z0=1q2-M2+iMΓ.In (19), we have used the equality z--z+=-2iMΓ. One can check that the same result follows from the integration along the contour C+.Thus, UP can be described in the framework of two different hierarchical levels—“fundamental” level, by the integral representations (4), (5), and phenomenological one, by the effective theory after integrating out unobservable mass parameter m2 according to (19). In the framework of the effective theory, UP is described by the observed physical values M and Γ, which can always be defined as a positive quantity. So, at this phenomenological level UP has no explicit tachyonic content which could lead to the abovementioned problems. Instead, we get the term iMΓ which describes the instability in a traditional way.To define the structure of vector propagator, we assume that the spectral functionρ(m2) is the same as for a scalar UP. Using the standard vector propagator for a free vector particle with a fixed mass, we get(20)Dμνq=1π∫-∞+∞-gμν+qμqν/m2-iϵq2-m2+iϵMΓdm2m2-M22+M2Γ2.In the term qμqν/(m2-iϵ) we use the same rule of going around pole as in the denominator q2-(m2-iϵ). The integral in (20) can be evaluated with the help of formula (6); however, it is easier to do it using the method of contour integration. The integration along the lower contour C- gives(21)Dμνq=-MΓπ∮C-gμν-qμqν/z-iϵdzz-z-z-z+z-z0=-2iMΓgμν-qμqν/z-z--z+z--z0=-gμν+qμqν/M2-iMΓq2-M2+iMΓ.One can check that the integration along the upper contour C+ or with the help of the formula (7) leads to the same result. The expression (21) coincides with the well-known expression for modified BW propagator (3) which satisfies to electromagnetic Ward identity [3].We should note that both the scalar and vector propagators of UP can be represented in the form with universal complex mass squared:(22)Dq=1q2-MP2,Dμνq=-gμν+qμqν/MP2q2-MP2,where the structure MP2=M2-iMΓ usually is called complex-mass definition. This definition is the base element of the so-called complex-mass scheme of calculation [16, 17]. The dressed propagator of a bosonic UP can be formally obtained from the “free” propagator by the substitution M02-iϵ→M2-iMΓ. So, the infinitesimal value ϵ, which formally defines the rule of going around pole in bare propagator, is an analog of the infinitesimal width of the intermediate state in the framework of the model approach.


## 4. Propagator of Spinor Unstable Particles

The propagator of a free fermion can be represented in two equivalent forms:(23)D^q=1q^-m+iϵ=q^+m-iϵq2-m-iϵ2.According to the abovementioned formal rule for constructing the dressed propagator, we have to make the substitution m-iϵ→M-iΓ/2. Then, the dressed propagator of the spinor UP takes the form (3). Now, we show that the expression (3) can be derived in a more systematic way with the help of the integral representation:(24)D^q=∫q^+m-iϵq2-m-iϵ2ρmdm,where the integration range is not defined yet. The spectral function ρ(m) for fermions differs from the bosonic one, because of another parametrization M(q)=M0+RΣ(q) and Γ(q)=IΣ(q). The spectral function for the case of the spinor UP is as follows:(25)ρm=1πΓ/2m-M2+Γ2/4=1πΓ/2m-M-m-M+,where M±=M±iΓ/2. The main difference between boson and spinor cases is a presence of the linear term m instead the quadratic one m2, which is defined at the whole real axis m2∈(-∞,+∞). Here, we consider a straightforward relation between the bosonic parameter range and spinor one. Thus, we have two intervals, namely, (+i∞,i0;0,∞) and (-i∞,i0;0,∞), for the value m. In the method of contour integration the signs ± correspond to integration along the contours C±, which enclose the first or fourth quadrants of the complex plane. Then, from (24) and (25) it follows that(26)D^±q=±Γ2π∫C±q^+zdzz2-z02z-z-z-z+,where z02=q2+iϵ, z±=M±, and C± are the above described contours. By simple and straightforward calculations we can see that the correct result follows from the integration along the contour C-, while the integration along the C+ leads to nonphysical result. This is likely caused by the presence of the branch point z02 in the first quadrant. From (26) it follows that(27)D^-q=-Γ2π∫C-dzz-z-q^+zz2-z02z-z+=-iΓqq^+z-z-2-z02z--z+=q^+M-iΓ/2q2-M-iΓ/22.The last expression in (27) coincides with the corresponding expression in (3). The spinor complex-mass definition differs from the bosonic one; however, it has similar pole-type complex structure. Then, the pole definition of the mass and width of the spinor UP is MP=Mρ-iΓρ/2 in our consideration.


## 5. Complex-Mass Scheme in Effective Theory

The main result of the previous two sections is the modified BW expressions (3) derived in analytical way. We have showed also the connection between scalar, vector, and spinor propagator with the help of the spectral approach. Note that the analogous connection takes place for the case of free fields, that is, for the stable particle approximation [37]:(28)Dikx=gik+1M2∂2∂i∂kDx=12π4∫gik-kikk/M2e-ikxk2-M2dk,D^x=i∂^+MDx=12π4∫k^+Mk2-M2e-ikxdk.In (28) the value M2=M02-iϵ and D(x) is scalar casual function, that is, propagator in coordinate representation for free scalar field Φ(x), which satisfies to Klein-Gordon equation:(29)∂k∂k-M2Φx=0.We have derived just the same expressions for the case of dressed propagators in the momentum representation, that is, for complex massM=MP, which should be inserted into Lagrangian (vertexes, sin2θW, etc.) and into motion equation (29). In such way, we have come to the so-called complex-mass scheme of calculation [16–18], which is realized at Lagrangian level of effective theory. It should be noted that free casual functions Dik(x) and D^(x), which are defined by (28), in analogy with scalar one can be represented as vacuum expectation value of chronological field operator product [37]:(30)Dikx-y=i0Tϕixϕky0,D^x-y=i0Tψxψ¯y0.As it was shown in Section 2, the scalar field function can be redefined according to (5) with weight function ω(m2)=±ρ(m2) which leads to BW propagator. The same redefinition can be done for the case of vector and spinor UP, which provides the validity of (30). So, we have effective theory which has some principal properties of fundamental quantum field theory. As was noted in Section 3, UP can be described at two hierarchical levels, fundamental one and phenomenological one (after integrating out unobservable mass parameter m2). In the case under consideration, the phenomenological approach corresponds to the effective theory, which can be represented at lowest order by the Lagrangian with complex masses. The effective field function, which describes UP, is defined in a correspondence with the conventional definition of Green’s function.The problems of renormalization procedure in the effective theory arise at next-to-leading order. To date there is no fully established treatment of UP within perturbation theory, although many solutions have been proposed [18]. For instance, the unitarity in scalar field theories was studied within the framework of the CMS [18] at one-loop approximation. Evidently, the effective field function of UP is formed by self-energy contribution at fundamental level and contains corresponding information about mass and width of UP. In the case under consideration, this information is included into spectral function ρ(m2;M,Γ). So, we have to avoid double counting of self-energy contribution in the calculations at loop level of the effective theory. Just this contribution stipulates the divergence of renormalization constant at threshold M→2MV, where the vectors are in the self-energy loop [20]. Thus, we do not deal with the conventional TS in the framework of the effective theory. As was shown in Section 2, the problem of TS appears at the leading order, and its nature differs from the conventional one. It should be noted, however, that mathematically strict status of our consideration is due to appearance of the negative spectral component which has no clear physical meaning.


## 6. Conclusions

The definitions of the mass and width of UP, as a rule, are closely connected with the construction of the dressed propagators. It was underlined in this work that traditional approaches, which are based on the Dyson procedure and spectral representation, have formally crucial peculiarities. We have considered the structure of the propagators of UP in the phenomenological approach which is based on the spectral representation. The spectral function describes the distribution of continuous (indefinite, smeared) mass parameter, contains a principal information concerning UP, and defines a spectral structure of the propagators.In this work, we have analyzed a special case of the spectral function which follows from matching the model and standard scalar BW propagator. This function contains the parametersM,Γ and mass variable m2 proven to be in the interval (-∞,+∞). So, the variable m can be imaginary; however, such states have no explicit physical content. It was shown that contribution of the negative component to the full propagator is significant for the deep virtual states. In the framework of this approach we get vector and spinor propagators with the well-known modified BW structure. This structure provides the gauge invariant description and explicitly leads to the complex-mass definition. The q-dependence of the UP mass and width can be introduced into the function ρ(m2;Γ(q),M(q)) without the loss of the generality. We formulated some problematical aspects of the propagators construction which require an additional analysis.



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