arXiv:hep-ph/9411217v1 3 Nov 1994
DESY 94-197
hep-ph/9411217
Towards the Phenomenology of
QCD–Instanton Induced Particle Production
at HERA∗
A. Ringwald and F. Schrempp
Deutsches Elektronen-Synchrotron DESY, Hamburg, Germany
Abstract
We present a first status report on a broad and systematic study
of possible manifestations of QCD-instantons at HERA. Considerable
motivation comes from the close analogy between instanton-induced
B + L violation in electroweak processes and effects of QCD-instantons
in deep inelastic scattering. We concentrate on the high multiplicity final state structure, reminiscent of an isotropically decaying “fireball”.
A set of experimental isolation criteria is proposed. They serve to
further enhance the striking event signature without significantly suppressing the expected rates.
∗
to pe published in Proc. of the International Seminar “Quarks–94”, Vladimir/Russia,
May 11-18, 1994
1
Introduction
The basic significance and possible importance of QCD-instanton effects in
deep inelastic scattering for decreasing Bjorken variable xBj and high photon
virtuality Q2 has recently been emphasized [1].
First of all, it has been argued [2, 1] that the calculable small scale
instanton dynamics [3] may be factorized from the large distance effects,
allowing for a semiquantitative estimate of instanton-induced contributions
to the structure functions
[1] and the hadronic final state [4]. This is rooted
p
in the fact that 1/ Q2 plays the rôle of a dynamical infrared cut-off for the
instanton size [3].
Secondly, QCD-instanton effects for decreasing xBj are largely analogous to the manifestation of electroweak instantons for increasing energies
[3]. The anomalous B + L violation due to electroweak instantons is paralleled by a chirality violation induced by QCD-instantons [5]. The spectacular
possibility of a strong increase of multi-W ± /Z 0 production in the multi-TeV
regime [6, 7] due to electroweak instantons corresponds to a strong enhancement of multi-gluon production at small xBj due to QCD-instantons. Striking consequences include a high multiplicity final state structure, reminiscent
of a decaying “fireball”.
Whereas a promising search for anomalous electroweak events is only
possible in the far future, presumably at a post-LHC collider [8] or at cosmic
ray facilities [9], the search for anomalous events induced by QCD-instantons
can start right now, in deep inelastic e± p scattering at HERA.
The present paper represents a first status report on a broad and systematic study of possible manifestations of QCD-instantons which could be
searched for at HERA [4]. While a theoretical derivation of crucial quantities characterizing the instanton-induced final state (1, 2 . . . particle inclusive
rates, average multiplicity, average transverse momenta, energy flow, etc.)
will be deferred to Ref. [4], we mainly report here on the phenomenological
aspects of our results.
The organization of this contribution is as follows. We start off
in Section 2 by expanding on the close analogy between instanton-induced
B + L violation in electroweak processes and effects of QCD-instantons in
deep inelastic scattering. Section 3 contains a summary of the results of Balitsky and Braun [1] concerning the QCD-instanton induced contribution to
the gluon and quark structure functions. We also emphasize the approximations and limitations inherent in this calculation. Furthermore, we present
the instanton contribution to the nucleon structure function F2 (xBj , Q2 )
2
obtained by convoluting the results of Ref. [1] with phenomenological distributions of quarks and gluons in the nucleon. In Section 4 we report on our
ongoing investigation [4] of the QCD-instanton induced hadronic final state
in deep inelastic scattering. The main emphasis rests on the characteristic
event topology along with a discussion of experimental isolation criteria,
serving to further enhance the striking event signature without significantly
suppressing the rates. A search strategy for instanton-induced events is formulated. In Section 5, we present a summary and an outlook on related
aspects and open problems under study.
2
The QFD – QCD Connection
The Standard Model of electroweak (QFD) and strong (QCD) interactions
is remarkably successful. In particular, its perturbative formulation (“Feynman diagrammatics”) appears to be theoretically consistent and agrees with
precision experiments (where applicable, i.e. for small coupling constant).
Nevertheless, even for small couplings, there exist physical processes
which cannot be described by conventional perturbation theory, notably,
phenomena associated with quantum tunnelling.
In non-Abelian gauge theories such as QFD and QCD the vacuum
actually has a complicated structure, even on the classical level [10]: The potential energy is periodic with respect to the so-called Chern-Simons number
(c. f. Fig. 1),
g2
NCS [A] =
16π 2
Z
3
d x
ǫijk Aai ∂j Aak
g
− ǫabc Aai Abj Ack ,
3
(1)
which is the (topological) winding number of the (non-Abelian) gauge field
(A) under consideration. Pure gauge fields corresponding to the degenerate
minima of the potential energy (perturbative vacua) have integer values of
the Chern-Simons number NCS . Moreover, pure gauge fields differing by
△NCS = n = integer are topologically inequivalent. They are related to
each other by a topologically non-trivial static gauge transformation with
winding number n. This means that they are separated by an energy barrier,
as shown schematically in Fig. 1.
In the electroweak theory a mass scale, v ≈ 246 GeV, is introduced
via spontaneous symmetry breaking and, correspondingly, there is a definite
3
-2
-1
0
NCS
1
2
Figure 1: Schematic illustration of the static potential energy of the gauge (and
Higgs) field vs. the Chern-Simons number
minimum barrier height associated with the W -mass, of order [11]
QFD
Mbarrier
∼
mW
∼ O(10 TeV).
αW
(2)
As is well known, this minimum barrier energy is associated with a certain static, unstable solution to the classical field equations, the so-called
‘sphaleron’ [11]. It may be viewed [12] as an intermediate, coherent field
configuration consisting of a large number, O(1/αW ), of W/Z (and Higgs)
bosons, confined to a characteristic volume of order m−3
W .
In QCD, being an “unbroken” gauge theory, the minimum barrier
height depends on the considered process and its kinematics. It turns out,
that the notion of the minimum barrier may be qualitatively transcribed
from QFD, provided that there is a (process dependent) hard scale Q′ available. Specifically, in deep inelastic e± p scattering,
Q′ 2 ∝ Q2 = −(mass)2 of the virtual photon.
(3)
Besides αW → αs , one is then led to substitute the characteristic linear
dimension [3, 2, 1, 13]
1
1
→
.
(4)
mW
αs (Q′ )Q′
The minimum barrier energy ( from Eqs. (2, 4))
QCD
∼ Q′ ,
Mbarrier
4
(5)
is now associated with a sphaleron-like intermediate, coherent field configuration consisting of a large number, O(1/αs ), of gluons in a characteristic
volume (αs Q′ )−3 .
Transitions between minima of the effective potential in Fig. 1 lead
to a violation of fermionic quantum numbers in the Standard Model [5, 14].
In particular, baryon (B) and lepton (L) number conservation is violated
due to non-perturbative electroweak gauge fields (W ) associated with the
SU(2) flavour gauge group, according to the selection rule
△Le, µ, τ =
1
△B = −△NCS [W ].
3
(6)
In analogy, non-perturbative gluon fields (G) associated with the SU(3)
colour gauge group induce a violation of chirality conservation for (massless)
quarks,
△Q5u, d, s, ... = 2 △NCS [G].
(7)
√
For parton-parton center of mass (c.m.) energies1 s′ < Mbarrier ,
such processes are classically forbidden and only occur via quantum tunnelling under the barrier in Fig. 1. In this case, the sphaleron-like intermediate state corresponding to the energies (2), (5) can only be reached
virtually. Correspondingly, the respective cross sections are exponentially
suppressed in the coupling [5],
σtunnelling ∼ exp(−4π/α) ;
α = αW , αs .
(8)
Let us recall the origin of this tunnelling suppression factor in somewhat more detail. The amplitude of anomalous fermion number violating
processes can be obtained by expanding the path integral for the corresponding Green’s functions about instantons [15, 5, 16], which are classical solutions of the Yang-Mills(-Higgs) equations in 4-dimensional Euclidean space
with finite action. The instanton (I) (anti-instanton (I)) may be viewed as a
most probable tunnelling solution, interpolating in Euclidean time between
the gauge (and Higgs) field configurations of two neighbouring vacua with
△NCS = +1(−1). It passes the above-mentioned sphaleron-like intermediate state in-between.
√
Henceforth, we√ shall denote by s′ the total c.m. energy of the non-perturbative
subprocess, while s refers to the total c.m. energy of the physical process under
consideration.
1
5
In QCD, for example, the instanton is explicitly given by2
Gµ(I) (x − xI ; UI , ρI ) = −
i UI [σµ (x̄ − x̄I ) − (x − xI )µ ]ŪI 2
ρI ,
g (x − xI )2 ((x − xI )2 + ρ2I )
(9)
depending on a set of collective coordinates {xI , ρI , UI }, like center, xI ,
size, ρI , and orientation in group space, UI . Since the action is independent
(QCD) or only slightly depends (QFD) on these collective coordinates, they
are to be integrated over. For the simplest exclusive anomalous processes
one obtains (for QFD, see Refs. [5, 6], for QCD, see Refs. [3, 2, 1]) in this
way to exponential accuracy:
△(B + L) = −2nfamily = −6 :
T (qq → 7q3l ) ∝
Z
dρI
2π
QFD
(ρI ) ,
... exp −
−1 SI
αW (ρI )
(10)
△Q5 = 2nf = 6 :
T (g∗ g
∗
→ 3qL 3qR )
Z
2π
→ 2qL 3qR )
T (qL g
QCD
′
∝ dρI ... exp −Q ρI −
S
,
T (qL ∗ qR → 2qL 2qR )
αs (ρ−1
) I
I
···
(11)
where, in our normalization, the action of the QCD-instanton is given by
SIQCD = 1, whereas the action of the QFD-instanton reads SIQFD = 1 +
(1/2)ρ2I m2W . In the various QCD-instanton induced subprocesses of Eq. (11),
the star indicates that the corresponding parton carries a virtuality Q′ =
p
−q ′ 2 > 0. We observe that, for exclusive anomalous processes, the instanton size is effectively cut off at ρcut ∼ v −1 in the electroweak theory [5, 16]
and at ρcut ∼ Q′ −1 in QCD [3, 2, 1] (for early discussions, see Ref. [17]).
Most interesting from a theoretical point of √
view and in the light of
present and future collider experiments is the case s′ > Mbarrier , where a
transition over the barrier is classically allowed, i.e. energetically possible.
Unfortunately, the crucial dynamical question is still unsettled [7] whether
the transition from a state with a few initial partons to the very different
sphaleron-like multi-parton coherent state can proceed without extra suppression. Only then could such anomalous processes acquire an observable
We use here the notations σµαα̇ = (−iσ, 1), σ̄µα̇α = (+iσ, 1) (σ are the standard Pauli
matrices). Furthermore we abbreviate x = xµ σµ , x̄ = xµ σ̄µ , etc.
2
6
cross section and the final state would consist of a large number, O(α−1
W (s) ),
of W/Z’s (gluons) in addition to the few fermions required by the anomaly.
The possibility that this intriguing scenario might be realized in
nature was first observed in the context of the electroweak theory in Ref. [6].
It was found [18] that, to exponential accuracy, the total cross section for
anomalous B + L violation, in the high energy and weak coupling limit,
√
√
αW s′
s′
→ ∞,
fixed,
(12)
mW
mW
can be written in the following scaling form
(I) tot
σQFD
√ !#
s′
,
M0
"
4π
QFD
∝ exp −
−1 F
αW (ρ∗ )
(13)
√
where M0 = 6πmW /αW is of the order of the minimum barrier height Eq.
(2). The so-called “holy-grail” function F in the exponent is known only in
a low energy expansion whose first few terms are given by [19]
F QFD (ǫ) = 1 −
9 4/3
9 2
ǫ +
ǫ + O(ǫ8/3 [1 + ln ǫ]),
8
16
(14)
√
where ǫ = s′ /M0 . The effective instanton size entering the running coupling in (13) scales like m−1
W ,
1
ρ∗ =
mW
"r
#
3 2/3
ǫ + ··· .
2
(15)
Note, that the first term in the series expression for the holy grail function,
Eq. (14), corresponds to the “naive” tunnelling factor, Eq. (8).√Apparently,
the total cross section is exponentially growing for (mW ≪) s′ ≪ M0 ,
but still small within the region of validity of expansion (14). As anticipated
above, in this energy region, it is dominated by the associated production
of a large number of W and Z bosons,
h nW i =
π
αW
3 4/3
ǫ + O(ǫ2 ) .
2
(16)
Unfortunately,
nothing is known about the behaviour of the holy grail func√
QFD
′
. The different terms
tion for s around or above the barrier energy Mbarrier
in the perturbative expansion of F QFD become comparable in size, and the
7
perturbative expansion breaks down, just in this most interesting region.
Unitarity and other arguments along with various assumptions have been
used to argue [20] that the decrease of the holy grail function may well level
off at values of order F QFD ≃ 1/2, leading to unobservably small cross sections of electroweak B + L violation. However, this question is not finally
settled.
It is very remarkable that the contribution of QCD-instantons to
deep inelastic scattering strongly ressembles Eqs. (13)-(16), as first observed
for g∗ g scattering in Refs. [3, 2] and elaborated for γ ∗ g scattering in Ref.
[1]. In the Bjorken limit (c. f. Fig. 2 for the kinematics),
)
Q′ 2
fixed,
2pq ′
(17)
the total subprocess cross section for instanton-induced chirality violation is
found to have the following structure
Q′ 2 = −q ′ 2 ,
2
c. m. energy of I-subprocess, s′ = (q ′ + p)2
(I) tot
σQCD
→ ∞ ; x′ =
#
"
4π
F QCD (x′ ) ,
∝ exp −
αs (ρ−1
∗ )
(18)
where [3, 2, 1]
F
QCD
3
(x ) = 1 −
2
′
ρ∗ =
1 − x′
1 + x′
2
+O
"
4π
1 − x′
3
αs (Q′ )Q′
1 + x′
2
1 − x′
1 + x′
4
1 − x′
1 + ln
1 + x′
#
+ ··· .
!
,
(19)
The effective instanton size ρ∗ in Eqs. (18, 19), acting as the characteristic
linear dimension, as well as the scaling form of F QCD (x′ ) are in accordance
with the substitution rule (4) from QFD to QCD. The average gluon multiplicity is found to be [4],
π
h ng i =
αs
"
1 − x′
6
1 + x′
2
+O
1 − x′
1 + x′
3 !#
.
(20)
It is exactly this similarity between QFD and QCD instanton-induced scattering processes which makes the study of the latter at HERA so
interesting.
8
3
Instanton-Induced Contributions to Structure
Functions
In this Section, let us sketch the essential steps in the pioneering calculation of QCD-instanton contributions to the (nucleon) structure functions in
Ref. [1]. Along the way, we shall emphasize the basic ingredients as well
as the inherent limitations. Finally, a state of the art evaluation of the
I-induced contribution to the F2 structure function of the proton will be
presented.
First of all, it is argued [1] that the celebrated factorization theorem
remains valid beyond conventional perturbation theory and allows to express
the instanton contribution to the nucleon structure functions F1, 2 in the
familiar form
!
Q2
x, 2 , αs (µ2 ) .
= ai (xBj )
µ
p=g,q,q̄ xBj
(21)
In Eq. (21), a1 = 1/2, a2 (xBj ) = xBj , x is the Bjorken variable of the γ ∗ parton subprocess , and µ is the factorization scale separating “hard” and
“soft” contributions to the cross section. The distributions p(z, µ) of partons p in the nucleon absorb all information about the dynamics at large
distances and, as usual, are to be taken from experiment. By virtue of
Eq. (21), the theoretical efforts in Ref.
[1] concentrate
on calculating the
(I) p
Q2
2
“parton” structure functions Fi
x, µ2 , αs (µ ) in the instanton background. For a detailed discussion on the familiar and important problem of
infrared (IR) divergencies (associated with integrations over the instanton
size), we have to refer to Ref. [1]. In summary, it is claimed that these divergencies may be consistently absorbed into the parton distributions p(z, µ),
and an unambiguous, IR-protected contribution from small instantons may
be isolated.
According to the optical theorem the parton structure functions
(I) p
Fi
are related to the imaginary part of the forward virtual photon-parton
matrix element (c.f. Fig. 2)
X Z
(I)
Fi (xBj , Q2 )
parton
Tµν
=i
Z
1
xBj
dx
p
,µ
x
x
(I) p
Fi
d4 z eiqz h parton(p), λ |T {jµ (z)jν (0)}| parton(p), λ i.
(22)
The calculation of the instanton-induced contribution to the parton
structure functions then involves the following steps:
9
• The path integral expression for the matrix element (22) in Euclidean
space is expanded about the instanton/anti-instanton pair configuration, defined via the so-called valley method [3, 21]3 .
• Next, the integrations over the large number of collective coordinates
associated with the II configuration have to be performed.
• After Fourier transformation, the last step consists in rotating the
result to Minkowski space and, thereafter, taking the imaginary part.
After a long and tedious calculation, heavily exploiting the light-cone
approximation, Balitsky and Braun [1] succeeded in performing these steps.
Their final answer for the instanton-induced contribution to the gluon and
quark structure functions, derived in the Bjorken limit (c. f. Fig. 2),
Q2 = −q 2 ,
γ ∗ –parton c. m. energy2 , ŝ = (q + p)2
)
→∞; x=
Q2
fixed,
2pq
(23)
reads:
(I) g
F1, 2 (x, Q2 ) ≃
X
e2q
q
×
d2 π 9/2
1
9(1 − x)2 bS(ξ∗ )[bS(ξ∗ ) − 1]
2π
αs (ρ−1
∗ )
!19/2
"
exp −
16
ξ∗3
nf −3
!
d2 π 9/2
128
1
e2q′ + e2q
2
81(1 − x)3 bS(ξ∗ )[bS(ξ∗ ) − 1]
q ′ 6=q
(I) q
F1, 2 (x, Q2 ) ≃
X
×
2π
αs (ρ−1
∗ )
!15/2
"
exp −
#
4π
+ 2b S(ξ∗ ) ,
αs (ρ−1
∗ )
!
16
ξ∗3
#
4π
+ 2b S(ξ∗ ) ,
αs (ρ−1
∗ )
(24)
nf −3
(25)
where eq are the electric charges of the quarks, b = 11 − (2/3)nf , and
d ≃ 0.00363 (for nf = 3 massless flavours) is a constant which enters the
expression for the instanton density [5].
The classical action of the instanton/anti-instanton pair, S(ξ), is the
most important ingredient in Eqs. (24, 25), since it enters in the exponent.
3
For any fixed values of the collective coordinates {τ }, the pair configuration (II
“valley”) is required to minimize the action within the subspace orthogonal to ∂GII /∂τi .
10
q
q
q’
q’
_
_
p
p
g
g
q
a)
q
b)
Figure 2: The contribution of an II pair to to the structure function of a gluon (a)
and of a quark (b). Solid lines are quark zero modes in the case that they are ending
at the instanton (anti-instanton), and quark propagators in the II background
otherwise. Note that the black blobs denoted by I(I) are often referred to in the
text as the I(I)-subprocess.
Due to conformal invariance, it only depends on the following combination
[3, 21] of collective coordinates,
ξ=
R2 + ρ2I + ρI2
ρI ρI
,
(26)
with R2 = (xI − xI )2 being the instanton – anti-instanton separation, and
ρI , ρI their sizes, respectively. For large ξ, the action ressembles a “dipole”
form [22, 3, 21]
6
S(ξ) = 1 − 2 + O(ln(ξ)/ξ 4 ).
(27)
ξ
Finally, in this “dipole” approximation, the effective conformal parameter
11
ξ∗ and instanton size ρ∗ entering Eqs. (24, 25), read
1+x
,
1−x
4π 12
.
αs (Q)Q ξ∗2
ξ∗ ≃ 2
(28)
ρ∗ ≃
(29)
At this point a number of important remarks should be made.
Despite the complications associated with the γ ∗ -parton dynamics (c.f. Fig. 2), the gluon and quark structure functions (24, 25) apparently exhibit the typical signatures of an individual I-subprocess cross section (18, 19). Of course, the I-subprocess variables x′ , Q′ appearing in
Eqs. (18, 19) are integrated over here (c.f. also Fig. 2) and effectively substituted by the appropriate γ ∗ -parton variables x, Q. Let us note, in particular, that the approximate expressions (28, 29) agree with the solutions
of the “saddle-point equations” – associated with the integrations over the
collective coordinates – in case of an individual I-subprocess [3, 2].
The applicability of Eqs. (24, 25) is restricted to sufficiently large x
(c. f. Eq. (28)), since their derivation was based on the large ξ (“dipole”)
approximation
(27) for the action. A further technical requirement is 1−x ≫
q
αs (ρ−1
∗ ), excluding the neighbourhood of x = 1.
In general, the II interaction, Uint (ξ∗ ) = S(ξ∗ ) − 1, describes the
emission and absorption of gluons from the instanton to the anti-instanton
and vice versa (wavy lines between instanton and anti-instanton in Fig. 2).
It generates via the Cutkovsky rules all final state tree-graph corrections to
the leading semi-classical result (for a formal proof, see Ref. [23]). These
final state corrections are well known to exponentiate [18]. However, it has
been argued that some initial state and initial state – final state corrections
exponentiate as well [24] and might give rise to additional corrections of
order 4π/αs O((1 − x)5 ) in the exponent.
The pre-exponential factor in Eqs. (24, 25) is calculated only to leading accuracy in the strong coupling and up to corrections of order O(1 − x).
This is largely due to the fact, that I – I interactions have been essentially
neglected in the prefactor, unlike the II action in the exponent.
• On the one hand, this refers to the treatment of the “current quark”
propagating in the II background (c. f. Fig. 2). Its presence gives
rise to great technical complications and, correspondingly, the results
(24, 25) only account for the first nontrivial terms in the cluster expan-
12
6
2 and 1 [GeV]
5
Q=100
4
3
Q=50
2
1
Q=10
0.1
0.2
0.3
0.4
x
0.5
0.6
0.7
0.8
Figure 3: The effective conformal parameter ξ∗ − 2 (solid) and inverse instanton
size ρ−1
∗ (dashed), obtained as solutions of the saddle point equations, Eq. (30), for
a range of Q values (in GeV) and nf = 3.
sion [25] of the full current quark propagator in terms of the known
propagator [26] in the background of a single (anti-)instanton.
• On the other hand, this refers to the evaluation of the functional determinants entering the pre-exponential factor. An improvement based
on the II valley is under way [27].
Despite these considerable formal restrictions in the derivation of
the gluon and quark structure functions (24, 25), it is tempting to try and
evaluate these results within an experimentally accessible regime of xBj and
Q2 . In order to hopefully enlarge the kinematical region where Eqs. (24, 25)
may be qualitatively trusted, we have heuristically applied the following
“improvement” steps [4] (see also Ref. [1]):
• Throughout, in Eqs. (24, 25), we use the II valley action S(ξ) of
Refs. [3, 21], rather than its “dipole” approximation (27). This action represents an extension of Eq. (27) to arbitray values of ξ ≥ 2. It
is worth pointing out that it continuously interpolates between S = 1
(the sum of individual instanton and anti-instanton actions) at large ξ,
and S = 0 for ξ = 2. These limiting situations correspond to a widely
13
separated, non-interacting II-pair for ξ → ∞ and the perturbative
configuration of a collapsing and annihilating II-pair for ξ → 2 (i.e.
for R → 0, ρI = ρI ).
• We replace the approximate expressions (28, 29) for the effective conformal parameter ξ∗ and instanton size ρ∗ , respectively, by the solutions of the exact “saddle-point” equations [3, 2, 1],
√
8π p
ŝρ∗ =
ξ∗ − 2 S ′ (ξ∗ ) ,
(30)
)
αs (ρ−1
∗
4π
∂
2π
′
Qρ∗ =
(ξ∗ − 2)S (ξ∗ ) − ρ∗
S(ξ∗ ) ,
∂ρ∗ αs (ρ−1
αs (ρ−1
∗ )
∗ )
where S ′ (ξ) is the derivative of the valley action S(ξ) with respect to ξ.
We have numerically solved Eqs. (30) (see Fig. 3), using the two-loop
expression for the running coupling αs (ρ−1
∗ ) with three active flavors,
(3)
and the value ΛMS = 365 MeV. It corresponds to αs (mτ ) = 0.33 [28].
The I-contribution to the nucleon structure function was finally obtained from convoluting the “improved” Eqs. (24, 25) with very simple phenomenological expressions [29] for the gluon, u quark and d quark distribu√
√
tions, g(z) = (3/z)(1 − z)5 , u(z) = (2/ z)(1 − z)3 , d(z) = (1/ z)(1 − z)3 ,
respectively. In view of the qualitative nature of this study, they turn out to
be quite adequate for a factorization scale µ ≃ ρ−1
∗ , which is natural in this
context. It turns out that over the whole xBj range considered the γ ∗ g con(I)
tribution to F2 dominates. The sea-quark contributions can be neglected
throughout the xBj range considered.
The resulting instanton-induced contribution to the structure function F2 of the proton is displayed in Fig. 4. The expected very strong rise
of the I-induced contribution with decreasing xBj is both apparent and suggestive!
Unfortunately, any further conclusions directly reflect the (xBj , Q2 )
region where the above approximations are supposed to hold. For instance,
the dashed lines in Fig. 4 define the boundaries of various “fiducial” regions
corresponding to values of S(ξ∗ (xBj , Q2 )) ≥ 0.5, 0.4, 0.3. As mentioned
QCD
= S(ξ∗ )min = 1/2 as a
before, some authors [20] have advocated Fmin
QCD
saturating value for the holy grail function F
. The minimum value of
Q considered in Fig. 4 is determined by the requirement that the effective
instanton size should be sufficiently small. At Q = 10 GeV one finds ρ∗ ≃ 1
GeV−1 (c. f. Fig. 3).
14
(I )
log10 [F2
2
(xBj; Q )]
0
S = 0:3
data
-2
-4
S = 0:4
-6
S = 0:5
-8
Q [GeV]:
-10 0.1
0.2
100
20
50
0.3
0.4
0.5
10
0.6
0.7
0.8
xBj
Figure 4: The logarithm of the instanton-induced contribution to the structure
(I)
function F2 of the proton, log 10 [F2 (xBj , Q2 )], Eq. (21), as a function of xBj ,
for a range of Q values (in GeV) and nf = 3. The curves denoted by “data” are
to roughly represent the trend of the experimental data for F2 within the same
range of Q. The dashed curves correspond to constant values of the valley action,
S(ξ∗ (xBj , Q2 )).
4
Phenomenology of Instanton Induced Particle
Production at HERA
There are three main reasons which favour experimental searches for instanton-induced “footprints” in the multi-particle final state over searches
via the structure functions, being the most inclusive observables in deep
inelastic scattering.
• On the one hand, the only experimental signal for QCD-instantons in
15
the structure functions could be in form of an excess over the expected
inclusive leptoproduction rate. However, enhancements at small xBj
are also expected from other competing mechanisms like “(perturbative) Reggeization”. Therefore, the structure functions are only of
limited value in searches for manifestations of QCD-instantons.
• On the other hand, as we shall see, the instanton-induced final state
is distinguished by a quite spectacular event topology together with a
characteristic flow of flavour quantum numbers.
• Furthermore, the additional possibility of imposing experimental cuts
on kinematical variables of the final state may well allow to restrict
the I-subprocess variables x′ , Q′ , . . . within a theoretically controllable
regime despite small xBj . Along these lines one may hope to bridge
> O(0.1), where
the substantial gap between the regime of larger x′ ∼
the I-subprocess cross sections may be theoretically estimated, and
< O(10−3 ), where the bulk of HERA data is
the small xBj regime, xBj ∼
accumulating at present.
To elaborate on the last two aspects is the purpose of this Section.
A graphical display of the modulus squared of the relevant γ ∗ g matrix element, along with various four-momenta of interest, is presented in
Fig. 5. Its structure suggests that the instanton-induced contribution to the
differential cross sections for γ ∗ g(q) → · · · can be written in a “canonical”
convolution form, as familiar from perturbative QCD:
(I)
dσγ ∗ p (x, Q2 , . . .)
∼
XZ
Q2 /x
p′
dQ′2
Q′2
Z
1
x
dx′ (I)
f ∗ ′
x′ γ p
x ′2
(I)
, Q dσp′ p (x′ , Q′2 , . . .).
x′
(31)
The integrations in Eq. (31) extend over the variables x′ , Q′ 2 , referring as
in Sect. 2 to the instanton-induced subprocess (denoted by I in Fig. 5),
Q′2 = −q ′2
s′
x′ =
= (q ′ + p)2
Q′2
Q′2
=
.
2pq ′
s′ + Q′2
(32)
Their definition is completely analogous to the standard e± N variables Q2 =
−q 2 and xBj = Q2 /2P q referring to the nucleon target of momentum P . The
parton (gluon) momentum fraction with respect to the proton is z = xBj /x =
(pq)/(P q) and
0 < xBj ≤ x ≤ x′ ≤ 1.
(33)
16
q’
~
g(p)
Figure 5:
Graphical display of the instanton-induced contribution to the cross
section of γ ∗ g scattering for ∆Q5 = 2nf = 6.
The conditions for the validity of Eq. (31) (beyond the set of approximations inherent in Ref. [1]), as well as a determination of the “splitting
(I)
function” fγ ∗ p′ (z ′ , Q′2 ), associated with the propagation of the current quark
in the instanton background, are presently under active investigation [30].
To establish a structure of type (31) is quite an important task both from
a theoretical point of view and also for further studies of instanton-induced
phenomenology by means of Monte Carlo methods [31]. For the time being,
we shall simply assume that Eq. (31) is valid approximately.
17
(I)
It is quite plausible that the “splitting function” fγ ∗ p′ (z ′ , Q′2 ) in
Eq. (31) only exhibits a relatively mild dependence on its variables. In
(I)
contrast, the I-subprocess cross sections dσp′ p (x′ , Q′2 , . . .) bring in the main
dependences (of exponential type) and, of course, are most interesting from
the physics point of view. Accordingly, we have concentrated our theoretical
efforts in Ref. [4] on calculating the crucial observables characterizing the
I-subprocess, such as normalized 1, 2, . . .-parton inclusive cross sections,
1
(I) tot
σp′ p (x′ , Q′2 )
(I)
dσp′ p (x′ , Q′2 , . . .),
(34)
along with the respective average parton multiplicities, transverse momentum (flow), etc. Corresponding to the restrictions discussed in Sect. 3 in the
context of the structure functions, the I-subprocess variables should not be
> O(0.1), Q′ > O(10 GeV), say.
too small, x′ ∼
∼
Since a calculation of the “splitting function” in Eq. (31) is still under
way [30], a discussion of expected event rates has to be deferred to a later
stage. In the present analysis, we only make use of information abstracted
from our calculations of the I-subprocess observables [4] along with HERA
kinematics. This is sufficient, however, to obtain important insight into
the expected event topology in the most interesting regime of small xBj .
Moreover, the connection between kinematical quantities measurable in the
laboratory system and the variables controlling the instanton subprocess
may be studied.
Specifically, we use the following set of working hypotheses about
the I-subprocess:
i) Isotropy: In its c.m. system, q~′ +~
p = 0, the instanton-induced multi-parton
production is supposed to proceed isotropically. We may imagine a “fireball”
in S-wave configuration, decaying into gluons and at least 2nf − 1 quarks,
including strangeness (!) and possibly charm, if kinematically allowed (c. f.
Fig. 5).
(I)
ii) Dependence on x′ , Q′ 2 : The I-subprocess cross sections dσp′ p (x′ , Q′2 , . . .)
are expected to strongly decrease with increasing Q′2 for fixed x′ and to
strongly increase with decreasing x′ for fixed Q′2 (c. f. Sect. 2). As discussed
above and in Sect. 3, it remains uncertain, however, how long the cross
sections continue to increase towards x′ → 0.
18
iii) Multiplicity: The total multiplicity associated with the I-subprocess is
expected to be large,
π
hng+q (x , Q )i ∼ O
2αs
′
′2
> O(10),
+ 2nf − 1 ∼
(35)
on the parton level, leading typically to O(20÷30) particles after hadronization. In Fig. 6, we display hng+q (x′ , Q′2 )i as calculated in Ref. [4].
At small values of x′ and large Q′2 , the multiplicity obtains a large
contribution from gluons and peaks around x′ ≈ 0.2 ÷ 0.3, whereas at large
x′ the 2nf − 1 = 5 produced quarks dominate. The peaking of the gluon
multiplicity at small, non-vanishing x′ actually has an appealing interpretation:
For large values of Q′2 the coefficient of π/2αs in Eq. (35) turns
out to be [4] 4(ξ∗ − 2) S ′ (ξ∗ ), involving the derivative of the valley action with respect to the conformal parameter ξ, taken at the saddle point
value ξ∗ (x′ , Q′2 ) (c.f. Fig. 3). As discussed in Sect. 3, the full valley action smoothly interpolates between a non-interacting, infinitely separated
instanton/anti-instanton pair for ξ → ∞ (probed for x′ → 1) and the perturbative vacuum for ξ → 2 (probed for x′ → 0). Hence, in both limits
a decrease of the gluon multiplicity matches well the intuition! The peak
of the multiplicity inbetween corresponds to the maximal variation of the
action with ξ.
We also note the substantial increase of the gluon multiplicity with
increasing Q′2 , which at large Q′2 mainly reflects the running of αs in Eq.
(35).
iv) k⊥ signature: The transverse momenta of the partons emerging from the
instanton subprocess and the one of the current-quark jet (c.f. Fig. 5) are
expected to be “semi hard”, typically of order [4, 1]
√
√
π
s′
s′
< k⊥ tot >
=
∼ αs
; i ⊂ I, and
(36)
|k⊥ i | ∼
<n>
4<n>
2
|k⊥ current
quark | ∼
q
αs Q2 .
(37)
Given this plausible generic input i) - iv), we may now ask, how instantoninduced events would look like in the H1/ZEUS detectors.
First of all, we observe that as a direct consequence of the isotropy
assumption i), the (pseudo) rapidity distribution of a single final state parton
19
hng+q (x0 ; Q0 2)i
Q’ [GeV]
14
100
12
50
10
20
8
10
6
4
2
0 0.1
0.2
0.3
0.4
0
0.5
0.6
0.7
0.8
x
Figure 6: The average, total parton multiplicity associated with the I -subprocess
as a function of x′ , for different values of Q′ and nf = 3, from Ref. [4].
in the I-c.m. system takes the form
1 < n(x′ , Q′2 ) >
dσ (I ) (x′ , Q′2 , ηI )
=
,
dηI dφI
4π cosh(ηI )2
σ (I ) tot
1
(38)
i.e. it is strongly peaked in (pseudo) rapidity ηI = − ln tan(θI /2) around
ηI = 0 with a half width of
∆ηI ≈ ±0.9.
(39)
The shape and width of the distribution in pseudo rapidity remains, of
course, very similar in the HERA laboratory system, for kinematical configurations where the I-c.m. system is dominantly boosted longitudinally.
Depending on the values of the various subprocess variables, the peak position (ηI = 0) fluctuates in general over the available range of η lab (for given
20
xBj and y viz. Q2 ):
ηIlab
=
1
ln
2
EP xBj 1 − x′
x′
+ xγ (1 − y) + (1 − xγ )( − 1)
yEe xγ
x
x
s
x′
−2 (1 − y)xγ (1 − xγ )( − 1) cos χ .
x
(40)
In analogy to the standard y variable, we have introduced in Eq. (40) the q ′
momentum fraction
q′ p
0 < xγ =
< 1.
(41)
qp
The variable χ denotes the azimuthal angle of the vector q~′ in the HERA laboratory frame. Due to momentum conservation, |~q⊥′ | sin χ = −ky current quark ,
the component of the current-quark momentum out of the ee′ P scattering
plane.
In Fig. 7, the dominant matrix element and (η lab , φlab )-plot of a typical instanton-induced event is contrasted with the canonical two-jet configuration in perturbative QCD.
Clearly, the “0th level” signature to watch out for is a densely populated hadronic “band” in the (η lab , φlab )-plane, centered at a fluctuating
value (40) of ηIlab . This striking multi-hadron final state originates from
8 ÷ 10 “semi-hard” jets (c. f. Fig. 6), always includes strangeness and is
characterized by a width △ηIlab = ±0.9. Let us point out two observables,
which – on an event-by-event basis – appear to be particularly sensitive to
this event structure.
• The (transverse) energy flow, dE(⊥) /dη lab (integrated over φlab ), will
exhibit a strong enhancement at the position η lab = ηIlab of the “band”,
since each of the 8÷10 instanton-induced jets contributes a comparable
energy into a single η lab bin of width ≈ 1.8. If, in addition, the currentquark jet is isolated from the “band” (see below), one even expects a
double-peak structure in dE(⊥) /dη lab . The energy flow signature may
well be less affected by hadronization than patterns associated with
individual tracks.
• Pseudo sphericity: The usual event-shape variables like sphericity and
aplanarity should be useful tools in analysing the manifestations of
an isotropic instanton-induced subprocess in the final state. Of particular sensitivity appears the so-called pseudo sphericity [32], which
21
e’
e’
e
e
jet
jet
O(20) hadrons
jet
g
g
P
P
Conventional DIS (2 jets)
360
QCD-Instanton Induced DIS
360
isotropy, strangeness (charm)!
jet
180
180
jet
jet
0
0
-4
0
4
-4
0
4
The dominant matrix element and (η lab , φlab )-plot of a typical
instanton-induced event is contrasted with the canonical two-jet configuration in
perturbative QCD.
Figure 7:
22
incorporates only transverse information from the event in terms of
the azimuthal angles φi of the N final state hadrons:
v
u N
N
X
X
1u
t
2
Pseudo sphericity = 1 −
( cos φi ) + ( sin φi )2 .
N
i=1
(42)
i=1
Apparently, it equals to 1 in the c.m. system of an isotropical event
and vanishes for a single “collimated” jet.
As a next level of sophistication, we study the effects of kinematical cuts on suitable final-state variables with the aim, to further enhance
the event topology and to unfold and/or restrict the I-subprocess variables
x′ , Q′ . Of course, this has to be achieved
• without affecting significantly the expected size of the I-subprocess
cross section dσ (I) (by exploring input ii) above);
• such that the I-subprocess is invoked in a kinematical region of (x′ , Q′ ),
where it induces a high average multiplicity hng+q i according to Fig. 6.
The key aspect is to focus on an event topology corresponding
p to an
isolated (semi-hard) current-quark jet (c. f. input iv) above: k⊥ ≈ αs Q2 )
in addition to a hadronic “band” in (η lab , φlab ) as discussed in “level 0”
above. To this end, let us consider the constraints on the (internal) subprocess variables xγ , x′ , Q′ . . ., implied by the following reasonable separation
criteria:
• The hadronic “band” should be contained in the (central) detector,
< 1, say (in practice, this
such that its peak position satisfies |ηIlab | ∼
upper bound for ηIlab may well be pushed up to ∼ 2).
• The current-quark jet is required to be separated in η lab from the
hadronic “band” (centered around ηIlab ) by
lab
△η ≡ ηIlab − ηcurrent
quark
(
<
∼ − 1.5 or
>
∼ + 1.5
• A minimal transverse momentum, k⊥ current
for the current-quark jet.
23
>4
quark ∼
(43)
GeV, is required
In Fig. 8 we have displayed the resulting restrictions on the internal
subprocess variables xγ , x′ , for a typical set of fixed “external” parameters xBj ,y,x. Apparently, after imposing the isolation requirements for the
current-quark jet we are left with two allowed, ‘triangular’ regions 1 and 2,
in the (xγ , x′ )-plane. The central portion of Fig. 8 is excluded by the cut
on △η (solid lines), with the left- (right-) hand boundary corresponding to
△η = +1.5 (−1.5). The excluded portion on the left (short dashes) refers
to the hadronic “band” being centered within 1 ≤ ηIlab ≤ 2.2, with ηIlab = 1
located on the right. Hence, if a value of ηIlab above 1 is experimentally tolerable, the allowed region 1 increases significantly. Finally, the main effect
of the requirement k⊥ current quark ≥ 4 GeV , is to set a lower limit to the
involved values of x′ , and to exclude the region xγ very close to 1 (long
dashes).
These results demonstrate that, indeed, kinematical cuts of the type
considered here, may well restrict the I-subprocess variables x′ , Q′ to regions
(I )
where the computation [4] of dσp′ p (x′ , Q′ ) may be trusted (e.g. within regime
2 of Fig. 8).
According to our input ii) above and Fig. 9, regime 1 in Fig. 8 will
presumably be associated with considerably higher rates, since it typically
corresponds to much smaller values of Q′ and x′ than regime 2. From Fig. 9
we also infer a comfortably high total √parton multiplicity hng+q i ≈ 8 in
> 3 GeV in the I-c.m. system.
regime 1, as well as an energy/parton = s′ /8 ∼
Let us finally illustrate in Figs. 10, 11 an event in the HERA laboratory frame, corresponding both to a striking signature (isolated currentquark jet along with a densely populated hadronic “band”) and favourable
rate/multiplicity conditions for the instanton subprocess. We note the corresponding event-shape variables (on the parton level in the laboratory frame)
as calculated from the instanton-induced partons within the “band”
(I)
Sphericity|lab ≈ 0.45,
(I)
Aplanarity|lab ≈ 0.22,
(44)
(I)
Pseudo sphericity|lab ≈ 0.90.
Of course, due to the isotropy of the instanton-induced subprocess, the
sphericity, aplanarity and pseudo-sphericity variables essentially adopt their
maximal values of 1, 1/2 and 1, respectively, in the I-c.m. frame. Apparently, the pseudo sphericity is least affected by the Lorentz transformation into the laboratory frame and continues to reflect the underlying
24
1
2
0.8
0.6
x
0
0.4
0.2
1
0.2
0.4
x
0.6
0.8
1
In the displayed regions 1, 2 of the (xγ , x′ )-plane, the current-quark
jet is isolated from the instanton-induced “band” (centered at ηIlab ). The excluded
lab
lab
domains are: −1.5 ≤ △η ≡ ηIlab − ηcurrent
quark ≤ 1.5 (solid lines), 1 ≤ ηI
(short dashes) and k⊥ current quark ≤ 4 GeV (long dashes). The parameters are
Ep = 820 GeV, Ee = 30 GeV, xBj = 0.001, y = 0.5 (Q = 7 GeV), x = 0.025
√
( ŝ = 44 GeV) and q~′ azimuthal angle χ = 0.
Figure 8:
isotropy. Clearly, for a quantitative discussion, hadronization effects have
to be included[31], which may well wash out somewhat the traces of the
underlying isotropy in the various event shape parameters.
5
Summary and Outlook
The search for QCD-instanton induced events at HERA is well worth the
effort:
First of all, these “anomalous” processes are predicted to occur
within standard QCD. Secondly, there is a close analogy to electroweak B +L
25
1
5 GeV
7.2
10 GeV
0.8
7.1
8.4
15 GeV
20 GeV
9.0
0.6
x
0
p
s
0
=25 GeV
9.3
7.6
0.4
9.4
7.7
Q’=20 GeV
7.7
0.2
7.6
Q’=10 GeV
00
0.2
0.4
x
0.6
0.8
1
√
Figure 9: Lines of constant invariant mass of the I -subprocess, s′ , and constant
Q′ (dashed), versus the subprocess variables x′ and xγ , for the same parameters as
in Fig. 8. The numbers at the crossing points denote the respective I -subprocess
multiplicities hng+q i according to Fig. 6.
violating processes, as was discussed in detail in Sect. 2. While a promising
search for anomalous electroweak events is only possible in the far future,
the search for manifestations of QCD-instantons can start right now, in deep
inelastic e± p scattering at HERA.
Besides summarizing the essence and limitations of the theoretical
calculations involved [1], we have presented in Sect. 3 a state of the art evaluation of the instanton-induced contribution to the nucleon structure function
F2 . It rises strongly with decreasing xBj and tends to reach the size of the
experimental data around xBj ≈ 0.1 ÷ 0.25. Unfortunately, due to inher< 0.35,
ent uncertainties, the calculation cannot be trusted anymore for xBj ∼
say. Nevertheless, the trend is very suggestive! However, enhancements of
the inclusive leptoproduction rate at small xBj are also expected from other
competing mechanisms like “(perturbative) Reggeization”. Therefore, the
26
10
kz 0
current quark
-10
-10
e0
0
kx
10
0
10
-10
ky
Figure 10: 3d-momentum display (in GeV) for a typical instanton-induced event
before hadronization, in the HERA laboratory frame, satisfying the kinematical
cuts discussed in the text. The current-quark jet is well isolated. Not shown are
the incoming proton (+z direction) and e± (−z direction), as well as the proton
fragments. The parameters
are as in Fig. 8 and moreover, xγ = 0.32, x′ = 0.1,
√
such that Q′ ≈ 8 GeV, s′ ≈ 24 GeV and hng+q i ≈ 8.
structure functions appear only of limited value in searches for “footprints”
of QCD-instantons.
In Section 4 we have reported first phenomenological results of our
ongoing broad and systematic investigation of the QCD-instanton induced
hadronic final state [4]. Since a calculation of the “splitting function” –
associated with the propagation of the current quark in the instanton background – is still in progress, a discussion of expected event rates has to
be deferred to a later stage. In the present analysis we only made use of
information abstracted from our calculation of the instanton-subprocess observables [4] along with HERA kinematics. This was sufficient, however,
27
10
current quark
8
E?
6
4
2
0
6
4
lab
2
0
-1
0
1
2
3
lab
Figure 11:
Lego plot of the transverse energy in GeV (before hadronization)
for the same instanton-induced event as in Fig. 10, satisfying the kinematical cuts
discussed in the text. Not shown are the scattered e± and the proton fragments.
to obtain important insight into the expected event topology in the most
interesting regime of small xBj .
• The “0th level” signature to watch out for is a densely populated
hadronic “band” in the (η lab , φlab )-plane (c. f. Fig. 7), centered at some
fluctuating value ηIlab . This striking multi-hadron final state originates
from 8 ÷ 10 “semi-hard” jets (c. f. Fig. 6), always includes strangeness
and is characterized by a width △ηIlab = ±0.9. It directly reflects
an underlying instanton-subprocess, associated with the formation of
an S-wave “fireball”, which then decays isotropically into gluons and
at least 2nf − 1 quarks. Observables which are particularly sensitive
to this event structure are e.g. the (transverse) energy flow and the
so-called pseudo sphericity. The energy flow signature may well be
less affected by hadronization than patterns associated with individual
28
tracks.
• As a next level of sophistication, we have studied kinematical cuts on
suitable final-state variables, which help to further enhance the event
topolology and to unfold and/or restrict the (Bjorken) variables of the
instanton subprocess within a theoretically controllable regime, despite
small xBj . Along these lines one may hope to bridge the substantial
gap between the kinematical region, where the instanton-subprocess
cross sections may be theoretically estimated [4], and small xBj val< O(10−3 ), where the bulk of HERA data is accumulating at
ues, xBj ∼
present.
In summary, experimental searches for instanton “footprints” in the multiparticle final state appear to be much more promising than searches via the
structure functions.
Finally, let us briefly mention some related theoretical and phenomenological issues presently under study. Theoretical work is in progress
to improve the pre-exponential factors, affecting quite strongly the predictions for structure functions and the various subprocess cross sections. This
refers in particular to a more reliable evaluation of the functional determinants [27] in the instanton/anti-instanton valley background beyond the
dilute instanton-gas approximation.
Of great importance for further studies of QCD-instanton phenomenology is the task of establishing a convolution form [30] of the γ ∗ -parton
multi-particle cross sections in terms of “splitting functions” and instantonsubprocess cross sections (c. f. Eq. (31)). Once the “splitting functions”
have been isolated and calculated, we hope to come forward with predictions for the rate of instanton-induced multi-particle events. We are then
ready to study the instanton-induced multi-particle final state by means of
a Monte Carlo based event generator [31]. Only after including effects of
hadronization and background will it be possible to address the crucial question: How many “anomalous” events are needed to establish the “discovery”
of an instanton at HERA?
Acknowledgements
We would like to thank W. Bartel, T. Haas, M. Kuhlen and A. de Roeck
for many useful suggestions on experimental issues. Furthermore, we would
29
like to acknowledge helpful discussions with V. Braun, S. Moch, G. Schuler
and C. Wetterich.
References
[1] I. Balitsky and V. Braun, Phys. Lett. B314 (1993) 237.
[2] I. Balitsky and V. Braun, Phys. Rev. D47 (1993) 1879.
[3] V.V. Khoze and A. Ringwald, Phys. Lett. B259 (1991) 106.
[4] A. Ringwald and F. Schrempp, in preparation.
[5] G. ‘t Hooft, Phys. Rev. Lett. 37 (1976) 8; Phys. Rev. D14 (1976) 3432.
[6] A. Ringwald, Nucl. Phys. B330 (1990) 1;
O. Espinosa, Nucl. Phys. B343 (1990) 310.
[7] For a review, see:
M. Mattis, Phys. Rep. 214 (1992) 159;
P. Tinyakov, Int. J. Mod. Phys. A8 (1993) 1823;
R. Guida, K. Konishi, N. Magnoli, Int. J. Mod. Phys. A9 (1994) 795;
I. Balitsky, talk presented at the Workshop ‘Continuous Advances
in QCD’, Minneapolis, 18-20 February 1994, Penn State University
preprint PSU/TH/146 (May 1994), hep-ph 9405335.
[8] G. Farrar and R. Meng, Phys. Rev. Lett. 65 (1990) 3377;
A. Ringwald, F. Schrempp and C. Wetterich, Nucl. Phys. B365 (1991)
3;
M. Gibbs, A. Ringwald, B. Webber and J. Zadrozny, CERN preprint
CERN-TH.7090/93 (June 1994), hep-ph 9406266.
[9] D. Morris and R. Rosenfeld, Phys. Rev. D44 (1991) 3530;
D. Morris and A. Ringwald, Astropart. Phys. 2 (1994) 43.
[10] R. Jackiw and C. Rebbi, Phys. Rev. Lett. 37 (1976) 172;
C. Callan, R. Dashen and D. Gross, Phys. Lett. B63 (1976) 334.
[11] N. Manton, Phys. Rev. D28 (1983) 2019; F. Klinkhamer and N. Manton, Phys. Rev. D30 (1984) 2212.
30
[12] H. Aoyama and H. Goldberg, Phys. Lett. B188 (1987) 506;
P. Arnold and L. McLerran, Phys. Rev. D37 (1988) 1020.
[13] I. Balitsky and V. Braun, DESY preprint DESY 94-179 (October 1994),
hep-ph 9410271.
[14] S. Adler, Phys. Rev. 177 (1969) 2426;
J. Bell and R. Jackiw, Nuovo Cimento 51 (1969) 47;
W.A. Bardeen, Phys. Rev. 184 (1969) 1848.
[15] A. Belavin, A. Polyakov, A. Schwarz and Yu. Tyupkin, Phys. Lett. B59
(1975) 85.
[16] I. Affleck, Nucl. Phys. B191 (1981) 429.
[17] N. Andrei and D. Gross, Phys. Rev. D18 (1978) 468;
L. Baulieu, J. Ellis, M. Gaillard and W. Zakrzewski, Phys. Lett. B77
(1978) 290; ibid. B81 (1979) 41;
T. Appelquist and R. Shankar, Phys. Rev. D18 (1978) 2952;
V. Novikov, M. Shifman, A. Vainshtein and V. Zakharov, Nucl. Phys.
B174 (1980) 378;
M. Dubovikov and A. Smilga, Nucl. Phys. B185 (1981) 109.
[18] L. Yaffe, in: Proc. of the Santa Fe Workshop on Baryon Number Violation at the SSC?, eds. M. Mattis and E. Mottola, (World Scientific,
Singapore, 1990), pp. 46-63.
P. Arnold and M. Mattis, Phys. Rev. D42 (1990) 1738;
S. Khlebnikov, V. Rubakov and P. Tinyakov, Nucl. Phys. B350 (1991)
441.
[19] V. Zakharov, Minnesota preprint TPI-MINN-07/7-T (1990) (unpublished); Nucl. Phys. B371 (1992) 637;
M. Porrati, Nucl. Phys. B347 (1990) 371;
S. Khlebnikov, V. Rubakov and P. Tinyakov, Nucl. Phys. B350 (1991)
441;
V.V. Khoze and A. Ringwald, Nucl. Phys. B355 (1991) 351;
P.Arnold and M.Mattis, Phys. Rev. D44 (1991) 3650;
A. Mueller, Nucl. Phys. B364 (1991) 109;
D. Diakonov and V. Petrov, in: Proc. of the XXVIth LNPI Winter
School, (Leningrad, 1991), pp. 8-64;
I. Balitsky and A. Schäfer, Nucl. Phys. B404 (1993) 639;
P. Silvestrov, Phys. Lett. B323 (1994) 25.
31
[20] V. Zakharov, Nucl. Phys. B353 (1991) 683;
M. Maggiore and M. Shifman, Nucl. Phys. B365 (1991) 161;
G. Veneziano, Mod. Phys. Lett. A7 (1992) 1661;
D. Diakonov and V. Petrov, Phys. Rev. D50 (1994) 266.
[21] A. Yung, Nucl. Phys. B297 (1988) 47;
V.V. Khoze and A. Ringwald, Phys. Lett. B259 (1991) 106;
V.V. Khoze and A. Ringwald, CERN preprint CERN-TH.6082/91 (unpublished);
J. Verbaarschot, Nucl. Phys. B362 (1991) 33;
I. Balitsky and V. Braun, Nucl. Phys. B380 (1992) 51.
[22] C. Callan, R. Dashen and D. Gross, Phys. Rev. D17 (1978) 2717.
[23] P. Arnold and M. Mattis, Phys. Rev. bf D44 (1991) 3650.
[24] A. Mueller, Nucl. Phys. B348 (1991) 310; Nucl. Phys. B353 (1991) 44.
[25] E. Mottola, Phys. Rev. D17 (1978) 1103;
N. Andrei and D. Gross, Phys. Rev. D18 (1978) 468.
[26] L. Brown, R. Carlitz, D. Creamer and C. Lee, Phys. Rev. D17 (1978)
1583.
[27] J. Fuchs, A. Ringwald and F. Schrempp, work in progress.
[28] D. Buskulic et al. (ALEPH Collaboration), Phys. Lett. B307 (1993)
209.
[29] G. Schuler, private communication.
[30] S. Moch, A. Ringwald and F. Schrempp, work in progress.
[31] M. Gibbs, A. Ringwald and F. Schrempp, work in progress.
[32] P. Carlson, in: Proc. 4th Workshop on p̄p collider physics (Bern 1984),
CERN Yellow Report 84-09, p. 286;
J. Rushbrooke, in: Workshop on p̄p options for the supercollider (SSC),
(University of Chicago, February 1984), p. 176;
Ch. Geich-Gimbel, in: The quark structure of matter, (StrassburgKarlsruhe, 1985), (World Scientific, 1986), p. 465.
32