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393

THE STRUCTURE OF THE POMERON

P V Landshoff CERN, Geneva *

ABSTRACT

The phenomenology of pomeron exchange, which controls total hadronic cross-sections, elastic scattering and diffraction dissociation, is surprisingly simple and has resulted in several successful predictions. Among these are the size of the total cross-section and the shape of the forward elastic-scattering peak at energy, and the pomeron structure function recently measured at the CERN collider.

*On leave from DAMTP, University of Cambridge 394

1. INTRODUCTION My talk is about the long-range at high energy. Its phenomenol­ ogy is surprisingly simple and is described by pomeron exchange between [1l . This has made possible a number of predictions, which have subsequently been verified by experiment. In the short time I have available I shall briefly discuss these three topics: Total cross-sections for -hadron and -hadron scattering • The forward peak in pp and pp elastic scattering • Diffraction dissociation and the pomeron structure function. • It is a difficult but very interesting theoretical problem to understand why the phenomenology of pomeron exchange should be so simple. It is now rather sure that pomeron exchange occurs between single quarks and is just exchange. The sim­ plest approximation to it is the diagram of figure 1. Notice, though, that this is only an approximation and so it has to be used with care and intelligence; for example figure 1 gives no variation with the energy s and so a Regge factor s"'(t) has to be added by hand. Figure 1 approximates well to experiment only if the that are exchanged have propagators t):iat are nonperturbative!2l . They must not have a pole at k2 0. This pole is removed by the confinement mechanism; if it were present gluons would= be able to propagate through infinitely large distances. Thus pomeron exchange is a nonperturbative mechanism. Recently, there has been a lot of interest in the possibility that there might be also a purely perturbative pomeron!3l. If this does exist it should become apparent in semi-hard processes. So far, however, experiment has not revealed it, and the processes I shall talk about are all controlled by nonperturbative pomeron exchange.

2. TOTAL CROSS-SECTIONS Figure 2 shows data for the pp and pp total cross-sections. The curves date from 1985, before the measurement by the E710 experiment at the Tevatron. Other people expected that the cross-section at the Tevatron would be about 10 mb higher, so our prediction is something of a success for simple . The curves in the figure correspond to

u(pp) - u(pp) 70s-0 56 = u(pp) + u(pp)] l50s-056 + 22.7s' �[ = (I) Here, the terms s-0·56 correspond to the exchange-degenerate Ji, a2 trajectory and are a standard consequence of Regge theory. They are largep, w, at low energy and provide the initial fall with increasing energy seen in the data. The term ' provides the rising part of the curves. is an effective power because it decreases withs increasing E s, but only very slowly. We need 0.08 (2) E ::::::

The reason that varies with is that the term ' represents a mixture of effects. E s s At present energies the main one is single-pomeron exchange, which behaves something 395 like s0·086• The power closer to 0.08 is obtained by adding in double-pomeron exchange, which is negative and at CERN collider energy decreases the total cross-section by about 10%. At higher energies the contribution from double-pomeron exchange will become relatively larger. Eventually, one will also have to take account of the exchange of more than two pomerons (though up till now this seems to be unimportant), until at asymptotic energies an effective power s' is not a good representation and instead the Froissart bound log2 s is saturated. But we will never reach such asymptotic energies and, in this sense, the Froissart bound is irrelevant. (It is amusing that predictionsl41 based on a belief that the Froissart bound is relevant at present energies yielded a much higher prediction for the Tevatron energy.)

E710

70

60 .0 E

AD + PVL

Figurel 1985 Exchange of nonperturbative gluons between quarks

Figure 2

pp and pp total cross-section data. The curve is the 1985 prediction of reference 1 Notice that the same steadily-rising component s' is present the way from.Js all = 5 GeV to .Js 1800 GeV. This is remarkable, when one realises that sorts of things are produced =at 1800 GeV, particularly minijets, which cannot be producedall at 5 GeV. The total cross-section does not notice this new production and is smooth: as new final states come in, old ones are correspondingly reduced. 396

Fits exactly similar to (1) may be applied to other total cross-sections. For example[5] Hu(7r+) + u(7r-)] 46s-0 56 + l4s' (3) = with the same f. It is significant that the ratio 14/22.7 of the s' terms is very close to 2/3. This is a sign that the pomeron couples to single valence quarks in a hadron (the additive rule). The additive quark rule extends very well to total cross-sections that involve containing strange quarks provided one allows for the fact that strange quarks apparently scatter more weakly:

u(su) �u(uu) (4) �

For real scattering on a we have made the fit[l]

u(rp) = ll5E-o 56 + 74E' (5)

The data are not good enough to constrain the coefficients here very accurately. How­ ever, (5) predicts something like 170 µb at Js 250 GeV. It will be interesting to measure this at HERA because there have been other= predictions that are very much higher[6l , even up .to 250 µb. Such predictions are based on the supposition that the onset of minijet production will lead to a significant increase. As we have seen, this has not happened with pp scattering.

3. ELASTIC SCATTERING When one considers all the available data for total cross-sections, elastic scattering and diffraction dissociation, the following phenomenological facts about the pomeron become apparent[1l: It is rather like a C = + 1 isoscalar photon • It couples to single quarks • It is a simple Regge pole. • The Regge trajectory of the pomeron is found to be

a(t) = 1 + + a'(t) (6) Eo The value of fo is somewhere between 0.085 and 0.9, while a' is very close to 0.25 Gev-2 , with an error of perhaps ±0.01 Gev-2 or less. When one considers pp or pp scattering, wave-function effects require the intro­ duction of a Dirac form factor F1 ( t), just as in ep scattering. The contribution from single pomeron exchange is

=constant 2 - (7) �: [F1 (t)]4s "(t) z For want of any better knowledge we take the same form factor F1 (t) as has been mea­ sured in ep scattering, and this seems to work well. _(There is no contribution from the other Dirac form factor F2(t), because apparently pomeron exchange does not flip the 397

hadron's helicity.) In order to compare with data we have to add in to (7) the cor­ rection corresponding to two-pomeron exchange, which is relatively small. Comparing the result with very-small-t data at Js 53 GeV determines a', and we then have an excellent fit to all ISR data out to values= of ltl of about 0.7. The same fit[1l , with no adjustment since 1985 to the small number of parameters, correctly describes the recent l l Tevatron data 7 (figure 3). This is something of a triumph for Regge theory, which correctly predicted the change of exponential slope of about 3.5 units compared with ISR energies. Single-pomeron exchange gives a change of slope equal to Ll(2a'log s), though there is a small correction because of the two-pomeron exchange. It would be very interesting to discuss the shape of the curve for the larger values of ltl in figure 3, but there is no time for this. I hope that one day there will be data!

102

101 "'� u ° > 10 Q) �

.0 10-1 .s

15 0 "O

10-3

10-4 0 0.5 1.0 1.5 I t I Figure 3

data for pp elastic scattering at Js 1800 GeV with prediction ofreference 1 E710 = 1985 4. POMERON STRUCTURE FUNCTION Diffraction dissociation is the name given to inelastic events in which one of the initial hadrons changes its momentum by only a very small amount. In doing so, it 'radiates' a pomeron. The other initial hadron is hit by the pomeron and breaks up into a system X of hadrons. The UA8 experiment at the CERN colliderl8l has measured the angular distribution of the energy flow of the that make up the system X, in its rest frame, thatis in the centre-of-mass frame of the pomeron-hadron collision. This is shown in figure for events where the pomeron takes only a fraction 0.006 of the 4, initial momentum of the initial hadron from which it was radiated. This corresponds to an invariant mass of 50 GeV for the system X. Notice the vertical logarithmic scale: there is a huge forward peak. The pomeron has hit the other initial hadron hard and knocked most of its fragments forward. In this respect it behaves as if it were itself a 398

hadron, or a photon. In fact, as I have already said, it is useful to think of the pomeron as resembling a C +1 isoscalar photon. One cannot take this analogy too far; for example, there is no such= thing as a pomeron state, it can only be exchanged. However, one can define its structure functionf9l .

105 i$' .[

"O 101 !g .JI! __ .....__ ------..... --..• -1 .0 -0.5 0 0.5 1.0

cos 8

Figure 4 data for energy flow in diffraction dissociation, in the rest frame of the system X of U AS fragments of the shattered hadron. This is measured from events where the system X has resulted from a hard col­ lision, for example when it contains high-Pr jets. Given that, as we have seen, the pomeron couples to quarks, it is natural to suppose that the corresponding diagram for this reaction is that of figure 5, where one of the quark lines at the pomeron vertex suffers a hard collision with a gluon from the other initial hadron and so produces a pair of high-pr jets. If we forget the initial hadron from which the pomeron radiated, it is as if the pomeron were an initial , and then one would calculate such a diagram by introducing its structure fu nction. We predictedf10l that, for each light quark and antiquark to which the pomeron couples, its structure function is

xqpomeron !C7r:r(l- X (8) = ) where the constant C is determined by measuring the small-x behaviour of the quark distribution in a proton: (9) so that C 1/6. If we sum over the light quarks and antiquarks, �

xqpameron O.Bx l - x (10) � ( )

U AS has studied the shape of the pomeron structure function, by looking at events where the sytem X contains jets with 8 GeV and the pomeron takes about 5% of the momentum of its parent hadron. FigurePT > 6 shows their raw dataP 1 l , compared with the result of subjecting two guesses forthe shape of the pomeron structure function to a Monte Carlo that simulates the acceptance of their apparatus. Evidently the shape x(l - x) works well, much better than (1 - x )5 • It does not fit perfectly - I will come back to this in a minute - but UA8 go on to determine the coefficient that the data 399

require for x(l . This depends whether the structure function is dominantly a quark - x ) one, as we suppose, or a gluon one. UA8 are not able to distinguish the two possibilities from their data. If quark, the coefficient is 0.8, as predicted in (10). If gluon, it is less than half this, because gluons are more efficient than quarks in producing high-pr jets. The experimental error on the coefficient is quite large, perhaps 50%, but one can certainly exclude the coefficient 6 which would be obtained by supposing that a pomeron is so much like a hadron that its structure function obeys a momentum sum rule.

0.7 0.94 0.96

0.6 • DATA \ x(1-x) MC \ c (1-x)3 MC 0.5 ..,,Ci) 0 � "O 0.4

z "O z 0.3

Figure 5 0.2 + Diffractive high-pr jet production mechanism 0.1

� �L-�L-�.l--�.U-.--1.S::::.-.J;J1.5 OL--2.0 -1L-.5 -1 .0 -0.5 0 0.5 1.0 U....,..-o-'2.0 11 Jet

Figure 6

data for pseudorapidity distribution of 8 GeV jets UA8 PT > produced in diffraction dissociation, with expectations for two different choices of the shape of the pomeron structure function

It is important to determine whether the pomeron structure function is indeed predominantly quark rather than gluon. There has been some confusion about this. The fact that, as everybody agrees, pomeron exchange is gluon exchange, does not imply that the structure function is entirely, or even predominantly, gluonic. What is what the pomeron prefers to couple to. While we cannot exclude that it couples to gluons, there is certainly an important coupling to quarks, otherwise we should not have the additive-quark rule for total cross-sections. We have argued that the quark coupling in fact dominates, though there is some uncertainty about this and further experiment, particularly at HERA, is needed to decide the . Because virtual photons couple to quarks, HERA will measure the quark structure function directly. Let me return now to the small discrepancy between the raw data in figure 6 and 400

the output from the :z:{l assumption. UA8 have confirmed that the discrepancy - x) is indeed a real one, by looking at those events in which they see both of the high-pr jets. They find that the two-jet system can take or nearly the energy of the all, all, parton/pomeron collision; that is, in some events there is little or no energy to spare for any spectator fragments from the pomeron structure. In figure 5 there is one such spectators. One can also draw a diagrams in which this second quark is actually the recoil high-pr jet, instead of being a spectator. An example is drawn in figure 7. It is consistent to suppose that figure 7 is responsible for the discrepancy that UA8 find, but this is not certain. It will therefore be interesting to look for such a mechanism directly at HERA. The diagram is drawn in figure 8, where now we are considering the case of a real initial photon. In the final state, there is only the initial proton !l.nd a pair of high-pr jets. In the gluon-exchange model, figure 8 corresponds to fourdiagra ms. Our calculation of these[121, for .J 250 GeV and p ET > 5 GeV, s,P = � gives a cross-section 1 nb. 17'YP :::::;

---- pomeron

Figure 7 Figure 8 Alternative mechanism for diffractive high-pr jet production Mechanism for HERA events where the proton loses only a small fraction of its momentum, with all the remaining energy going into a pair of high-pr jets

REFERENCES 1 A Donnachie and P V Landshoff, Nuclear B244 (1984) 322; B267 (1986) 690 2 L Gribov, EMLevin and M G Ryskin, Physics Reports 100 (1983) 1 3 P V Landshoffand Nachtmann, Z Phys C35 (1987) 405 0 4 M Block and R Cahn, Phys Lett B188 (1987) 143 5 J P Burq et al, Nuc Phys B217 {1983) 285; fit by HGDosch (private communication) 6 R S Fletcher, T K Gaisser and F Halzen, preprint MAD-PH-689 7 E710 collaboration: N Amos et al, Phys Lett B243 (1990) 158 8 UA8 collaboration: P Schlein, talk at LPHEP'91 Conference (Geneva, July 1991) 9 G Ingelman and P Schlein, Phys Lett B152 (1985) 256 10 A Donnachie and P V Landshoff, Phys Lett B191 (1987) 309 11 UA8 collaboration: A Brandt, seminar at CERN (December 1991) 12 A Donnachie and P V Landshoff, preprint CERN-TH-6431/92