KNO and Polyakov's multiplicity scaling in inelastic pp- and pp -collisions at superhigh energies

It is shown that the normalized Saleh-Teich's multiplicity charged particles distribution in inelastic pp- and pp-collisions describes the KNO scaling low in soft processes (the range of ISR energies) and can be exhibited as Polyakov's scaling low in hard processes ( (√s >> 1800 GeV)...

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Datum:2001
Hauptverfasser: Rusov, V.D., Zelentsova, T.N., Kosenko, S.I., Ovsyanko, M.M., Sharf, I.V.
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Veröffentlicht: Національний науковий центр «Харківський фізико-технічний інститут» НАН України 2001
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Zitieren:KNO and Polyakov's multiplicity scaling in inelastic pp- and pp -collisions at superhigh energies / V.D. Rusov, T.N. Zelentsova, S.I. Kosenko, M.M. Ovsyanko, I.V. Sharf // Вопросы атомной науки и техники. — 2001. — № 6. — С. 161-166. — Бібліогр.: 21 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Rusov, V.D.
Zelentsova, T.N.
Kosenko, S.I.
Ovsyanko, M.M.
Sharf, I.V.
author_facet Rusov, V.D.
Zelentsova, T.N.
Kosenko, S.I.
Ovsyanko, M.M.
Sharf, I.V.
citation_txt KNO and Polyakov's multiplicity scaling in inelastic pp- and pp -collisions at superhigh energies / V.D. Rusov, T.N. Zelentsova, S.I. Kosenko, M.M. Ovsyanko, I.V. Sharf // Вопросы атомной науки и техники. — 2001. — № 6. — С. 161-166. — Бібліогр.: 21 назв. — англ.
collection DSpace DC
container_title Вопросы атомной науки и техники
description It is shown that the normalized Saleh-Teich's multiplicity charged particles distribution in inelastic pp- and pp-collisions describes the KNO scaling low in soft processes (the range of ISR energies) and can be exhibited as Polyakov's scaling low in hard processes ( (√s >> 1800 GeV) but in any case the multiplicity scaling is always violated in the range of Sp − pS energies. It is supposed that the increase of transverse momentuma (or, what is the same, increase of phase volume) is the reason of the violation of any type scaling in the range of Sp − pS energies, when the part of semi-hard processes is essentially increased.
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fulltext KNO AND POLYAKOV'S MULTIPLICITY SCALING IN INELASTIC pp - AND pp - COLLISIONS AT SUPERHIGH ENERGIES V.D. Rusov, T.N. Zelentsova, S.I. Kosenko, M.M. Ovsyanko, I.V. Sharf Odessa National Polytechnic University, Odessa, Ukraine e-mail: siiis@te.net.ua It is shown that the normalized Saleh-Teich's multiplicity charged particles distribution in inelastic pp- and pp- collisions describes the KNO scaling low in soft processes (the range of ISR energies) and can be exhibited as Polyakov's scaling low in hard processes (√s >> 1800 GeV) but in any case the multiplicity scaling is always viol- ated in the range of pSpS − energies. It is supposed that the increase of transverse momentuma (or, what is the same, increase of phase volume) is the reason of the violation of any type scaling in the range of pSpS − energies, when the part of semi-hard processes is essentially increased. PACS: 13.85.-t;12.40.Ee;25.40.Ep 1. INTRODUCTION As its shown in [1], the multiplicity charged particles distributions in inelastic pp- and pp-collisions in all the range of ISR- and pSpS − energies up to en- ergy of Fer-milab tevatron collider are well described by Salech-Teich’s three-parametrical distribution. The ST- distri-bution is obtained in the supposition that on the first stage of interaction (which is described by homo- geneous Poisson process) the random number of primary particles <ν> (partons, pomerons, strings, etc.) in the impact parameters bt space1 is produced, and on the secondary stage each of primary particles generates inhomogeneous Poisson process of a random number of secondary particles <ε> («grey» hadrons) production on characteristic length <∆b> equal to average length of parton chain (or, in other words, characteristic length of hadron jet formation). Thus the decolouration of «grey» hadrons happens on the interval of impact parameters [0, R], where R is average so-called radius of interaction of primary particles [2]. We won't show here bulky expressions of Saleh- Teich’s three-parametrical distribution [1]. Let us note that identification and quantitative analysis of appropri- ate parameters of experimental charged particles distri- butions in hadron-hadron collisions is reduced to the de- termination of parametrical triplet R/<∆b>, <ε>, <ν>} by solution of the system of the nonlinear equations for 1 In impact parameters representation the naïve model [1] has such physical singularities. The Eq. (4) in [1] is the convolution of the func- tion of hadron production on the interval [0, R] (in terms of present paper), which can be re-written as: )()()(,)()()( RbububHdbbbhbHbh ttttttttR −−=′+⋅=′ ∫ ∞ ∞− where u(bt) is single Heaviside function. In this expression the physi- cal interpretation of the «step» H(bt) consists in the fact that in impact parameters space it represents a model image of real function, i.e. overlap function Gin under condition of unitary limit (Gin≤1) at s→∞. Then the maximum value of bt is meaningful of radius of primary par- ticles interaction R. ST-distribution moments, which are explicitly con- sidered in Ref. [3]. As result of the analysis of fitting data (collected in Table) of AВCDHW [4], UA5 [5], CDF [6] Collabora- tions experimental multiplicity distribution the follow- ing empirical dependences of the ST-distribution para- meters are obtained: ∆2 ~ sn , (1) ( ) ( )                 ∆ −−× ×−+        ∆ −⋅+ ∆ b b R sRs 2exp1 8.2ln11.12exp10066.0~ 2 ε (2) 1 42 41.023.123.1~ − ∆∆           +    +    − ∆ γγ γ ccb s s s sR , (3) where ∆ = 0.212, γ = (s – sc)/|s - sc|, √sc = 770 GeV. In a way, the asymptotic expressions (1)-(3) make it possible to consider the three-parametrical ST-distribu- tion as "one-parametrical" multiplicity distribution P(n,s), where the role of the parameter plays collision energy s. Hence naturally suggests the idea to verify the known hypothesis of the asymptotic scaling behavior of multiplicity distributions [7,8] : ( )         = )()( 1, sn n sn snP ψ , (4) which is widely known as KNO scaling of the multipli- city distributions. For the first time such form of P(n, s) was derived within the framework of the conformal theories in the paper by Polyakov [7] as consequence for the strong in- teractions of hadrons of the application of three ideas - unitarity, analyticity and similarity. The similarity hypo- PROBLEMS OF ATOMIC SCIENCE AND TECHNOLOGY. 2001, № 6, p. 161-166. 161 mailto:siiis@te.net thesis, i.e. hypothesis of asymptotic scale invariance (which was induced by "strong coupling" regime in the Pomeranchuk pole problem [9]) reduces both to scaling form of secondary particles distribution (4) and to the fact that the average multiplicity of hadrons in strong in- teractions at small distances is power-law function of collision energy s: ( ) ∆∝ 2ssn . (5) The same form of P(n, s) was obtained by Koba, Nielsen and Olesen [8], but it was based on Feynman's scaling [10]. The Feyman's model notions about high- energy collisions of hadrons (including the suppositions of transverse momentuma limitation of produced particles and the independence of Feynman's functions on collision energy) led the authors [8] both to scaling form of secondary particles distribution (4) and to the fact that the average multiplicity of hadrons in strong in- teractions at large distances is logarithmic function of collision energy s: ssn ln)( ∝ . (6) Let us add that in strong interactions at large dis- tances the dependence (5) was obtained earlier within frameworks of Regge phenomenology [11] and also in multiperipheral models [12]. The purpose of the given research are the study and designing of the properties of normalized multiplicity ST-distribution, which satisfy to condition of similarity in strong interactions at small distances (Polyakov's scaling) and at large distances (KNO scaling). 2. PHENOMENOLOGY OF ASYMPTOTICAL BEHAVIOR 0F NAIVE MODEL PARAMETERS Here we will consider in what degree qualitative and quantitative aspects of asymptotical behavior of expres- sions (1)-(3) at energies √s ≥ 900 GeV meet to relevant physical mechanisms. We understand relevance as a such asymptotic properties of parameters (1)-(3), which ensure not only optimum fits of experimental date in the energy range √s = 20÷1800 GeV, but also make it pos- sible physically grounded to simulate the probable beha- vior of multiplicity secondary particle distributions, which could be obtained in the future researches at vari- ous ultrahigh energies [1]. First of all it concerns the physical substantiation of evolution of the parameters <∆b>, R and their ratio (3) with the energy √s growth (because an asymptotical be- havior of other two parameters (1) and (2) is well known and are explicitly considered in Sec. 3 and 4 ac- cordingly). So, let us consider the phenomenology of the para- meter (3) evolution at increasing of collision energy √s. Now it is already indisputable that the semi-hard processes (i.e. production of hadron mini-jets with relat- ive large characteristic transverse momenta but with small part of an initial energy x<<1 [2, 13, 14]) become the main source of secondary particles at increasing of the collision energy. Such picture of hadron high ener- getic collisions was unusual for a long time because it was considered that dominating source of secondary particles were the soft processes. In particular, it con- cerns the pSpS energy range, where strong interactions at small distances become essential and where the QCD perturbation theory is true. Levin and Ryskin have shown [15] that the estima- tion of radius of interaction R0 calculated in frameworks of LLA QCD at certain value of scale of cutting (Q0) on transverse momentuma p⊥ has following form: [ ] 41 0 0 2954.0~ n Q R , (7) where factor 2 takes into account the fact that in our model the average multiplicity of secondary particles <n> is considered not for all charged particles but for a number of meson pairs [1]. It follows that R0=21/4R. On the other hand, the ratio R/<∆b> jumping varies at energy 900 GeV (see Table 1), and at the subsequent increase of energy the area of indeterminacy <∆b> of hadron production (in one mini-jet) in the impact para- meters space becomes essential small value in compar- ison with radius of interaction, i.e. R >> <∆b>. It means that just hard processes play decisive role at energy √s ≥ 900 GeV. Then taking into account that, on the one hand, p⊥⋅<∆b> ~1 and, on the other hand, that the con- sideration of the distribution of meson pairs numbers gives a value of effective transverse moment equal to p⊥ ≥2Q0, we have following an expression (with allowance for (7)) for hard processes: GeVsfornR b 900908.1 41 ≥⋅≥ ∆ . (8) Thus the expression (8) qualitatively and quantitat- ively reflects velocity gradient of ratio R/<∆b> (3) at ul- trahigh energies starting from √s = 900 GeV and it's also completely determined by the value of average multiplicity <n> of secondary particles. It means, in it's turn, that multiplicity ST-distribution becomes practic- ally two-parametrical at energies √s ≥ 900 GeV, i.e. it depends only on average multiplicity <n> and average multiplicity <ε> in one mini-jet. 3. POLYAKOV'S SCALING In terms of moments the homogeneous form of dis- tribution P(n,s) in (4) means the independence of nor- malized algebraic moments on collision energy s ∑== n qqqq q PnnwherennC , . (9) For clear understanding of the strategy of designing of the properties of normalized ST-distribution, which sat- isfies to conditions of similarity hypothesis in strong in- teractions at small distances, let's consider the asymptot- ic properties of second normalized algebraic moment of ST-distribution: 162 Table 1. Parameters of multiplicity ST-distributions obtained by fitting of experimental data and predicted by our naive model Experiment √s, GeV <n> <ε> R/<∆b> χ2/NDF pp – collisions ABCDHW Collaboration [4] 30.4 5.27 4.8 0.03 6/13 ABCDHW Collaboration [4] 44.5 6.04 5.5 0.05 6/15 ABCDHW Collaboration [4] 52.6 6.38 5.8 0.06 4/17 ABCDHW Collaboration [4] 62.2 6.81 6.2 0.07 3/16 −pp collisions UA5 Ansorge et.al. [5] 200 10.70 8.3 0.22 47/34 UA5 Alner et.al. [5] 546 14.55 10.4 0.37 63/56 UA5 Ansorge et.al. [5] 900 17.80 12.3 6.80 52/52 CDF [6] 1800 24.00 16.3 4.22 135/97 Predictions of naïve model - 2400 27.1 18.2 4.35 - - 6000 40.0 26.6 4.80 - - 14000 57.3 37.9 5.25 - - 100000 131.8 53.7 6.47 - - 200000 176.9 116.7 6.96 -         > > ∆ + + < < ∆ ∆ + + =+== .1, 1 1 ;1, 1 1)var(1 22 2 2 b b b R n R n R n n n n C ε ε (10) where as var (n) Eq. (11) from Ref. [1] is used. As it show the analysis of fitting data (Table), the values of ratio (R/<∆b>) are practically identical in all the range of ISR energies and monotonically increase in all the range of pSpS -energies up to energy √s = 1800 GeV. The asymptotic tendency of second moment (10) to constant value at energies over √s = 1800 GeV is stipulated by an identical asymptotic of <n> and <ε>. It means that if average multiplicity in hadron mini-jet <ε > and total average multiplicity of hadrons <n> behave uniformly (i.e., according to Polyakov [7], they are power-law functions of energy) the Polyakov's scaling must be observed in the range of ISR energies (where R/ <∆b> << 1) and can be observed at energies much above √s = 1800 GeV (where R/<∆b> >> 1). The power-law dependence of average total hadron multiplicity on energy (4) is practically beyond doubt. This is confirmed by experimental data in the range √s = 20-1800 GeV presented in Table. At the same time the analogous statement, which concerning the average multiplicity in hadron mini-jet <ε>, is rather ambiguous. Within the framework of existing experimental data, <ε > can be fitted both by logarithmic and by power-law dependence on energy. The mixed variant of these de- pendences with specified "survival" one of them in the limit of high energies is also possible. For instance, such mixed empirical dependence (which is almost «mirror» concerning Eq.(5)): ( )                 ∆ −−+⋅+ +        ∆ −⋅− ∆ b b Rs Rs exp110066.0 exp)8.2ln11.1(~ 2 ε , (11) describes the appropriate values <ε> as good as Eq. (5) (see Table), but this dependence asymptotically tends to power-law dependence at energies over √s = 900 Gev (R/<∆b> >>1), i.e., <ε> ~ s∆ with s → ∞. Explanation of power-low behavior of average mul- tiplicity in the jet <ε> is following. In 1968 Gribov and Migdal [9], considering the problem of the interaction of reggeons, showed that one possibility is "strong coupling" case in which the many-particle Green's func- tions are power-low, not logarithmic, functions of their arguments. On the other hand, as Polyakov has noted [7], the power-low asymptotic forms of the Green's functions at large momentumа mean that the theory has invariance with a respect to change of the space-time scale, which is manifested at very small distances. Thus the similarity hypothesis in the strong interaction at small distances reduces to power-low asymptotics of the average hadron multiplicity in the jet [7], i.e., <ε> ~ const⋅ s∆. In a way, the physical content of Eq. (8) is clear. In soft hadron-hadron collisions (i.e., in strong interactions a) b) c) d) Fig. 1. Normalized multiplicity ST-distribution for the non single-diffractive pp- and pp-collisions shows the validity of KNO scaling in soft processes (a) and predicts the approximate validity of Polyakov's scaling in semi- hard (c), hard processes (d) and strongly violation of any type scaling in the range of pSpS -energies (b) L ((R/<∆b>)<< 1), but in semi-hard and hard hadron- hadron collisions (i.e., in strong interactions at small distances) the power-law physics "survives "((R/<∆b>) > > 1). et us consider the behavior of Polyakov's scaling in the energy range √s = 0.03 - 100 TeV. For this purpose we used the values obtained by fitting of experimental distribution of secondary particles on energy interval √ s= 0.03 - 1.8 TeV and theoretically predicted by empir- ical expressions (1), (8) and (11) at asymptotically high energies (see Table) as the parameters of three-paramet- rical ST-distribution. The research of properties of such normalized ST-distribution (which satisfy to conditions of the similarity hypothesis in strong interactions at small distances) has shown an anomalous behavior of Polyakov's multiplicity scaling of charged particles pro- duced in hadron collisions. Scaling is valid inthe range of ISR energies (Fig.1а), it is approximately valid at su- perhigh energies starting from the energy √s = 100 TeV (Fig. 1d) and it is completely violated in pSpS energy range √s = 200-1800 GeV (Fig. 1b). In the energy range s2-100 TeV slow but stable tendency to scaling is ob- served (Fig. 1с). The analysis of multiplicity distributions parameters (Table 1) and expressions (1) and (11) shows that the parameters <n> and <ε> are monotone increasing power-law functions of energy, whereas the parameter R/<∆b> jumping increase just in the energy range √ s=200-1800 GeV. It is experimentally shown that an av- erage radius of inelastic interactions R is increased in- significantly on energy in the range 200-1800 GeV and is on interval R~<bt 2>1/2= 0.9-1.1 Fm [16]. The theoretical estimation of average radius of in- elastic interaction (7) is calculated in LLA of QCD for d large transverse momenta [15] and satisfactorily de- scribes known experimental data for semi-hard pro- cesses [16]. Hence, the nature of R/<∆b> change on en- ergy interval √s = 200-1800 GeV allows to conclude that the sharp decreasing of average length of parton chain <∆b> is main reason of total violation of Polyakov's scaling. Such sharp decrease of <∆b>, which is accompanied by the simultaneous increase of average hadron multiplicity in mini-jet <ε>, point out the sharp increase of parton density in the chain. This, in its turn, means that the increase of multiplicity in mini-jet hap- pens only due to the increase of transverse momentum, i.e. directly due to increase of phase volume [2]. Thus, it is possible to assume that significant increase of phase volume in semi-hard processes is the reason of total vi- olation of Polyakov's scaling. Let's consider the mathematical interpretation of Polyakov's scaling violation in energy range √s=200- 1800 GeV. It is easy to show that with (<ε>R/<∆b>)→0 ST-distribution asymptotically transforms to Poisson distribution and with (R/<∆b>) >>1 it transforms to Ney- man type A distribution from two parameters <n> and < ε> [3, 17]: ( )∑ ∞ =                 −        ⋅−= 0 exp ! 1exp ! )( )( k kn nn k k n k nP εε ε ε , (12) which exactly coincides with compound Poisson distri- bution [18]. Hence, the jumping increase of parameter R/<∆b> from 0.22 to 6.8 (see Table) in indicated energy range leads to the fact that the ST-distribution (by virtue of its asymptotic properties on parameter R/<∆b> [3, 17]) sharply changes its type and structure, i.e., it changes Poisson (one-humped) type at R/<∆b> <<1 to Neyman (multi-humped) type at R/<∆b> >>1 [3, 17]. Thus, such an asymptotic transition causes the loss of self-similarity of distribution function, and this is the reason of Polyakov's scaling violation. Physically it usu- ally means the change of phase states of researched sys- tem on parameter R/<∆b>. A test of the scaling hypothesis is provided by an ex- amination of energy dependence of the moments of the distribution. The moments C2-5 for the non-single-dif- fractive events are shown in Fig. 2. The behavior of moments confirms our expectations concerning to anomalous behavior of Polyakov's scaling (Fig. 1) and, what is especially important, total equiva- lence of Polyakov's scaling and normalized Neyman type A distribution (12) in the limit of high energies (over 100 TeV) (see Fig. 1d). 4. KNO SCALING As it was noted above, KNO scaling grows out of the approach based on similarity hypothesis in strong in- teractions at large distances, and, in a way, it reflects the self-similar properties of logarithmic physics. The au- thors of Ref. [8] accent attention just to such properties. They written that theirs' result "... can be expressed by the saying that the normalized multiplicity distribution keeps its form independently of the beam energy and just scales up as lns" [8]. Fig. 2. Values of the first four C-moments for the non single-diffractive ST-distributions as a function of the center of mass energy. The values of C-moments at ISR-, pSpS -energies and at √s=1800 GeV are given in Refs. [4], [5], [13], accordingly The asymptotic analysis of algebraic moments (6) of ST-distributions (and, in particular, an example of an asymptotic dependence of normalized second moment (10) on collision energy s) presented in Sec. 3 allows to make the conclusion concerning to KNO scaling also. If the average multiplicity in hadron mini-jet <ε> and total average multiplicity of hadrons <n> behave uniformly (for instance, they both are logarithmic functions of en- ergy), then KNO scaling must be observed in the ISR energy range (where R/<∆b> <<1) and can be observed at energies over √s >> 1800 GeV (where R/<∆b> >> 1). However, as it shown above (see Table), the average hadron multiplicity <n> is power-law function of colli- sion energy s, i.e. <n>~s∆ at s→∞. Then, if the average hadron multiplicity in mini-jet <ε> is logarithmic depen- dence on collision energy (for example, such as Eq. (2)), KNO scaling must be observed in the range of ISR-en- ergies and always must be violated at energies over ISR- energies. Such asymptotic of <ε> and <n> and also the reasons of KNO scaling violation are typical, for exam- ple, in different versions of dual parton model and quark-gluon strings model [19], which met with consid- erable success in describing and, in some cases, predict- ing the main feature of low-pT physics at ISR and collid- er energies [20]. In our case, in spite of the fact that the parameters <n> and <ε> have different functional forms on collision en- ergy s, KNO scaling really satisfies to a good accuracy in the range of ISR-energies (and practically does not differ from Fig. 1а); however as energy increases KNO scaling is strongly violated. The validity of KNO scal- ing in the ISR energy range is explained by the fact that the asymptotic expressions for <n> and <ε> (though they have power-law and logarithmic forms of the de- pendence on collision energy s) are close in this energy range and insignificantly vary with energy growth. 5. CONCLUSIONS The basic result of the present work consists in that the normalized multiplicity ST-distribution describes KNO scaling in soft processes and can be exhibited as Polyakov's scaling in hard processes. We assume that the increase of transverse momentuma (or what is the same, increase of phase volume) is the reason of the vi- olation of any type scaling low in the range of pSpS - energies, where the part of semi-hard processes is essen- tially increased. If further collider pp-experiments at energies s >>1800 will prove the Polyakov's scaling existence, then, firstly, the importance of true reasons of any type scaling violation in area of pSpS -energies can be scarcely exaggerated, and, secondly, the very important answer to very old question: «Could it be that as in the theory of critical phenomena, while the basic physics (Hamiltonians) between e+e- annigilation and hadronic multiparticle production could be entirely different, multiplicity scaling may yet still be a universal feature shared by both ?» [21] can be obtained. REFERENCES 1. V.D. Rusov, T.N. Zelentsova, S.I. Kosenko, M.M. Ovsyanko, I.V. Sharf. Cascade parametriza- tion of multiplicity distributions in inelastic pp- and pp -interactions of energy interval in c.m.s. √ s=20-1800 GeV // Phys. Lett. 2001, v. B504, p. 213-217. 2. E.M. Levin, M.G. Ryskin. Growth of total cross-sections of hadron interactions at energy in- ceasing // Usp. Fis. 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id nasplib_isofts_kiev_ua-123456789-79477
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
issn 1562-6016
language English
last_indexed 2025-12-02T06:10:36Z
publishDate 2001
publisher Національний науковий центр «Харківський фізико-технічний інститут» НАН України
record_format dspace
spelling Rusov, V.D.
Zelentsova, T.N.
Kosenko, S.I.
Ovsyanko, M.M.
Sharf, I.V.
2015-04-02T15:21:10Z
2015-04-02T15:21:10Z
2001
KNO and Polyakov's multiplicity scaling in inelastic pp- and pp -collisions at superhigh energies / V.D. Rusov, T.N. Zelentsova, S.I. Kosenko, M.M. Ovsyanko, I.V. Sharf // Вопросы атомной науки и техники. — 2001. — № 6. — С. 161-166. — Бібліогр.: 21 назв. — англ.
1562-6016
PACS: 13.85.-t;12.40.Ee;25.40.Ep
https://nasplib.isofts.kiev.ua/handle/123456789/79477
It is shown that the normalized Saleh-Teich's multiplicity charged particles distribution in inelastic pp- and pp-collisions describes the KNO scaling low in soft processes (the range of ISR energies) and can be exhibited as Polyakov's scaling low in hard processes ( (√s >> 1800 GeV) but in any case the multiplicity scaling is always violated in the range of Sp − pS energies. It is supposed that the increase of transverse momentuma (or, what is the same, increase of phase volume) is the reason of the violation of any type scaling in the range of Sp − pS energies, when the part of semi-hard processes is essentially increased.
en
Національний науковий центр «Харківський фізико-технічний інститут» НАН України
Вопросы атомной науки и техники
Electrodynamics of high energies in matter and strong fields
KNO and Polyakov's multiplicity scaling in inelastic pp- and pp -collisions at superhigh energies
KNO и поляковский законы скейлинга множественности в неупругих pp- и pp-столкновениях при сверхвысоких энергиях
Article
published earlier
spellingShingle KNO and Polyakov's multiplicity scaling in inelastic pp- and pp -collisions at superhigh energies
Rusov, V.D.
Zelentsova, T.N.
Kosenko, S.I.
Ovsyanko, M.M.
Sharf, I.V.
Electrodynamics of high energies in matter and strong fields
title KNO and Polyakov's multiplicity scaling in inelastic pp- and pp -collisions at superhigh energies
title_alt KNO и поляковский законы скейлинга множественности в неупругих pp- и pp-столкновениях при сверхвысоких энергиях
title_full KNO and Polyakov's multiplicity scaling in inelastic pp- and pp -collisions at superhigh energies
title_fullStr KNO and Polyakov's multiplicity scaling in inelastic pp- and pp -collisions at superhigh energies
title_full_unstemmed KNO and Polyakov's multiplicity scaling in inelastic pp- and pp -collisions at superhigh energies
title_short KNO and Polyakov's multiplicity scaling in inelastic pp- and pp -collisions at superhigh energies
title_sort kno and polyakov's multiplicity scaling in inelastic pp- and pp -collisions at superhigh energies
topic Electrodynamics of high energies in matter and strong fields
topic_facet Electrodynamics of high energies in matter and strong fields
url https://nasplib.isofts.kiev.ua/handle/123456789/79477
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