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COO 264-579 EFI 71-32

*fAW# " = 2 8.W#..3 HIGH ENERGY SCATTERING OF

Reinhard Oehme

1 The Institute

i and the Department of

1 The University of , Chicago, Illinois 60637

1 May, 1971

Contract No. AT (11-1)-264

sponsoredThis report by thewas prepared as an account of work United States Government. Neither the United States nor the United States Atomic Energy Commission, nor any of their employees, nor any of their contractors, subcontractors, or their employees, makes any warranty, express or implied, or assumes any legal liabUity or responsibility for the accuracy, com- < productpleteness or usefulness of any information, apparatus, or process disclosed, or represents that its use · would not infringe privately owned rights.

PISIRIBIET.oN w IHIS DOCUMENT IS UNLIMm /\\\, DISCLAIMER

This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency Thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof. DISCLAIMER

Portions of this document may be illegible in electronic image products. Images are produced from the best available original document. HIGH ENERGY:SCATTERING.OF HADRONS

Reinhard'Oehme

The

and the Department of Physics

The , Chicago, Illinois 60637

Meinem verehrten Lehrer

Herrn Professor

zum siebzigsten Geburtstage gewidmet

/2 -2-

Zusammenfassung

Nach einer kurzen Einleitung uber die Entwicklung der Dispersions-

theorie wird zunachst der Zusammenhang zwischen der asymptotischen

Form von Streuamplituden bei hohen Energien und den Singularitaten

der Partialwellenamplituden in der komplexen 2-Ebene des gekreuzten

Kanales betrached. Einschrdnkungen des Charakters und der analytischen

Eigenschaften dieser singuldren Flochen durch AnalytizitHtseigenschaften

und Unitaritdtsbedingungen in beiden Kandlen werden abgeleited und deren

Einfluss auf das Verhalten der Amplitude bei hohen Energien besprochen.

Insbesondere werden komplexe Traj C ktorien eingefuhrt und ihr Zusammenhang

mit Stossparameter Darstellungen aufgezeigt. Die Betrachtungen beziehen

sich hauptsdchlich auf Probleme der Diffraktionstreuung und auf damit

zusammenhdngende Fragen.

t

./ -3-

I. INTRODUCTION: Dispersion Theory.

Twenty years ago in Gottingen, I wrote an article in collaboration with LOders and Thirring which was dedicated to Heisenberg on the occasion of his fiftieth birthday.1 In this paper, we explored the possible

implications of covariant and of the renormalization scheme for the physics of strongly interacting particles. Although we saw some precursors of later developements, we also found that the methods of perturbation theory, which worked so well in quantum electrodynamics, were compl etely insufficent for hadronic interactions. We indicated that,a new mathematical formalism was required which incorporated the general invariance principles. Indeed, a few years later, such a formalism began to take shape with the developement of relativistic dispersion theory.

Dispersion Relations for the forward scattering of light had

2 been known for quite some time, and they were rederived on the basis of relativistic.quantum electrodynamics. Although analytic methods had,been used before in order to make the connection between causality and forward.dispersion relations,2,3 for the extension of dispersion theory to hadronic interactions it bacame essential to recognize the importance of the complex plane and to view physical amplitudes as 4 boundary values of analytic functions. In particular, certain related amplitudes were seen to be different boundary values.of one and the same analytic function of two or more complex variables. It is true that these crossing properties can be read off from.perturbation theoretical . '

-4-

' . models, but they were introduced at this time directly on a more general basis. Perturbation theory was so much in disrepute that it would not havebeen sufficiently convincing for the acceptance of these resol ts. The further exploration of the analytic properties of amplitudes changed this view, and we learned to use perturbation theory as a valuable guide to extend our understanding of the singularity structure of Green's functions.5

Particularly, the artifitial limitations of general proofs of analytic properties from the basic assumptions of field theory could be judged very 6 well on the basis of Feyman graphs. The latter were also most helpful for the understanding of those singularities which are not directly related 6,7 to the physical intermediate states of a given channel. These singularities describe the structure effects of particles considered as composite systems of other particles;8 they emerge from unitarity and crossed channel properties.

We have described these singularities ten years ago in an article entitled

"The Compound Structure of Elementary Particles", which was written on the 9 occasion of Heisenbergs sixtieth birthday. These structure singularities or anomalous thresholds may well be of importance in connection with scaling

properties of off-shell amplitudes at nonasymptotic energies, and for higher order Green's functions.

On the phenomenological side, the prompt and astonishing success of

10 forward - dispersion relations gave a wellcome boost to the

analytic approach to particle physics, as did sensible pole dominance

methods and other approximate dispersion calculations for low energy scattering.11

On the other hand, high energy limits came into focus with the advent of

complex methods. These provided a tool to correlate the

asymptotic expansion in one channel with the low energy properties of the

appropriate crossed channels.They also brought a connection between the -5-

12 ···" classification of hadrons and the analytic methods.

Approximate higher symmetries had been developed rather independent 13 of dispersion theoretical methods. But then a very interesting connection 14 was discovered with the help of superconvergent dispersion relations. It was found that, for amplitudes which vanish sufficiently fast at infinity, these dispersion relations could be saturated with a finite number of resonances. Consistency requires that the saturation is made with sets of resonances which fall into the lower representations of rest symmetry 15 groups like U(6) 0 U(6), and it turns out that vertex symmetries of 16 17 collinear U(6) emerge automatically. Since these symmetries are broken in reality, their association with an approximate scheme within the dispersion theoretical framework seems most natural. In any case, we have here a certain connection between the analytic methods of dispersion theory and the group theoretical structure which is characteristic for the quark model.

The approximation of amplitudes with only resonance states has in recent years been extended by the introduction of meromorphic functions which satisfy crossing and which have Regge asymptotic behaviour in directions 18 away from the real axes. The resonances in. one channel are generated by the controlled divergence of the infinite sum of resonances in the corres- 19 ponding crossed channel (mathematical duality). Meromorphy makes it possible to write down explicite forms with factorized residua even for production 20 amplitudes. But the ghosts which have been seen before with super- convergence relations are still present in spite of the exponentially increasing degeneracy of states which factorization requires, although in | -6-

certain models they reappear in the form of Tachyons. Nevertheless,

there are attempts to use meromorphic amplitudes as a basis for a new

approximation scheme which would bring in the unitarity constraints.

Of special interest are the implications of dispersion theory and

complex angular momentum methods for high energy scattering. Unfortunately,

what we have here is only a general scheme rather than a complete theory.

We know from basic assumptions that there must be Regge poles, branch

points and possibly other singularities in the complex angular momentum

21 plane. But at present, we have no reliable method to calculate the

actual singularity structure. In general there are many constraints,

and for certain situations these can be quite restrictive.

There are several models for diffraction scattering which use 22 quasiclassical notions or intuitive abstractions from field theory.

These are often consi dered as an end in themselves because they can be

easily explained and understood. On the other hand, the methods of dispersion

theory are more mathematical and more abstract, and sometimes rather subtle

to handle. Nevertheless, we think that this framework is a very comprehen-

sive one for the description of hadrons and hence that we should try to

understand diffraction scattering on this basis. Of course, as we have

21 pointed out on previous occasions, it is not impossible that the disper-

sion scheme itself is too narrow and that there is something wrong with the

basic assumptions. To find such a discrepancy would be a most important

discovery in itself and may give a clue for a more concise theory. In the following we /8escribe some of the constraints dispersion theory imposes upon the high energy limits of amplitudes. We are. pa.rticularly interested ,in diffraction .scattering, which is a most.important and central problem. It is al.so,.of higli current interest in view of the. new data , :. - now becoming available from ·Serpukhov, CERN and NAL. -8-

II. COMPLEX ANGULAR MOMENTUM

1..,Partial Wave Amplitudes · ..· · ·· ·, ·' i , i ...

We consider first the'high energy behavior of scattering amplitudds ' as described by Regge trajectories in thecomplex angular mome'num plane of ; the crossed channel . The unique analytic interpolation of partial wAve amplitudes is a direct consequence of the existence of single variable 22 dispersion relations with a finite number of subtractions. Let us use invariant amplitudes F(s,t) and F(s,t) for particle and * scattering, and introduce the combinations

-I...

F; cs,t 3 - Fcs,t ) f FCs,t JI . (2.1) they satisfy the reality condition * .4

Ft (si, t ) = F t(S,t) , (2.2) and they have the symmetry property

Ft c s 1 2 ) = + 1 : C u, 2 ) , (2.3) where u = -s-t+I (I = sum of squares of external masses). For appropriate values of t (like real t 1 0),we have the dispersion relations

:t

1 * For simplicity of writing, we use the Feldverein model. -9-

00

ic,i 163 r. , vt A+(,24 ) - i (3,t )= 1:S (40,t , + r - Ja" 1. ' . (vit v &)(112- 4 J

(2.4)

Vr-' F ·i-O i t ) = 96 - - t- (4 0, t) loe . 4 (9 )- 11 )2 92 1,1,1, i - ' 1 ' (2.5) 1( CV,1 'C')(411. Vol) 0

where the symmetric variable v E (s-u)' has been introduced for simplicity. On the basis of the dispersion relations we obtain continued partial wave

amplitudes 06

10- E ct,,) . * Fet'' 1, Ox c "42*,) A, c.>,2 J , J 2 1-Ct) 20 (2.6)

with

A t Le, i , = A l (#-1 j i A 4L c..., 1 j .

(2.7)

The absorptive parts As and Au determine analytic functions which uniquely

interpolate the physical partial wave amplitudes for e > 1:

FI (t, A- e j = 5 (t), 2 = e#*w *401 . (2.8)

l -10-

Since Qx is a meromorphic function with only simple poles at negative integer values of x, we have in Eq. (2.6) a direct correspondence between the asymptotic expansion of absorptive paits At(v,t) for v + -,'and the singularities of F (t,x) in the complex A-plane. For sufficiently large values of Rex, these functions are always given by the representation (2.6), and the continuation to smaller values of x can be done with the,helb of the asymptotic expansion of At(v,t). Hence the singular surfaces of

F+(12) are determined by the high energy part

--Il-

C 2 I A ) a<: GJ# V- 2- ' 1+ C .0-, 6 ) I /*bl k (2.9) 6L of Fi(t,x), with b2 taken as large as we please. We see·that the power behavior of an. asymptotic term in the expansion of A corresponds generally to the position of the related singularity in the complex

A-plane; logarithmic factors are related to the character of the singular surfaces.

We are here particularly interested in the restrictions imposed upon the character of 3.-plane. singularities by the unitarity condition in the t-channel. We have discussed this subject on several Drevious occasions 23 ,

t - 11 -

* but there are reasons to resume and to combine these earlier .treatments.., t,

2. Continued Unitarity -

The continued unitarity condition, in the case of an elastic cut ** for t 0- < t i t i, may be written i n the form

Flt,„.*,7,- F(t-io, A) = 2.·f(t)F(t+,0,2,Fa-··o, A) , (2.10)

and hence the continuation of F(t,A) around the branch point t into the second sheet is given by

1 Ct,A ) = F -'ct, 2 ) + 2 2 f (t ) (2.11)

Here and' in Eq. (·2.10)·,.we have

/ 6-918 )44 1 ' (t) . C t .1 I (2.. 12)

* Prior to the introduction of complex angular momentum methods, it has already been pointed out by Gribov that a high energy behavior like F(s,t)- i C(t)s is not allowed for to i t< ti. This interesting result is however much weaker,than the absence of a fixed pole at.x = l. For example, an asymptotic behavior of the form F(s,t) - iC(t)s + 8(t)S'(t with Rea(t)<1 for t<0 and.Rea(t)>1 for t l t would be compatible with the theorem of

Ref. 24, but it would be forbidden if a fixed pole at x= 1 is not allowed. ** Here and in the following we iinore signature indices whenever they are not relevant. - 12 -

The characteristic feature of this condition is not only the boundedness which it implies for real t s t < ti' where

S c t, A ) S'(t, A' ) -1 (2.13) with '

S Ct,X) = 1+ 2.'fa,Fit, A), (2.14) but also the more detailed information that F(t,x) has a square root branch * point at t=t . These features, combined with the fact that F(t,x) is an analytic function of two complex variables, impose many restrictions upon· the singular surfaces of this function. In their most general form, these 25 restrictions are a consequence of the continuity theorem. Roughly

speaking, this theorem states that a singularity of a function of several complex variables cannot simply disappear somewhere if one follows them

through the inside of the domain of definition of the function.

a the The most simple example is fixed pole 'of F(t,x) at point A=10.

If x is real, we see of course directly from the boundedness for t st

* There is a superimposed winding point, but the corresponding cut should

be drawn to the left. It does not interfere with our considerations. In

the physical sheet, it can be removed by multiplication with (t-t )- = -2x (29(t)) . See OI.

1 - 13 - in Eq. (2.13) that it is forbidden. But for complex poles the situation in Eq. (2.13) is not so straightforward. On the other hand, the continuity theorem immediately gives the result. We see from Eq. (2.11) that

F WAN-0 F -Ct, A ) = I lt, A-0 Jo 1 r f (2.15) and hence the pole appears to get, lost in the continuation from sheet I to sheet II. If this continuation is possible, then we have a contradiction and the fixed pole is forbidden. In order to see this more directly, we write for A ina neighborhood of xo: -

11 1 -1

-1 .-.1 6 ell' F--9,4 j E (214) I i . ., 2 F : T 31-A. C which ·is. possible since FI[ 'is regular there as seen from Eq. (2.15). Let , us now continue this ·representation through the elastic. branch cut, appropriately deforming the closed contour C in order to avoid other singularities. If this continuation is not blocked, and wd. wil'l see later that it may be blocked by very specific shielding cuts, we obtain

-' Fit A' ) _11 L 441 1--- 1- C t, A e ) Z r f c' A'- Ae

Hence there can be no pole at A = A . - 14 -

Ihe arguments given above are not restricted to fixed poles in the

A-plane. They apply also for singular surfaces x= a(t) which have the following properties:

1) lim F(t,x) = oo

1 + a(t)

2) a(t) = oF(t), i.e. the analytic function a(t) has

no branch point at t = to

From Eq. (2.11) and the condition 1), we obtain

.. I - F i L ct , A - 0(l t) j )

Ziecti (2.16) and if the limit x + a(t) and the continuation Fe Fn can be interchanged, we see that Eq. (2.16), together with the condition 2),would lead to i I l t) ) = - - j F (t, A. i ) 2; tt (2.17) which contradicts condition 1).

So far, in our discussion, we had in mind trajectories a(t) which are pole surfaces and branch point surfaces with t-independent character.

However, the arguments can be generalized to many other situations which we do not want to discuss here in detail. We mention only the case of an essential singularity of F(t,A) at a point x =a(t) with aI(t) = a(t). - 15 -

We know that there must then be sequences {An(t) } + a(t) for n + oo such that

1·- F (t, A., (t , b = ee . 11 -DOE ,

If there is a-sequence {An(t)} with n(t) = An(t) for almost all An' then we have again a contradiction with the unitarity condition.

So far, we have considered only the implications of elastic

26 unitarity in the t-channel. The arguments can however be generalized to systems with many coupled channels. As long as all thresholds Are' different, we can always find a Riemann sheet where a singularity would have to di'sappear suddenly unless specially arranged shielding cuts" intervene and prevent the continuation. There are some 4ossible ekceptions for nonfactorlzing singularities, but they are not of direct physical interest for hadronic interactions. Also coupled spin channels with identical threshold requi.re special treatment. Here we do not want to elabor- ate on these details. - 16 -

3. Shielding Cuts

As we have al ready i ndi cated above, there are ways to prevent a contradiction with the unitarity condition, even though a singular· surface a(t) satisfies the condition 1). If the character of the singularity is t-dependent, we may have in some cases the possibility to adjust this t- dependence in order to get consistency with the unitarity condition.

But it is difficult then to comply with the known analytic properties Of

F{t,x). Here we do not want to elaborate on this possibility. Rather, we concentrate on two methods which are of importance for high energy scattering.

a) A well known solution to the unitarity problem is the introduc- tion of a branch point in a(t) at t = 0, with a cut.alonq the real axis for t L t,. Then we. have a (t) :t a(t). This branch point is related to the unitarity cut of. F(t,x), and for Regge poles one can show,that it is

22 of the form 0(tto ) + i 0 lt) - 0( l t. ) + 6», 4. 01: o-t ) +...

b) The other possibility is the presence of shielding cuts which make the continuation through the cut t>_ t non- the limits X -*a(t) and - 0 interchangable. Let us denote these branch point surfaces of F(t,x) by t = ts(X) or X = as(t), as(ts(A)) = 1. In order to see the required - 17 -

character of these surfaces, we consider the (t,A), which is * function defined by

'.'

Cf- '(-i, A ) F -c t, 2 3 + Lf (0) ,

(2.18),

and which does ·not have ·the unitarity branch point at.t = to:

-"- 9 -Ct, A) 9 (2'A) (2.19)

If F(t,A) + - for.1 + a.(t), we find .

. 9 - 'c t i A = O( lt) ) = '. f (t ) (2.20)

We assume here a (t) = 0(t). Since %(t,A) does not have the elastic branch 1/2 cut corresponding to (t-t ) , the latter must be supplied by the shielding cut trajectory ts(x). Hence we have the requirement

t s C A = 0 (1 1 2 = -t o + · · · (2.21) so that the branch cut on the right hand side of Eq. (2.20) is generated by

* 2A Again there is a left hand cut due to'the factor (t), which does not disturb us. - 18 -

1/ . ' '11 -/ (ts (Al- 6 ) -> (2.-t) (2.22)

for A + a(t). We see that shielding cuts must be of square-root type.

As an oversimplified example for the' way a shielding cut works, we give an explicite function which has a pole at X = a (t) with aoll(t) =

a (t), and which is bounded at this point in the second sheet. We write Cts(A)-t)1/2 + (to-t) // L f i t, ) ) 9 - A - 0<0 (t , (2.23) physical with ts(00(t)) = to. Then we have in the sheet for A+ 50(t)

2 (10 -t ) 4,

i 11, A ) = 3 - Holt) ' (2.24)

whereas in the second sheet we obtain

iF /

2,4. f i 1, A ) -9 -i s ( 0(• li ) ) , A -, Hell) (2.25)

which is finite.

e -.19'-

4. Applications

There are many physical implications of the restrictiohs discussed here. The most familiar is perhaps the fact that a positive signature fixed 'pore at x=1, which gives a high energy limit for t i O o f the' form

-Fi ( s, i ) 4 ; 3 (t ) s (2:26) corresponding to a non-shrinking diffraction peak, must be accompanied by an appropriate shielding cut as(t) with as(to) = 1. A high energy behavior of the form (2.26) is typical for semiclassical models which are a priori unrelated tb the t-channel exchanges. But via the required shielding.cut, and possible Regge poles which· generate this shielding cut, they are indirectly connected with the low energy properties of the t- channel reaction.

As a further application, we mention the branch point trajectories which are associated with Regge poles. .In the most simple cases, the position of -these branch points is given by

0(y, (t j - 1 0( C 6 ) - M + | , 0 2 1 J (2.27)

27 where a(t) is a pole trajectory. By themselves, these cuts act as shielding cuts for the nonsense wrong signature fixed poles of the amplitude 28 F(t,A), which are due to the poles of Q1 in Eq. (2.6). Since the pole trajectory a(t) has a branch point at t = t , we see from Eq. (2.27) that the functions an(t) generally do not have one at this threshold. Hence we see from our previous disscussions that these trajectories an must be singular surfaces such that F(t,x) remains bounded for 1 + an(t). But - 20 -

quite apart from this general restriction, they must be square-root - 23 branch points in order to- act as shielding cuts for the fixed poles·

at nonsense wrong signature points, 1 '.,

From our discussions, we see that t-channel.unitarity imposes certain

restrictions upon the singular surfaces of the partial wave amplitude

F(t,x), and hence also upon the high energy limits of F(s,t) in the s-

channel. It is true that the connection with physical high energy limits requires.,analytic continuat.ions between the regions t K 0 and t 2-to. It should be noted that this is not a very restrictive requirement in view of * the analytic properties of.F(t,x) as a function of two complex, variables.S

Of course, there may be, for example, very sophisticated natural boundaries

which in principle could block an analytic connection, but·we must recal,1

that sucb boundaries themselves must comply with the unitarity condition

and also with the known analytic properties of F(t,x). We know that· for

* For example, one may think of writing F (s,t) + ie(t)s for s + = with expansion 8(t)ace(to-t). This would correspond to a term in the meromorphic

of F (t,x) which is proportional to

0(to-t) 1-1

1. This term generally is not compatible with the analytic properties of the

t paftial wave amplitudes in the finite t-plane. Although we are dealing with

an asymptotic expansion of F(s,t) for s + -, the t-dependence appearing in the

* individual terms of this expansion is related to'the t-dependence of the partial wave amplitude F(t,x), which is an analytic function. - 21 -

the > 1, = even/odd the function F(t,X) coincides with physical partial wave amplitudes in the t-channel. For z = 0, 1 we cannot prove this coin- cidence, but this does not detract from the existence of a continuation of

F(t, x) into the region Rex<1. In fact, as we have seen in Eq. (2.6), the asymptotic expansions of the absorptive parts As and Au completely determine this continuation. If it should happen that F (t,0) f FQ(t) and/or F_(t,1)

Fl(t), then we have only an additional real polynomial of the form

F S l t) + A F t (t, E ( 1+ -s. 21 Let) * in the asymptotic expansion of F(s,t). In principle, the functions AF (t) and 8F1(t) are also determined by F(t,x), but at present we have no method ** for their explicite construction.

* Elsewhere we have given a detailed discussion of these terms,in particular in view of their connection with "elementary poles". 23) ** It is important to note that the presence of a term proportional to high energy limit of implies the existance of· a 8Fl(.t)s in the F(s,t) contribution in the absorptive part which grows at least like s. Hence . 29) there must be a singularity in the amplitude F*(t,x) at x=l for t=u .. This follows from s-channel unitarity for t = 0. Using s-channel unitarity also for t < 0, one can give some argument for 30)

A (s.o) - 0(s 1gs). S

A finite term Afl(t) can be related to an "elementary" vector meson. - 22 -

III. HIGH ENERGY'LIMITS

1. General Bounds.

The restrictions for the high energy limit of the amplitude,

which follow from direct channel properties, can in many cases be "

formulated independent of the complex angular momentum description.

However, many of the constraints obtained from unitarity and analyticity

are particularly interesting in connection with complex angular momentum

methods. The usual axiomatic s-channel bounds have been discussed in

31 great detail in the recent literature. Therefore we concentrate here

on the interplay of these bounds with the crossed channel Regge description

considered in the previous Section.

Most of the general bounds for F(s,t) in the s-channel are a conse-

quence of the-analyticity·of F(s,t) as.a function of two complex variables

and of unitarity. Actually only analyticity in- a domain l (s,i): di s.plawi® lilito 1 (3.1 )t.

is required, which can even be proven from the axioms of'field theory. The''

important practical step is the truncation of the partial wave series. From

unitarity and polynomial boundedness in the domain (3.1), we obtain for

t < t and s + - 0 L

Fls,t ) ·- S (.11+1) .lici, i (1+ 2- ) (3.2) £=0 21'1 f, 1/

6 -I *

- 23 --

wi th -1

-1 = 1 /- A A _ + I VAS Egg , CL - #-O/' 6 , (3.3)

because partial waves with £ >L decrease exponentially and become '' ' negligible for s + =. With Eq. (3.2)'.and the unitarity relations

Lir 7 ., f i rt (11 1 - 6 f 15. Fi ( ' ) tr i , (3.4) //L 32 f = (9-30) , we get the Froissart bound i & S L IF(t,0,1 6 -1FQ s (4s j (3.5) for s + ... It implies

1

5.4 6 4r Q s (el E j . (3.6)

With the same assumptions and the Schwarz inequality, we find also that * asymptotically

LF,s,0,11

-I ' c >- -1 5 f S (4-5 J (3.7)

* /6- -L .2 .L L L -1 611 A. S _!1 0 2 cle,t) Ili' 2 29- (Z. (12.1,15.1 ) If-(21.1,1

12 1- 4 r 2,-1 fig- i F i s, 0, i 2 g L 4- 5 l e l s) J - 24 -

Other bounds, which we will need later, are

1 Fcs,i, 1 6 4t s (ea s)zI0 (jakas) (3.8) for 0 s t< to, and

1- 1 Fls,i) 1 6 -3. S (fls) (3.9) for t I 0. - 25 -

2. Complex Trajectories.

In Section II, we have considered the properties of Regge trajectories from the point of view of the t-channel, and we have pointed out that the position of a singularity x = a(t) of F(t,x) in the complex x-plane corresponds to the power behavior of the related term in the asymptotic expansion of F(s,t) for s + oo. Let us now see how the analytic properties of the trajectory function a(t) affect the high energy behavior. We are particularly interested in diffraction scattering, and hence in the neighbourhood of (t,x) = (0,1).

The singular surfaces a(t) do not inherit the left-hand branch 33 points of F(t,x). This follows from Eqs. (1.6) .and (2.9), which show that only the asymptotic properties of As and ALL are relevant for the trajectory functions. A priori, we may therefore assume that the a(t) are regular functions near t = 0:

0( el ) '- Of (6) 4 06(0, t + ... (3.10)

For poles and branch-point trajectories, we obtain then a high energy contribution of the form

°(tt , 1 Fig,t) oc s which gives at most a logarithmic shrinkdge of the diffraction peak. We have

1 f l I f t s,t, 1 ' CAT ( 0f'*La 'j- (3.11) ' -1 - 26 -

with

f (s, t) Fig,t) . Fls,0, (3.12)

Faster shrinkage can be obtained if there is a branch point in a(t) at t = 0. Such branch point must not be present in the continued partial wave amplitude F(t,x), and therefore it is only possible if we have two 34 or more trajectories of the same character which cross at t = 0. Then a(t) near t=0 can be expanded in the form

00 r

0(lt) - 0(l o) + 2. Ci t =0 (3.13) with n -22 being an integer. There are n trajectories which are branches 35 of the same analytic function, and all these branches must appear in

F(t,x) in a completely symmetric fashion.

Of special interest for diffraction scattering are crossing tra- jectories with the behavior *4 - n O(lt 1 = 1 + ct (3.14) near t=0. We are interested in exponents <1. For El = J- w e have n z, a(t) real for t 20 and two complex conjugate singularities for t<0.

This case complies with the bounds (3.9) and (3.91 for c < /3. However, - 27 -

m 1 1 m for 0 < w < 2 and -2- < w < 1, we must have n 2 3 and m < 22- n or m < n, and hence there is always an asymptotic term like *4 1+ 6 IiI E S (3.15) with Re b > 0. Such terms violate at least one of the bounds (3.8) or

(3.9), and we are left with the poss i bility = · . Trajectories of the form

6, (t) = 1 + c.„44. 4£ (3.16) near t=0 can give rise to diffraction peaks which shrink according to 0 -2

f Ott i<,9,0,11 00 (6 9) , (3.17) | -S 37 and they have many interesting properties. One is that they satisfy the bootstrap-like condition

, 0(lt ) = 0( % (t) , 04, l·t ) = 'n 0 (fi ) - 14+1 (3.18) where an(t) is the branch point trajectory generated by the iteration of poles a(t). Other properties will be mentioned later.

In order to see more directly when trajectories of the form (3.16) are required, we make specific Ansatze for the high energy limits of the

forward positive and negative signature amplitudes as defined in Eq. (2,1). 38 In accordance with the dispersion relations (2.4) and (2.5), we write

8 -I +... (3.19)- Fics,03 ac is (fas)8.+ TA s(fas),4 j -'28 -

/ +I FICS,O) 06 - 1 -1-1_ s (f,s) 12 + i s (lig)(i 4-0.. G. A+ 1 (3.20)

General bounds like (3.5) and (3.7) imply the restrictions 31

1 8 2 a„ot 8 5 1 p., . (3.21)

Using the c requirement .cels tot' it is a simple to show that the shrinkage of the diffraction peak must be faster than (lgs) if we have

lf | (3.2 2) for the positive signature, and if

1 A +1 - (4 > 1 (3.23) for the negative signature trajectory. In these cases we conclude from our previous considerations that the appropriate singular surface a(t) must have a branch point at t= 0. Here we assume that the shrinkage is generated by the trajectory function, which is generally the case for * pole-and branch point surfaces. We note that for 2- = B = 0 and a_(0)'= 1, complex trajectories 36. 39' must be present in both the negative and the p6sitive signature amplitude in order to comply with positivity conditions for Im F(<,t) and Im F(s,t) for 0 i t.< t . Of course, we may have trajectories of the fo·rm (3.16) also in -cases where they are.not explici'tely required'.

* There are possible exceptions in the case of essential singularities. 29 -.

3. Impact Parameter Representation.

Another interesting aspect of complex trajectories like (3.16) 40 is their simple relation to Bessel-function representations. In general,

, we can write the amplitude F(s,t) for large values of s in thet form Fis,t j *v s f 11 4,(i,s ) 3.cif--KE- eis) 1 (3.24) which is the usual impact parameter representation with 6 - i li 4, and t''R6(1), S )

1 a 4(6(f i, s ) 6 - 1 1.t (i, s ) = i (fls) T - - ' (3.25) 2 i f B)

The maximal impact pa rameter b = ,/T 1 max gs corresponds to L = Tas l gs as given in Eq. (3.3).

Near (t,A) = (0,1), a rather general class of continued partial wave amplitudes with complex trajectories can be written in the form41, 42

1 f* (t'.t j Fi Lt,A ) »« fd, -

. 1 [CA-1,4.- {1Qt-]'02 (3.26)

We can make this Ansatz compatible with t-channel unitarity in several ways. * The Most ·direct one is to ·choose the weight functions appropriately.

* See Ref. 36 for explicite examples. - 30' -

Otherwise we may consider the denominator in Eq. (3.26) as a degenerate superposition of a complex. pole trajectory and a square-root branch point :trajectory. Further away from t = 0, the pole trajectory must then ., acquire the appropriate branch point at t = t in order to comply with, unitarity. As usual, we assume then that this threshold of a (t) can be neglected as far as the high energy behavior of F(s,i) is concerned.

For p we must also require the condition

j 41 i-' f (B,o ) = o (3.27) 0 in order to prevent singularities of the partial wave amplitude which are not allowed.

As an example, let us consider the case where 81. = B_ = 0 in Eqs. <3..19) and (3.20). Then -l,Le forward amplitude is dominated by the real part of

F_(s,t), and.we .have different asymptotic.total cross-sections a and 3 * for particle and antiparticle scattering. Hence we write

- 0 ' /t\ G--6 €--6- Fl cs, 0 ) 0' - 16 s l. 5 S ) -i i-F + ' s ·irii: + ,

(3.28)

42 we have and with ), f/L i) = f l i

* Whatever may .be the outcome of:present,experiments-on K-meson-nucleon total

cross-sections and on the K regeneration amplitude, the Serpukhov data have at least shown that a=c should not be taken·for granted. - 31 -

f tx ) f E cs,t > w 2 s (11' ) f''I6 (fi 5- ) 1 li 4-- T tls) 4.:, + .. s fot, f ti ) 3, 61'Ca eis ) (3.29) 0

For fixed t ag 0 and s + oo, the first term domi nates, and. we can calculate the asymptotic integrated cross-section 16 /08 (' 4 Gic- , .v ---- j elt 1 E (s, t ) I (3.20) -S in terms·.of p-:

1

6-C-, AJ 1 5 -A j.11 t-, ( f:, U'), e (3.31)

1-1 Except for a factor, the quantity c' ' is the charge exchange (e.g.nn, wN) or regeneration (KN) cross-section. In analogy with the·e'trivatioh of Eq.

43 (3.7), we find the lower bound (s + go)

(6--9-)1 eT G' 2 113Q (3.32)

There is also the upper bound

... 6- C- 6 4 4444* ( 6- 1 e ) . (3.33) - 32 -

It follows that the ratio

. , , & 60 ix, 4 (-) 1 P' 1. ' (fait-i- j 2= /39 6- - = -

- CS- F) , . [ f' 5 1 9:' ] , (3.34) varies between the limits

I6R& FT aa ,*#LLY (ir, 2 ? 6 6-- 2 ) 1

(3.35)

Of particular interest is the boundary case R + 1+0, which gives rise to fo,m 44, 42 2 a unique asymptotic/i,of. the amplitude for s+ = and T= -at(lgs) fixed. From Eqs. (3.28) and (3.34), we obtain

#

1, .0 ..... U (1 1 5-5- i Qtr S- = x L 6 4 (-21)0('-i-°) 0 (3.36) and hence

E c s,i ) A. - * s (t s)L E.-3- 2 3, (/F j 16 C 151

Gl -- S .2 3 (3.37) + 1 5 (,/F) 1 6·R . - >« - + % I, c 47 ) ) e

- 33 -

This is an example of a limiting situation where the general constraints

are sufficient to determine the form of the amplitude for large energies.

In the interval.0 6.t. < t , we have the inequalities Im F(s,t)2 0 and Im F(s,t) 5.0, and they imply that the negative siOnature part of .

these amplitudes cannot dominate. Consequently there must also be a

related complex positive signature trajectory so that, for large values

of s, there is a contribution to the amplitude F (s.,t) which is of the

form

r

S) , i s f Ot i f (i ) 30 ( 1 4--dE 4 (3.38)

However, it is not expected ·that the term ·(3.38) is dominati,ng the ampli- .,

tude for t s 0, at least in the range of presently accessible· energies.

It is probable that there is also a regular trajectory a(t) with a(0) = 1, 45 or a fixed pole at x=1 with the a'ppropriate shielding cuts.

The relevant feature of the representations .(3.29) and (3.38) i·s

the finite support of the weight functions for non-zero va.lues :of the

parameter 4,1.I n contrast, an asymptotic form corresponding to a Regqe

pole like

ir

with a(t) =1+ a'(0)t, would correspond to an s-dependent weight function in Eq.·(3.24), which is giveh by - 12''f 4 Ci,s ) AJ 6("fl,-f) i e (3.39) for lg s >> 1. For E>0, its' support vanishes in the limit s + = .

A fixed pole at x=1 would correspond to

ze l l, s J '« i /1 1-(1- £ ) , f - 0* (3.40)

There are other situations where a unique form of the asymptotic amplitude is obtained. The following case is quite familiar: We assume that the inelastic cross-section approaches a limiting form

Z F#,1 " r £ / .els 1 ' (3.41) which corresponds' to the maximal value which is compatible with the bound 2 9 L= Tas ]g s for .the relevant partial waves in the expansion of 41 42, 46 F(s,t). Then we,obtain '

2 31(,/F) Fcs,-./3. .4 f + , Q.(tjs )1- 1 \ 81 , 3- s f s) ---C-VT (3.42) for.fixed z = -at(lg s)2. This amplitude gives 0 - 20 ., and if it tot ei is extended to fixed values of t, it corresponds to a fully absorbing - 35 -

* disc of radius Ja-. In the complex angular momentum plane it corres- ponds to

-34 15.(t,2 ) oc 1-(A-1,1- 02 1 (3.43) near (t,A) = (0,1). Further away from this point the form (3.43) requires modification or shielding cuts.

* A form corresponding to Eq. (3.42) except for a factor of two is obtained by requiring full saturation of the Froissart bound. Then we have

'tot - cel - 47Ta(19 s)2. - 36 -

IV. Concluding Remarks.

Empirically, we know that.high energy collisions are accompanied

by the production of hadrons,with an average multiplicity which appears

to be slowly increasing with energy. Via s-channel unitarity, the absorp-

tive' part of the elastic amplitude is related to these production processes.

It is therefore of great interest to connect models'for the production ; ' :

amplitudes with the Ansdtze made for the description of diffraction

scattering. However, we may expect that in the sum over intermediate

states at high energy many details of the actual production amplitudes

will be washed out. In this sense, diffraction scattering should perhaps

be considered more as a constraint for these amplitudes, although it is

expected to depend upon the more general features like the increase of the

multiplicity, etc. . Because of the rather direct connection of the diffrac-

tion amplitude with the low energy properties of the crossed channel,

we may hope that an understanding will be possible without a complete

theory of production processes.

We have considered in this article only hadronic interactions and

we have explored asymptotic expansions within this framework. We hope that

the energy region of up to about 1000 GeV, which is now becoming available,

will bring some clarification of the uncertainties which at present cloud

the experimental situation of diffraction scattering. Some important

questions are: do total cross-sections for particle and antiparticle

scattering remain constant and different? does shrinkage stop or not? do

charge exchange and regeneration cross-sections continue to fall or do they

1 1 - 37 -

level off or even start to increase? There are of course many other questions. We should also keep in mind the possibility that the --strong inter- ' action asymptotics is only relevant for an intermediate energy region. -- It is no-t impossible that there is a new regime at higher energies where electromagnetic or even weak interactions come into play and are no more small corrections to the strong ones. However, this possibility does not detract from the importance of exploring the hadronic asymptotics within the framework of dispersion theory. Any indication of deviations from the assumption of this framework would be of greatest interest. In the study of high energy limits within tbe framework of dispersion theory, it is a principal aim ·to get some idea about the physics in small dimensions.

Once we have a reasonable understanding of the asymptotic expansions of amplitudes, we may go back to in the hope of obtaining new. insights. The recent. developements of operator product , ,, 47 expansions may be very helpful in order to establish a more intimate relationship between high energy limits and the space-time formalism.of field theory.

1

..1 - 38 -

REFERENCES

1) G. Luders, R. Oehme and W. Thirring, Z. Naturforschung la, 213 (1952) .

2) Sellmeier, Poggendorf Ann. 143, 271 (1871). R. Kronig, J. Opt. Soc. Am. 12, 547 (1926). H.A. Kramers, Physica 12, 543 (1946), Atti del

Congresso Internationale de Fisici; Como (Nicolo Zanchelli, Bologna,

1927) p. 454. J.S. Toll, Thesis Princeton 1952; Phys. Rev. 104, 1760

(1956). These papers contain further references.

3) M. Gell-Mann, M.L. Goldberger and W.E. Thirring, Phys. Rev. 98 771 (1955).

4) R. Oehme, Phys. Rev. 100, 1503 (1955); 102; 1174 (1956); Nuovo Cimento

10, 1316 (1956). .K. Symanzik, Phys. Rev. 100, 743 (1957). N.N. Bogoliu- bov, B.V. Medvedev and M.K. Polivanov,.Voprossi Teorii:Dispersionykh

Sootnoshenii (Fizmatgiz, Moscow, 1958). N.N. ,Bogoliubov and D.V. Shir-,

kov,·Quantum Theory of Fields (Interscience, New York 1959) ; this book

contains many further references. H.J. Bremermann, R.,Oehme and J.G.

Taylor, Phys. Rev. 109,.2178 (1958); Proceedings of·the "Colloque sur les Probl&mes Math&matiques ·de la The'orie Quantique des Champs," Lil.le,

France, June 1957. R. Jost and H. Lehmann, Nuovo Cimento 5, 1598 (1957).

F.J. Dyson, Phys. Rev. 110, 1460 (1958). H. Lehmann, Nuovo Cimento 1.0, 579 (1958). K. Hepp, Helv. Phys. Acta 37, 639 (1964). H. Epstein,

V. Glaser and A. Martin , Commun. Math. Phys. 13, 257 (1969).

5) S. Mandelstam, Phys. Rev. 112, 1344 (1958). For further references see, J.C. for example, R.J. Eden,P.V. Landshoff, D.I. Olive and Polkinghorne, The Analytic S-Matrix (Cambridge University Press, Cambridge, 1966). - 39 - i References (continued)

6) R. Oehme, Phys. Rev. 111, 1430 (1958); Phys. Rev. 117, 1151 (1960) ;

Phys. Rev. Letters 1, 510 (1960).

7) R. Karplus, C.M. Sommerfield and F.H. Wichmann, Phys. Rev.111, 1181

(1958); 1-14, 376 (1959). Y. Nambu, Nuovo Cimento 9, 610 (1958)..

8) R. Oehme, Nuovo Cimento 13, 778 (1959).

9) R. Oehme, in Werner Heisenberg und die Physik unserer Zeit,'ed. by

F. .Bopp (Vieweg, Braunschweig, 1961) p. 240; this paper contains

further references.

10) M.L. Goldberger, H. Miyazawa and R. Oehme, Phys. Rev. 96, 986 (1955) .

H.L. Anderson, W.C. Davidon and U.E. Kruse, Phys. Rev. 100, 339·(1955).

R. Karplus and M.A. Ruderman, Phys. Rev. 98, 771 (1955). M.L. Gold-

berger, Phys. Rev. 99, 979 (1955). R. Oehme, Forward Dispersion

Relations and Microcausality,in Quanta [Essays jn Theoretical Physics

Dedicated to Gregor Wentzel] (Univ. of Chicago Press, Chicago; 1970)

p.,309; this article contains a list of further references.

11) G.F. Chew, S-Matrix Theory of Strong Interactions (W.A. Benjamin, Inc.,

New york, 1961). J. Hamilton in Strong Interactions and High Energy

, Physics, ed. by R.G. Moorhouse (Oliver & Boyd, Edinburgh, 1964) -p. ·281.

These papers contain many further references.

12) R. Blankenbeckler and M.L. Goldberger, Phys. Rev. 126, 766 (1962),,and I

La Jolla Conference, 1961. G.F. Chew and S.C. Frautschi, Phys. Rev.

Letters 7, 394 (1961); 8, 41 (1962) G.F.'Chew, S. Frautschi and S.

1 Mandelstam, Phys. Rev. 126, 1202 (1962); S.C. Frly,tschi', M. Gell-Mann and F. Zachariasen, Phys. Rev. 126, 2204 (1962)1 - 40 -

References (cont.)

12) V.N. Gribov, Zh. Eksprim. i Teor. Fiz. 11, 1962 (1961) [Translation: Soviet Phys. JETP 14, 1395 (1962)]. R. Oehme, Phys. Rev. Letters 9,

358 (1962). R·. Oehme, in Strong Interactions and High Energy Physics ed. by R.G. Moorhouse (Oliver and Boyd, Edinburgh, 1964) p. 129-222.

13) See, for example, M. Gell-Mann and Y. Ne'eman, The Eightfold Way,

(W.A. Benjamin, Inc. New York, 1964).

14) R. Oehme, Phys. Letters 21, 567 (1966), 22, 207 (1966); Phys. Rev. 154, 1358 (1966). S. Fubini and G. SegrJ, Nuovo Cimento it, 641

(1966); V. de Alfaro, S. Fubini, G. Furlan and G. Rossetti, Phys. Letters 21, 576 (1966). L.D. Soloviev, Sov. J. Nucl. Phys. 3, 188

(1966).

15) A. Salam, R. Delburgo, and J. Strathdee, Proc. Royal Soc. (London) 284, 146 (1965). A. Pais, Rev. Mod. Phys. 38, 21.5 (1966); this paper

contains further references.

16) K.J. Barnes, P. Carruthers and F. von Hippel, Phys. Rev. Letters 11, 81

(1965). R. Oehme, Phys. Rev. Letters lt, 664, 866 (1965); Preludes in

Theoretical Physics ed. by A. De Shalit, H. Feshbach and L. Van Hove

(Nbrth-Holland, Amsterdam 1966) pp. 143-153. H.J. Lipkin and S. Meshkov,

Phys. Rev. Letters 14, 670 (1965); Phys. Rev. 143, 1269 (1966). K.J.

Barnes, Phys. Rev. Letters 11, 798 (1965). P.G.0. Freund, Phys. Rev.

Letters 14, 803 (1965). P.G.0. Freund and R. Oehme. Phys. Rev. Letters 11, 1085 (.1965). A. Pais, Rev. Mod. Phys. 38 215 (1966).; this paper

contains further references.

. - 41 -

Refs. (cont.)

17) R. Oehme, Phys. Rev. 154, 1358 (1966). R. Oehme and G. Venturi., Phys.

Rev. 159, 1283 (1967). G. Venturi, Phys. Rev. 161, 1438 (1967), 163

1826 (1967). P.G.0. Freund, R. Oehme and R. Rotelli, Phys. Rev. 164,

1859 (1967), Nuovo Cimento 51A, 217 (1967). R. Oehme, Ann. of Physics

(New York) 46 347 (1968); this paper contains further references.

18) G. Veneziano, Nuovo Cimento 57A, 190 (1968). K. Bardak i and H. Ruegg,

Phys. Letters 288, 342 (1968). For further references, see for example,

M. Jacob, Proceedings of the Lund International Conference on Elementary

Particles ed. by G. von Dardel (Berlingska Boktryckeriet,.Lund, 1969).

19) R. Oehme, Nuclear Physics 816, 161 (1970).

20) Y. Nambu, Proceedings of the International Conference on Symmetries and

Quark Models, Wayne University (Gordon and Breach, New York, 19701 p. 269;

preprint EFI 70-07 (1970). S. Fubini, D. Gordon and G. Veneziano, Phys. Letters 298, 679 (1969). L. Susskind, Phys. Rev. Dl, 1182 (1969).

Y. Miamoto, Prog. Theor. Phys. 42, 1166 (1969). K. Bardak i and S. Mandel- stam, Phys. Rev. 184, 1640 (1969). 21) For details and for references see R. Oehme, Complex Angular Momentum

in Elementary Particle Scattering·, in Strong Interactions and High

Energy Physics, ed. by R.G. Moorhouse (Oliver and Boyd, Edinburgh and

London, 1964) pp. 129-222; this article will be referred to as

OI. R. Oehme, Complex Angular Momentu'min Springer Tracts of

Modern Physics, Vol. 57, ed. by G. Hohler (Springer Verlag, Berlin-

Heidelberg, 1971) pp. 134-157. This article will be referred to in

the form OII, it also contains further references. R. Oehme, High

Energy Scattering and Dispersion Theory, in Dispersion Relations and

their Connection with Causality, ed. by E.P. Wigner (Academic Press,

L . - 42 -

Refs. (cont.)

21) New York, 1964) pp. 167-256.

22) See, for example, the Proceedings of the Third International Conference

on High Energy Collisions, ed. by C.N. Yang et al. (Gordon and Breach,

New York, 1969).

23) R. Oehme, Phys. Rev. Letters, 2, 358 (1962); Phys. Rev. 130, 424 (1963) ;

Phys. Rev. Letters 18, 1222 (1967); OI p.160; OII,p. 136 .

24) V.N. Gribov, Nuclear Physics 22, 249 (1961).

25) H. Behnke and F. Sommer, Math. Am. 121, 356 (1950).

26) See OI, p. 161.

27) S. Mandelstam, Nuovo Cimento -30, 1127, 1148 (1963). OI, p. 187.

28) C.E. Jones and V. Teplitz, Phys. Rev. 159 1271 (1967). S. Mandel.stam

and L.L. Wang, Phys. Rev. 160, 1490 (1967).

29) P.G.0. Freund and R. Oehme, Phys. Rev. Letters 10, 199 (1963).

30) K. Yamamoto , Phys. Letters 5 355 (1963).

31) See, for example, A. Martin, Scattering Theory: Unitarity, Analyticity

and Crossing (Springer Verlag, Berlin-Heidelberg, 1969). R.J. Eden,

Rev. Mod. Phys. 43, 15 (1971). These papers contain further references.

32) M. Froissart, Phys. Rev. 123, 1053 (1961).

33) R. Oehme and G. Tiktopoul·os, Phys. Letters 2, 86 (1962): OI.,r. 149.

34) R. Oehme, Phys. Letters 308, 414 (1969); Phys. Rev. 22, 801 (1970).

O I I , p. 1 4 4

W -43-

Refs. (cont.)

35) Hung Cheng, Phys. Rev. 130, 1283 (1963). OI, p. 155.

36) R. Oehme., Phys. Rev. .Qi, June 15 (1971); EFI-preprint 71-26 (1971).

37) R. Oehme, Nuovo Cimento 25, 183 (1962); Phys. Letters 318, 573 (1970);

OII 0.146 . P.G.0. Freund and.R. Oehme, Phys. Rev. Letters 10, & 1

415 (1963). J.H. Schwarz, Phys. Rev. 167, 1342 (1968). J.B. Bronzan,

MIT preprint # 199 (1971). F. Zachariasen, in Proceedings of the Coral

Gables Conference on Fundamental Interactions at High Energies II. ed.

by A. Perlmutter et al . (Gordon and Breach, New York, 1970) PR 103-122.

This paper contains further references; CERN preprint TH-1290-(1971).

38) See OI, p. 179

39) J. Arafune and H. Sugawara, Phys. Rev. Letters 25, 1516 (1970).

40) See, for example, R. Blankenbecler and M.L. Goldberger, Phys. Rev. 126,

766 (1962). F. Zacha hsen, CERN preprint TH-1284 (1971). R. Oehme,

EFI preprint 71-26 (1971); OII p. /St.

41) V.N. Gribov, I. Yu Kobsarev, V.D. Mur, L.B. Okun and V.S. Popov, Phys. Letters 328, 129 (1970). J. Finkelstein, Phys. Rev. Letters 24, 172

(1970). R.J. Eden and D.G. Kaiser, Cavendish-preprint, (1970).

42) R. Oehme, Lectures delivered at the International Summer Institute for

Theoretical Physics in Heidelberg, July 1970; OII p. ISI ; EFI-

preprint 71-26 (1971).

43) S.M. Roy and V. Singh, Phys. Letters 328, 50 (1970). J. Finkelstein

and S.M. Roy, Phys. Letters 348, 322 (1971). - 44 -

Refs. (cont.)

44) S.M. Roy, Phys. Letters 348, 407 (1971). G. Auberson, T. Kinoshita

and A. Marti,i Cornell-preprint CLNS-144 (1971).

45) R. Oehme, Phys. Rev. Letters 18, 1222 (1967). D.D. Friedman, EFI- -

preprint 71-25 (1971).

46) H. Cheng and T.T. Wu, Phys. Rev. J. Finkel- Letters 24, 1456 (1970). · i

stein and F. Zachariasen, CERN-preprint TH-1298 (1971). A.A. Anselm,

G.S. Danilov, I.T. Dyatlov, nd E.M. Levin, Yardern Fiz. 11, 896 (1970).

G. Auberson, T. Kinoshita and A. Martin, Cornell-preprint CLNS-144 (1971).

47) K. Wilson, Phys. Rev. 179, 1499 (1969).

I 't .

't.