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PHYSICAL REVIEW D VOLUME 5 1, NUMBER 7 1 APRIL 1995 Goldstone bosons in the Appelquist-Terning extended technicolor model Bhashyam Balaji Physics Department, Boston University, Boston, Massachusetts 02215 (Received 25 July 1994) It is demonstrated that the extended technicolor model proposed recently by Appelquist and Terning has a pair of potentially light U(1) Goldstone bosons coupling to ordinary matter with strength 2mf/F,m where mf is the mass of the fermion and F, RZ 125 GeV. These Goldstone bosons could get a mass if the spontaneously broken U(l) symmetries are also explicitly broken, by physics beyond that specified in the model. An attempt to break these symmetries by embedding the model into a larger gauge group seems to be inadequate. The problem is because there are too many representations and there is a mismatch between the number of condensates and the number of gauge symmetries broken. PACS number(s): 12.60.Nz, 11.15.Ex, 14.80.M~ I. INTRODUCTION The reasons for considering the standard model of elec- troweak interactions to be incomplete are well known. In particular, the scalar Higgs sector possesses unsatisfac- tory features such as the naturalness (gauge hierarchy) problem [I], arbitrariness of Yukawa couplings and triv- iality [2]. These are particularly disturbing since elec- troweak symmetry breaking is responsible for endowing ordinary fermions and the weak gauge bosons with their masses. One proposal for eliminating these problems assumes that there are no fundamental Higgs scalars. Instead, one postulates the existence of a new set of fermions, tech- nifermions, which interact via a new parity-conserving strong force called technicolor [3]. Crudely speaking, "standard" technicolor mimics QCD at a higher energy scale. Walking technicolor [4] modifies relations obtained by naive scaling from QCD, due to large anomalous di- mensions of relevant composite operators. Technicolor enables us to solve part of the problem, gauge boson mass generation, based on nontrivial dynamics. The dynamical generation of fermion masses requires vet another interaction: extended technicolor (ETC) [5,6]. It generates the current algebra masses of ordinary fermions by communicating the dynamical technifermion masses to the ordinary fermions. In other words, ETC gauge bosons couple ordinary fermions to technifermions, and couple to the various flavors differently. Three of the Goldstone bosons produced bv the spon- taneous chiral symmetry breaking of techniflavor symme- trv contribute to W" and Z0 masses. "Realistic" models usually contain other (pseudo) Goldstone bosons, most of which acquire some mass from color or electroweak inter- actions [6]. An ETC model explaining the wide range of values of ordinary fermion masses and the Cabibbo-Kobayashi- Maskawa (CKM) matrix elements has been elusive. In particular, it is hard to construct models compatible with experiments. Strong constraints from flavor-changing neutral current (FCNC) experiments ruled out QCD-like models long ago. Moreover, there are unwanted mass- less Goldstone bosons in any extended technicolor model with too many fermion representations [6]. Recently, severe constraints have also come from pre- cision electroweak measurements. Assuming the scale of new physics to be large compared to the W mass, it is found that there are important corrections to electroweak observables that are "obliquen-i.e., correction to gauge boson propagators [7]. These oblique corrections are en- coded in three parameters S, T, and U [a]. The pa- rameter T [9] is a measure of weak-isospin breaking- smallness of T means that technicolor models with large weak isospin breaking (needed to generate the b-t mass difference, for instance) are severely constrained. Calcu- lations of the S parameter in QCD-like technicolor mod- els with isospin symmetry indicates that technicolor mod- els with too many representations (the one-family tech- nicolor model, for instance) are incompatible with the experimental value of S. Of course, those models are al- ready ruled out on other considerations [6]. However, it is unclear if walking technicolor models are incompatible with the experimental values of S and T [lo] or correc- tions to the Zbb vertex [I], due to the difficulties inherent in performing reliable calculations in a strong interacting theory. An attempt in this direction was made recently by Ap- pelquist and Terning [12]. They constructed an ETC model and used it to produce a wide range of fermion masses. They also argued how the model could be com- patible with experimental constraints such as the value of S, FCNC's, and small neutrino masses. In this paper, we will begin by demonstrating the ex- istence of two potentially light U(l) Goldstone bosons in the Appelquist-Terning model. Appelquist and Tern- ing only specify gauge interactions below 1000 TeV and this is what we take to be the model. They also discuss the need for nonrenormalizable operators arising from physics beyond 1000 TeV. Those operators could give mass to the two Goldstone bosons by explicitly breaking their chiral symmetries. We shall discuss such a possi- bility assuming that these nonrenormalizable operators 0556-2821/95/5 1(7)/3969(5)/$06.00 - 51 3969 @ 1995 The American Physical Society

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Page 1: Goldstone bosons in the Appelquist-Terning extended technicolor model

PHYSICAL REVIEW D VOLUME 5 1, NUMBER 7 1 APRIL 1995

Goldstone bosons in the Appelquist-Terning extended technicolor model

Bhashyam Balaji Physics Department, Boston University, Boston, Massachusetts 02215

(Received 25 July 1994)

It is demonstrated that the extended technicolor model proposed recently by Appelquist and Terning has a pair of potentially light U(1) Goldstone bosons coupling to ordinary matter with strength 2mf/F,m where mf is the mass of the fermion and F, RZ 125 GeV. These Goldstone bosons could get a mass if the spontaneously broken U(l) symmetries are also explicitly broken, by physics beyond that specified in the model. An attempt to break these symmetries by embedding the model into a larger gauge group seems to be inadequate. The problem is because there are too many representations and there is a mismatch between the number of condensates and the number of gauge symmetries broken.

PACS number(s): 12.60.Nz, 11.15.Ex, 14.80.M~

I. INTRODUCTION

The reasons for considering the standard model of elec- troweak interactions to be incomplete are well known. In particular, the scalar Higgs sector possesses unsatisfac- tory features such as the naturalness (gauge hierarchy) problem [I], arbitrariness of Yukawa couplings and triv- iality [2]. These are particularly disturbing since elec- troweak symmetry breaking is responsible for endowing ordinary fermions and the weak gauge bosons with their masses.

One proposal for eliminating these problems assumes that there are no fundamental Higgs scalars. Instead, one postulates the existence of a new set of fermions, tech- nifermions, which interact via a new parity-conserving strong force called technicolor [3]. Crudely speaking, "standard" technicolor mimics QCD a t a higher energy scale. Walking technicolor [4] modifies relations obtained by naive scaling from QCD, due to large anomalous di- mensions of relevant composite operators. Technicolor enables us to solve part of the problem, gauge boson mass generation, based on nontrivial dynamics.

The dynamical generation of fermion masses requires vet another interaction: extended technicolor (ETC) [5,6]. It generates the current algebra masses of ordinary fermions by communicating the dynamical technifermion masses to the ordinary fermions. In other words, ETC gauge bosons couple ordinary fermions to technifermions, and couple to the various flavors differently.

Three of the Goldstone bosons produced bv the spon- taneous chiral symmetry breaking of techniflavor symme- trv contribute to W" and Z0 masses. "Realistic" models usually contain other (pseudo) Goldstone bosons, most of which acquire some mass from color or electroweak inter- actions [6].

An ETC model explaining the wide range of values of ordinary fermion masses and the Cabibbo-Kobayashi- Maskawa (CKM) matrix elements has been elusive. In particular, it is hard to construct models compatible with experiments. Strong constraints from flavor-changing neutral current (FCNC) experiments ruled out QCD-like

models long ago. Moreover, there are unwanted mass- less Goldstone bosons in any extended technicolor model with too many fermion representations [6].

Recently, severe constraints have also come from pre- cision electroweak measurements. Assuming the scale of new physics to be large compared to the W mass, it is found that there are important corrections to electroweak observables that are "obliquen-i.e., correction to gauge boson propagators [7 ] . These oblique corrections are en- coded in three parameters S, T , and U [a]. The pa- rameter T [9] is a measure of weak-isospin breaking- smallness of T means that technicolor models with large weak isospin breaking (needed to generate the b-t mass difference, for instance) are severely constrained. Calcu- lations of the S parameter in QCD-like technicolor mod- els with isospin symmetry indicates that technicolor mod- els with too many representations (the one-family tech- nicolor model, for instance) are incompatible with the experimental value of S. Of course, those models are al- ready ruled out on other considerations [6]. However, it is unclear if walking technicolor models are incompatible with the experimental values of S and T [lo] or correc- tions to the Zbb vertex [I] , due to the difficulties inherent in performing reliable calculations in a strong interacting theory.

An attempt in this direction was made recently by Ap- pelquist and Terning [12]. They constructed an ETC model and used it to produce a wide range of fermion masses. They also argued how the model could be com- patible with experimental constraints such as the value of S , FCNC's, and small neutrino masses.

In this paper, we will begin by demonstrating the ex- istence of two potentially light U ( l ) Goldstone bosons in the Appelquist-Terning model. Appelquist and Tern- ing only specify gauge interactions below 1000 TeV and this is what we take to be the model. They also discuss the need for nonrenormalizable operators arising from physics beyond 1000 TeV. Those operators could give mass to the two Goldstone bosons by explicitly breaking their chiral symmetries. We shall discuss such a possi- bility assuming that these nonrenormalizable operators

0556-2821/95/5 1(7)/3969(5)/$06.00 - 51 3969 @ 1995 The American Physical Society

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arise from a gauge theory. It will be shown that simple extensions, such as embedding into larger groups, will not solve the problem. Our analysis will naturally lead us to the main reason for the problem-a mismatch be- tween the number of broken diagonal gauge generators and the number of condensates. Note that the U(1)

% ,

Goldstone bosons discussed here are different from the Po discussed by Eichten and Lane [6]-those are avoided by implementing Pati-Salam unification and avoiding re- peated representations.

For brevity, the potentially light pseudo Goldstone bosons will be called axions. However, they have noth- ing to do with the conventional Peccei-Quinn axion since they couple to anomaly free currents. In Sec. 11, we briefly describe the model, paying attention to the sym- metry breaking pattern. In Sec. 111, we show the ex- istence of the unwanted massless Goldstone bosons and present an analysis of the general reasons for the prob- lem. We discuss the inadequacy of some "natural" ways of addressing the problem and present a solution. Finally, we present our conclusion.

11. THE APPELQUIST-TERNING MODEL

The gauge group is taken to be SU(5)ETC@ SU(2)HC@ SU(4)ps@ S U ( ~ ) L @ U ( ~ ) R with fermion content (all fermions taken to be left handed):

Here SU(2)Hc is an additional strong "hypercolor" (HC) gauge group which is needed to help break the SU(5)ETC down to SU(2)Tc. Hypercharge, Y (normalized by Q = T 3 ~ + Y/2), is given by Y = QR + TT, where T,P,S = diag (1/3,1/3,1/3, -1) is a generator of the SU(4)ps Pati- Salam group which implements quark-lepton unification. (For details regarding the motivation for the choice of the gauge group and fermion representation content see 1121.) L > r

At the Pati-Salam breaking scale (taken to be around 1000 TeV), a condensate is assumed to form in the chan- nel (5,1,4,1)-1 x (5,1,1, l ) o -+ (1,1,4, This chan- nel ((43$7) # 0) is not the most attractive channel (MAC) [13]. Instead, new physics is presumed to trig- ger its formation. This condensate breaks the U( l )R and SU(4)ps gauge groups leading to the gauge group SU(~)ETC@SU(~)HC@SU(~)C@ S U ( ~ ) L @ U(1) y below APS.

Next, it is assumed that at A5 = 1000 TeV a conden- sate forms in the channel (10,1,1, l)o x ( l o l l , 1, + (5, 1 ) - i.e., ($646) # 0. The singlet channel 10 X 10 -+ 1 is disfavored as SU(2)Hc is assumed to be relatively strong, so as to resist breaking. Then, the condensate (5,1,1, breaks the gauge symmetry to SU(~ )ETC@ S U ( ~ ) H C @ SU(3)c@ S U ( ~ ) L @ U(1) Y.

The next condensation is the attractive channel

(4, 21 1, l )o x (61 21 1, l )o + (4,1,1, 1) - ($s$s)i # 0 - which is taken to occur at A4 w 100 TeV. (The con- densate is subscripted to distinguish this channel from another at 113 arising from a different piece in $8.) The so-called "big MAC" criterion is applied here. When two or more relatively strong gauge interactions are a t play, the favored breaking channel is determined by the sum of the interactions. It is a generalization of the ordi- nary MAC criterion. Hence, below A4 the gauge group is SU(~ )ETC@ S U ( ~ ) H C @ SU(3)c@ SU(2) L@ u ( l ) ~ .

The final stage of ETC breaking takes place at the scale A3 a 10 TeV with the big MAC condensate (3,2,1, l ) o x (3,2,1,1)0 -+ (3,1,1, - ($8$a)2 # 0. This breaks S U ( ~ ) E T C to SU(2)Tc so that the gauge group below As is S U ( ~ ) T C @ ~ U ( ~ ) H C @ SU(3)c@ SU(2)I,@ U( l )y . Hy- percolored particles are confined at AHC = A3, and the HC sector decouples from ordinary fermions and tech- nifermions. We then have a one-family technicolor model (actually there is an additional "vector" quark [12]).

Finally, at the technicolor scale ATc, the SU(2)Tc be- comes strong resulting in condensation in the 2 x 2 -t 1 channel - ($1$2) # 0,($1$3) # 0, and ($1$6) # 0. This breaks the electroweak gauge group SU(2) L@ U(1) to U(1)em.

111. THE AXION ANALYSIS

For each fermion representation, there is a global U( l ) symmetry current. In general, these currents have gauge anomalies. From these currents, one can form anomaly- free combinations; these correspond to exact global sym- metries of the theory. One then follows this global sym- metry through the various gauge symmetry breakings and investigates whether or not it is spontaneously bro- ken at any scale. At each stage of symmetry breaking, one forms linear combinations of the gauged and global currents that leave the condensates invariant. These remaining symmetries generate unbroken global U(1)'s. The remaining orthogonal combinations couple to the massive gauge bosons [14].

To begin with, there are eight gauge singlet global U( l ) currents jf = where A = 1 , . . . , 8 correspond- ing to the eight representations. Each of them has an anomalous divergence due to the strong ETC, PS, and/or HC interactions:

Here Da = dpj$ and S, = (g2/32a2)~nfin, where n = 2,4,5 correspond to gauge groups SU(2)Hc, SU(4)ps, and S U ( 5 ) E ~ ~ , respectively. The electroweak s U ( 2 ) ~

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instanton has a negligible effect around Aps and weak anomalies are ignored.

From these currents, one can form five gauge anomaly free symmetry currents, which are

One of these currents, J:, is actually the U ( ~ ) R gauge current. So the global symmetry above Aps is U ( I ) ~ . [To include the s U ( 2 ) ~ we take three of the four lin- early independent current combinations not containing jb. The symmetry would be U( l )3 ; this will not change our conclusions. Note tha t the U ( l ) R anomaly is irrel- evant for our considerations due to the absence of in- stantons.] We follow this global symmetry through all of the gauge symmetry breakings; spontaneous breakdown of any global symmetry would result in a corresponding Goldstone boson a t that scale.

Below APS one can form four combinations from the above five currents which leave invariant the gauge sym- metry breaking condensate ( $ 3 4 7 ) # 0-the fifth one being the U ( ~ ) R gauge current [5]. So there still exists a U ( l ) 4 symmetry generated by (keeping the same symbol J for these currents)

One can proceed to find the four global symmetry cur- rents, which remain conserved below As t o be

Here J E E is the gauge current corresponding to the diag- onal generator in SU(5) which is not in SU(4). Note that J i is left unbroken although the gauge and global cur- rents are separately broken. This is analogous to the sit- uation in the standard model where S U ( ~ ) L @ SU(2)R + SU(2)v. The SU(5)E generator in the fundamental rep- resentation is chosen to be diag $(-4,1,1,1)-this au- tomatically fixes the U ( l ) charges in the other nonfun- damental representations. This is merely a convenient choice of a basis.

One can likewise obtain the global symmetry cur- rents below A4 and As. Finally, one investigates the U(1) global symmetries below the electroweak symme- try breaking scale. This entails three condensate's -

( $ 1 4 2 ) # 0, ( $ 1 4 3 ) # 0, and ( $ 1 $ 6 ) # 0. Only two of the four global symmetries are realized in the Wigner-Weyl mode, namely those corresponding to

The SU(2)3 generator in the fundamental representation is normalized as diag (1, -1). The SU(4) and SU(3) gen- erators in the fundamental representation are normalized as diag (-3,1,1,1) and diag (-2,1, I ) , respectively. Note that the jEm piece is irrelevant for our purposes since U(l),, is unbroken.

The other two broken global U ( l ) currents (up to un- broken pieces) are

One can incorporate the effect of the SU(2)L anomaly by constructing three linearly independent currents [from Eqs. (6) and (7)] not containing Jk . The unbroken cur- rent is

The remaining two (linearly independent) spontaneously broken global U ( l ) currents are

In terms of the first generation ordinary fermions, the two spontaneously broken global currents are

- - -dkyPd$ - ekyweff) + . . . .

There is no flavor mixing in this model; the CKM angles are assumed to arise from higher dimensional operators.

Our analysis has demonstrated that there are two po- tentially massless Goldstone bosons in the model. They couple with strength 2mf/F.rr where F, = 125 GeV to light fermions of current algebraic mass m f and are ex- perimentally ruled out [15].

Let us assume for the moment that these chiral symme- tries are explicitly broken by physics beyond 1000 TeV. I t is possible to obtain a rough estimate of the axion mass (ma) from four-fermion operators generated by heavy

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physics. Dashen's formula coupled with vacuum inser- tion approximation yields

where gsFs = As is the scale of new physics. Here ( T T ) ~ , = 4 x 10' GeV3 is a rough estimate of the technifermion condensates used by Appelquist and Tern- ing. Quoting values of the relevant anomalous dimensions from [12], we obtain

100 TeV 0'67 ( T T ) ~ , ( T T ) ~ , (rn)

1000 TeV 0'32 As TeV YS ( 100 TeV ) (1000 TeV) ( I2)

where y s is the anomalous dimension from 1000 TeV to As. Hence

lo3 T ~ V '-7s) m 32 ( ) GeV .

Here g s is taken to be N 1 and ys - a crude estimate of walking effects between As and Aps - is also expected to be of N 1.

In a pp collider, these neutral "axions" may be produced singly via gluon fusion (predominantly) or by quark-antiquark fusion [16]. Note that there is not enough phase space for it t o be produced in the pair technipion production mode (W* + A;P*), where P* is the charged pseudo Goldstone boson in the one-family technicolor model orthogonal to the absorbed Goldstone bosons, as the mass of the P* is expected to be in excess of 50 GeV [4]. These axions would decay into fermion-

~ -

antifermion pairs, principally the heavier ones (bb and 75. However, these decays are not of any experimental significance due to the smallness of mb,,/F,. Hence, a 32 GeV neutral, color-singlet "axion" is unlikely to be detected in the near future.

A natural approach for creating these four-fermion operators would be to embed the Appelquist-Terning gauge group into a larger gauge group. This will break some of the chiral symmetries so that the axions are no longer strictly massless. The simplest possible ex- tension (minimum ferrnion content and maximum chi- ral symmetry breaking) is to the gauge group SU(9) @

SU(2)Hc€3 SU(2)L@ U ( l ) R ; i.e., unification of the Pati- Salam and ETC gauge groups. The SU(9) is assumed to break into SU(5)ETC €3 SU(4)PS. The minimal repre- sentation content yielding us the eight representations in the Appelquist-Terning model, under decomposition, is

Since we want to avoid non-Abelian Goldstone bosons, no representations participating in any condensate should be repeated. The original fermions are contained in * I , . . . , q6. The representations Q7 and P8 are needed to cancel gauge anomalies.

However, this is not a resolution. While it explicitly breaks some chiral symmetries, the additional represen- tations create new chiral symmetries. The "axions" are still there.

Another approach for tackling this problem would be to gauge the two U(1)'s that are spontaneously broken a t the electroweak scale. [However, this would require a new set of spectator fermions so that the theory is anomaly free. One needs to assume that they are singlets under all but these two U ( l ) groups and get a mass from heavy physics.] Then, the two massless U(1) gauge bosons com- bine with the two massless Goldstone bosons to give the former their masses. The arbitrariness of the U ( l ) gauge coupling can push the gauge bqson masses beyond their current experimental limits. Z 0 mass (lower) bounds in- dicate that the U(1) gauge couplings would have to be rather large to be compatible with experiment.

Another possibility would be to arrange to have more than one condensate a t higher energy gauge symmetry breaking scales. As a result, the U*( l ) ' s are sponta- neously broken a t higher energies and hence are more weakly coupled to the light fermions (weak enough to be undetected). This way one ensures that there are no light Goldstone bosons a t the electroweak scale. How- ever, "f," would have to be between 10'' GeV and 10'' GeV from cosmological [17] and astrophysical considera- tions [18].

The above discussion can be stated in more general terms. A reason for the ~ r o b l e m is well known-too many representations [6]. If the number of irreducible representations (no) is less than or equal to the number of simple non-Abelian gauge group factors (ns) there will be no anomaly-free global U(1) currents to worry about.

If n o > n s , we have (nD - ns) anomaly-free global

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U ( l ) symmetries. We t h e n investigate t h e fate of these symmetr ies a s we pass th rough t h e various gauge sym- met ry breaking scales. Suppose t h e gauge symmetry breaking a t A involves c condensates a n d there a re d bro- - ken diagonal generators which a c t a s t h e number oper- a to r i n t h e subspace of t h e fermions i n t h e condensate. [For instance, when S U ( n ) breaks into S U ( n - I ) , t h e element of t h e C a r t a n subalgebra i n SU(n) b u t not i n - \ ,

S U ( n - 1 ) ac t s a s t h e number operator i n t h e 1 a n d n - 1 subspace separately.] Consider t h e general lin- ear combination of these ( n D - n s + d) U ( l ) currents [J = C A, JG, r = 1, . . . , (no - n s + d)] a n d tabu la te t h e charges Qi (z = 1,. . . , c) of t h e c condensates. (Wi thout loss i n generality, we a re assuming n o global symmetry breaking above this scale.) Note t h a t these Qi are linear combinations of (no - n s + d) variables A,.

T h e conditions t h a t t h e charges of t h e c condensates vanish c a n be s ta ted a s a set of c linear homogeneous equat ions i n ( n o - n s t d ) variables. If t h e rank of t h e co- efficient mat r ix (c') is less t h a n c, only c' condensates a re said t o have linearly independent charges. We focus o n t h e c' linearly independent condensates, i.e., those con- densates with linearly independent charges. Only when c' = d a re t h e initial u ( ~ ) ( ~ D - ~ G ) global symmetries pre- served: otherwise there a re c' - d exactly massless Gold- s tone bosons, which would b e unwelcome if they couple t o t h e ordinary fermions. Gauging these U(1)'s is a solution, b u t th i s entails t h e introduct ion of spectator fermions.

We know of n o simple way of determining c' other t h a n t o explicitly construct t h e global symmetry currents a t

each s tage of t h e gauge symmetry breaking. I n a n y case, t h e analysis needs t o b e carried ou t only when c > d; i.e., when t h e number of condensates is larger t h a n t h e num- ber of "diagonal" gauge generators spontaneously broken at t h a t scale. I n particular, there could b e many (unre- peated) ETC representations a s long as c 5 d.

IV. CONCLUSION

We have shown t h e existence of two potentially light Goldstone bosons i n t h e Appelquist-Terning ETC model. T h e problem is related t o t h e fact t h a t there a r e t o o many representations a n d t h e number of condensates exceeds t h e number of diagonal gauge symmetr ies broken. These axions could get a mass from physics a t higher energy scales. A n a t t e m p t t o break these symmetr ies wi th new gauge interactions seems t o b e inadequate.

ACKNOWLEDGMENTS

I t h a n k K. Lane for guiding t h e investigation a n d for a critical reading of t h e manuscript. I also t h a n k R. S. Chivukula a n d J. Terning for useful discussions a n d suggestions. T h i s work was supported i n p a r t by t h e Depar tment of Energy under Contract No. DE-FG02- 91ER40676 a n d by t h e Texas National Research Labora- tory Commission under Gran t No. RGFY93-278.

[I] K. G. Wilson, Phys. Rev. D 3, 181 (1971). [2] R. Dashen and H. Neuberger, Phys. Rev. Lett. 50, 1897

(1993). [3] S. Weinberg, Phys. Rev. D 19, 1277 (1979); L. Susskind,

ibid. 20, 2619 (1979). [4] B. Holdom, Phys. Rev. D 24, 1441 (1981); Phys. Lett.

150B, 301 (1985); T . Appelquist, D. Karabali, and L. C. R. Wijewardhana, Phys. Rev. Lett. 57, 957 (1986); T. Appelquist and L. C. R. Wijewardhana, Phys. Rev. D 36, 578 (1987); K. Yamawaki, M. Bando, and K. Ma- tumoto, Phys. Rev. Lett. 56, 1335 (1986); T . Akiba and T . Yanagida, Phys. Lett. 169B, 432 (1986).

[5] S. Dimopoulos and L. Susskind, Nucl. Phys. B155, 237 (1979).

[6] E. Eichten and K. Lane, Phys. Lett 90B, 125 (1980). [7] D. C. Kennedy and B. W. Lynn, Nucl. Phys. B322, 1

(1989). [8] M. Golden and L. Randall, Nucl. Phys. B361, 3 (1991);

B. Holdom and J . Terning, Phys. Lett. B 247, 88 (1990); M. Peskin and T . Takeuchi, Phys. Rev. Lett. 65, 964 (1990); A. Dobado, D. Espriu, and M. Herrero, Phys. Lett. B 253, 161 (1991); M. Peskin and T . Takeuchi, Phys. Rev. D 46, 381 (1992); R. S. Chivukula, M. Dugan, and M. Golden, Phys. Lett. B 292, 435 (1992).

[9] M. Einhorn, D. Jones, and M. Veltman, Nucl. Phys. B191, 146 (1981); A. Cohen, H. Georgi, and B. Grin- stein, ibzd. B232, 61 (1984).

[ lo] R. Sundrum and Stephen D. H. Hsu, Nucl. Phys. B391, 127 (1993); Markus A. Luty and R. Sundrum, Phys. Rev. Lett. 70, 529 (1993); T . Appelquist and J . Terning, Phys.

Lett. B 315, 139 (1993). [ll] R. S. Chivukula, S. B. Selipsky, and E. H. Simmons,

Phys. Rev. Lett. 69, 575 (1992); R. S. Chivukula, E. Gates, E. H. Simmons, and J . Terning, Phys. Lett. B 311, 157 (1993).

[12] T . Appelquist and J . Terning, Phy. Rev. D 50, 2116 (1994).

[13] S. Dimopoulos, S. Raby, and L. Susskind, Nucl. Phys. Bl69, 373 (1980).

[14] K. Lane, in Unz$ed Field Theories and Beyond, Proceed- ings of the Fifth Johns Hopkins Workshop on Current Problems in Particle Theory, Baltimore, Maryland, 1981 (DOE, Washington, D. C., 1982).

[15] T . W. Donnelly et al., Phys. Rev. D 18, 1607 (1978); S. Barshay et al., Phys. Rev. Lett. 46, 1361 (1981); A. Bar- roso et al., Phys. Lett. 106B, 91 (1981); R . D. Peccei, in Proceedings of the International Conference on Neutrino Physics and Astrophysics, Wailea, Hawaii, edited by R. J . Lence, E. Ma, and A. Roberts (University of Hawaii, Honolulu, 1981), Vol. 1, p. 148.

[16] E. Eichten, I. Hinchliffe, K. Lane, and C. Quigg, Rev. Mod. Phys. 56, 579 (1984).

[17] J . Preskill et al., Phys. Lett. 120B, 127 (1983); L. F. Abbott and P. Sikivie, ibid. 120B, 133 (1983); M. Dine and W. Fischler, ibid. 120B, 137 (1983).

[18] D. A. Dicus et al., Phys. Rev. D 18, 1829 (1978); M. Fukugita, S. Watamura, and M. Yoshimura, Phys. Rev. Lett. 48, 1522 (1982), also Phys. Rev D 26, 1840 (1982); D. S. P. Dearborn et al., Phys. Rev. Lett. 56, 26 (1986); G. G. Raffelt, Phys. Rev. D 33, 897 (1986).