6
Neutron electric dipole moment and CP-violating couplings in the supersymmetric standard model without R parity Darwin Chang, 1 We-Fu Chang, 1 Mariana Frank, 2 and Wai-Yee Keung 3 1 NCTS and Physics Department, National Tsing-Hua University, Hsinchu 30043, Taiwan, R.O.C. 2 Concordia University, Montreal, Quebec, Canada H3G 1M8 3 Physics Department, University of Illinois at Chicago, Illinois 60607-7059 ~Received 18 April 2000; published 29 September 2000! We analyze the neutron electric dipole moment ~EDM! in the minimal supersymmetric standard model with explicit R-parity violating terms. The leading contribution to the EDM occurs at the two-loop level and is dominated by the chromoelectric dipole moments of quarks, assuming there is no tree-level mixings between sleptons and Higgs bosons or between leptons and gauginos. Based on the experimental constraint on the neutron EDM, we set limits on the imaginary parts of complex couplings l ijk 8 and l ijk due to the virtual b loop or t loop. PACS number~s!: 14.80.Ly, 11.30.Er, 13.10.1q The minimal supersymmetric standard model ~MSSM!@1# has been widely considered as a leading candidate for new physics beyond standard model. However, unlike the stan- dard model, supersymmetry allows renormalizable interac- tions which break R parity defined as ( 21) 3 B1L 1F and vio- late the lepton and/or the baryon numbers. It is in fact one of the main theoretical weaknesses of these models because R-parity conservation is an ad hoc imposition which may or may not have a fundamental theoretical basis. Therefore, in- stead of neglecting them completely, it is interesting to ask how small these R-parity breaking ( R ) couplings could be by investigating directly phenomenological constraints @2#. The most general renormalizable R-violating superpoten- tial using only the MSSM superfields is W R 5l ijk L i L j E k c 1l ijk 8 L i Q j D k c 1l ijk 9 U i c D j c D k c 1m j L j H 2 . ~1! Here, i,j,k are generation indices. The couplings l ij k and l ij k 9 must be antisymmetric in flavor, l ijk 52l jik and l ijk 9 52l ikj 9 . There are 36 lepton number nonconserving cou- plings ~9 of the l type and 27 of the l 8 type! and 9 baryon number non-conserving couplings ~all of the l 9 type! in Eq. ~1!. To avoid rapid proton decay, it is usually assumed in the literature that l,l 8 type couplings do not coexist with l 9 type couplings. This can be achieved easily by imposing baryon number symmetry. The bilinear terms m j L j H 2 con- tribute to lepton flavor and number violation and could be responsible for neutrino masses. Phenomenologically, many of these couplings have been severely constrained using low- energy processes or using high energy data at the colliders @3–10#. In this paper, we shall not consider l ijk 9 and m j cou- plings. However, most of the bounds in the literature constrain the real part of the trilinear couplings, or the product of tri- linear couplings. The exception is the bound coming from the e K which constrains Im(l i12 8 l i 21 8 * ) ,8 310 212 @11#. We propose to study the neutron electric dipole moment, which is tightly bound by experiment, and thus obtain limits on the imaginary parts of different products of trilinear couplings from the ones imposed by e K . The electric dipole moment of an elementary fermion is defined through its electromagnetic form factor F 3 ( q 2 ) in the ~current! matrix element ^ f ~ p 8 ! u J u ~ 0 ! u f ~ p ! & 5u ¯ ~ p 8 ! G m ~ q ! u ~ p ! , ~2! where q 5 p 8 2 p and G m ~ q ! 5F 1 ~ q 2 ! g m 1 F 2 ~ q 2 ! 2 m i s mn q n 1F A ~ q 2 ! 3~ g m g 5 q 2 22 m g 5 q m ! 1 F 3 ~ q 2 ! 2 m s mn g 5 q n , ~3! with m the mass of the fermion and F 1 (0) 5e f . The electric dipole moment ~EDM! of the fermion field f is then given by d f 5 eF 3 ~ 0 ! 2 m , ~4! corresponding to the effective dipole interaction L EDM 52 i 2 d f f ¯ s mn g 5 fF mn . ~5! In the static limit this corresponds to an effective Lagrangian L EDM d f C A 1 s W E W C A , where C A is the large component of the Dirac field. Similarly the quark chromoelectric dipole moment ~CEDM! is the coefficient d q g in the effective opera- tor: L CEDM 52 i 2 d q g q ¯ s mn g 5 l a 2 qG a mn . ~6! The relevant Lagrangian for generating an EDM is L52 S 1 2 ( ij C i ] 2 W ] f i ] f j C j 1H.c. D 1¯ 5@ l ijk 8 ~ 2 l ˜ i u j d k c 1n ˜ i d j d k c ! 1H.c. # 1¯ . ~7! PHYSICAL REVIEW D, VOLUME 62, 095002 0556-2821/2000/62~9!/095002~6!/$15.00 ©2000 The American Physical Society 62 095002-1

Neutron electric dipole moment and CP -violating couplings in the supersymmetric standard model without R parity

  • Upload
    wai-yee

  • View
    213

  • Download
    0

Embed Size (px)

Citation preview

PHYSICAL REVIEW D, VOLUME 62, 095002

Neutron electric dipole moment andCP-violating couplings in the supersymmetricstandard model without R parity

Darwin Chang,1 We-Fu Chang,1 Mariana Frank,2 and Wai-Yee Keung31NCTS and Physics Department, National Tsing-Hua University, Hsinchu 30043, Taiwan, R.O.C.

2Concordia University, Montreal, Quebec, Canada H3G 1M83Physics Department, University of Illinois at Chicago, Illinois 60607-7059

~Received 18 April 2000; published 29 September 2000!

We analyze the neutron electric dipole moment~EDM! in the minimal supersymmetric standard model withexplicit R-parity violating terms. The leading contribution to the EDM occurs at the two-loop level and isdominated by the chromoelectric dipole moments of quarks, assuming there is no tree-level mixings betweensleptons and Higgs bosons or between leptons and gauginos. Based on the experimental constraint on theneutron EDM, we set limits on the imaginary parts of complex couplingsl i jk8 andl i jk due to the virtualb loopor t loop.

PACS number~s!: 14.80.Ly, 11.30.Er, 13.10.1q

netaa

oau

, is

ou

th

in

bealode

airi-m

iche

s

is

ianfle

The minimal supersymmetric standard model~MSSM! @1#has been widely considered as a leading candidate forphysics beyond standard model. However, unlike the sdard model, supersymmetry allows renormalizable intertions which breakR parity defined as (21)3B1L1F and vio-late the lepton and/or the baryon numbers. It is in fact onethe main theoretical weaknesses of these models becR-parity conservation is anad hocimposition which may ormay not have a fundamental theoretical basis. Thereforestead of neglecting them completely, it is interesting to ahow small theseR-parity breaking (R” ) couplings could be byinvestigating directly phenomenological constraints@2#.

The most general renormalizableR-violating superpoten-tial using only the MSSM superfields is

WR”5l i jkLiL jEkc1l i jk8 LiQjDk

c1l i jk9 UicD j

cDkc1m jL jH2 .

~1!

Here, i,j,k are generation indices. The couplingsl i jk andl i j

k9must be antisymmetric in flavor,l i jk52l j ik and l i jk952l ik j9 . There are 36 lepton number nonconserving cplings ~9 of thel type and 27 of thel8 type! and 9 baryonnumber non-conserving couplings~all of the l9 type! in Eq.~1!. To avoid rapid proton decay, it is usually assumed inliterature thatl,l8 type couplings do not coexist withl9type couplings. This can be achieved easily by imposbaryon number symmetry. The bilinear termsm jL jH2 con-tribute to lepton flavor and number violation and couldresponsible for neutrino masses. Phenomenologically, mof these couplings have been severely constrained usingenergy processes or using high energy data at the colli@3–10#. In this paper, we shall not considerl i jk9 andm j cou-plings.

However, most of the bounds in the literature constrthe real part of the trilinear couplings, or the product of tlinear couplings. The exception is the bound coming frothe eK which constrains Im(li128 l i218* ),8310212 @11#. Wepropose to study the neutron electric dipole moment, whis tightly bound by experiment, and thus obtain limits on t

0556-2821/2000/62~9!/095002~6!/$15.00 62 0950

wn-c-

fse

n-k

-

e

g

nyw-rs

n

h

imaginary parts of different products of trilinear couplingfrom the ones imposed byeK .

The electric dipole moment of an elementary fermiondefined through its electromagnetic form factorF3(q2) in the~current! matrix element

^ f ~p8!uJu~0!u f ~p!&5u~p8!Gm~q!u~p!, ~2!

whereq5p82p and

Gm~q!5F1~q2!gm1F2~q2!

2mismnqn1FA~q2!

3~gmg5q222mg5qm!1F3~q2!

2msmng5qn, ~3!

with m the mass of the fermion andF1(0)5ef . The electricdipole moment~EDM! of the fermion fieldf is then given by

df5eF3~0!

2m, ~4!

corresponding to the effective dipole interaction

LEDM52i

2df f smng5f Fmn. ~5!

In the static limit this corresponds to an effective LagrangLEDM→dfCA

1sW •EW CA , whereCA is the large component othe Dirac field. Similarly the quark chromoelectric dipomoment~CEDM! is the coefficientdq

g in the effective opera-tor:

LCEDM52i

2dq

gqsmng5

la

2qGamn. ~6!

The relevant Lagrangian for generating an EDM is

L52S 1

2 (i j

C i

]2W

]f i]f jC j1H.c.D 1¯

5@l i jk8 ~2 l iujdkc1 n idjdk

c!1H.c.#1¯ . ~7!

©2000 The American Physical Society02-1

-

itsmee

tlydlee

ers.

re

e

tc

n-

cggism

iggghrigf

u-a

m

i-m

peb

e

rindina

on

hesgs

inggive

rm

ebi-n

.

ae-

a-ic

hed

CHANG, CHANG, FRANK, AND KEUNG PHYSICAL REVIEW D62 095002

It has been shown@4# that there is no one-loop contribution to EDMs based onl, l8, or l9 couplings based onhelicity properties and symmetry. Here we briefly revieworigin. It is easy to show that one cannot induce EDMs frothe diagram that requires the external mass insertion duthe equation of motion. As a result of this lemma, prophelicities for external fermion lines have to come direcfrom vertices. Let us look at the electron EDM, which neeexternalL andEc. For the correct quantum number, possibone loop contributions have to be proportional to eith(1)ll* or (2)l8l8* . Based on the above lemma, the extnal L and Ec are required to come directly from verticeCase~1! cannot produce the helicity flip. Case~2! is evenworse, there is no vertex to giveEc. So the one-loop electronEDM is absent. For thed quark EDM, possibilities are eithe~1! l8l8* or ~2! l9l9* . Case~1! does not work becausboth dL anddc have to come from aCP-even product of acomplex conjugated pair of vertices, and case~2! fails badlybecause there is no vertex to give an externaldL . Similarreason follows for theu quark EDM. As a reminder, therare one-loop EDM amplitudes@12# related to the bilinearterm m jL jH2 , which mixes sleptons and Higgs bosons, eWe do not consider these couplingsm i in this work.

At the two-loop level, a number of different types of cofigurations contribute, which we classify as rainbowlike~I!,overlapping~II !, tentlike ~III !, and Barr-Zee~IV ! @13# types.The rainbowlike graphs~I! are those with two concentriboson loops, the outer of which must be a charged Hiloop ~for the same reason that one-loop graphs do not ex!.The inner loop may have a left or right sfermion. The coplete set of this type of graphs is given in Fig. 1~a!. Thecomplete set of overlapping type of graphs is given in F1~b!. In this case, one of them must be a charged Hiboson, the other a left or right sfermion. The tentlike grap~III ! have a trilinear bosonic vertex. Again, the three diffeent boson legs can be two sfermions and one charged Hboson~in all possible configurations!. The complete set othis type of graphs is given in Fig. 1~c!. Careful consider-ation of all the type I–III graphs shows that their contribtions are suppressed by both one power of light quark mplus some Cabibbo-Kobayashi-Maskawa~CKM! mixingangles factor compared to those of type IV~Fig. 2!. There-fore, one expects the Barr-Zee type of contributions to donate and we shall study them in detail next.

In Ref. @4#, only a rough estimate of the two-loop contrbutions to EDMs is provided. We shall present here a coplete calculation of the quark~or electron! EDM and thequark CEDM at the two-loop level due to the Barr-Zee tymechanism and show that the neutron EDM is dominatedthe CEDM of thed quark. This calculation leads to morstringent bounds than previously obtained.

There is another class of Barr-Zee graphs with sneutline replaced by the charged slepton line and corresponmodifications of the fermions charges in the loop. The cculations of these type of graphs are very similar to thein the charged Higgs models ofCP violation as in Refs.@14#,@15#. Comparing the charged Higgs contributions to tEDM in Refs.@14#, @15# with the neutral Higgs contributiongiven in Ref. @13#, one can observe that the neutral Hig

09500

tor

s

r-

.

st-

.ss-gs

ss

i-

-

y

og

l-e

contributions generally dominate given comparable couplconstants and boson masses. Therefore, we shall onlydetails of sneutrino contributions here.

ngg vertex of the inner loop. The two-loop diagram of theCEDM of thed-type quark can appear with the couplingl i jk8through the virtual vertexngg. The amplitude of the innerloop in terms of the leading gauge invariant terms is

Gmn5S~q2!@knqm2k•qgmn#1P~q2!@ i emnabpaqb#,~8!

whereS and P correspond to scalar and pseudoscalar fofactors, respectively:

S~q2!5mbgs

2l i338*

16p2 E0

1

dy122y~12y!

mb22y~12y!q2 ,

P~q2!5mbgs

2l i338*

16p2 E0

1

dy1

mb22y~12y!q2 .

Second loop. Combining the two twisted diagrams and thtwo choices of sneutrino flow directions, we have a comnatoric factor of 4 in the the two loop CEDM amplitude. Ithe convention of Eqs.~2!–~6!, we obtain the CEDM of thed quark at the scale ofmb ,

S ddg

gsD

mb

5mbgs

2umb

128p4 Im~l i338* l i118 !

3E0

1

dyE0

` Q2d~Q2!@12y~12y!#

@mb21y~12y!Q2#~Q21M n i

2 !Q2

5as Im~l i338* l i118 !

32p3

mb

M n i2 •FS mb

2

M n i

2 D , ~9!

with the loop function

F~t!5E0

1

dy~y22y11!

y~12y!2tlnS y~12y!

t D ~10!

→ p2

3121 ln t1~ ln t!2 for t→0. ~11!

Implicit sum over sneutrino flavorsi is assumed in the aboveThe last asymptotic form is useful because the ratiot5mb

2/M n i

2 is small. The large logarithmic factor helps placestrong constraint onl8 couplings. Note that sneutrino is thheaviest particle in the loop. Atmb scale, the sneutrino induces a four fermion interaction ofb and d quarks. As aresult, by simple power counting, the gluonic loop is logrithmically divergent which explains the large logarithmenhancement factor.

Replacing the gluon line by the photon line, we obtain tEDM of the quark simply by substituting the color factor anthe charge factor:

2-2

NEUTRON ELECTRIC DIPOLE MOMENT ANDCP- . . . PHYSICAL REVIEW D 62 095002

FIG. 1. ~a! ~i! Rainbowlike diagram for thed quark. The genericR” vertex is marked bys and its complex conjugate byd. ~ii !Rainbowlike diagram for theu quark.~b! ~i! Overlapping diagram for thed quark usingl8. ~ii ! Overlapping diagram for theu quark usingl8. ~c! ~i! Tentlike diagram for thed quark usingl8. ~ii ! Tentlike diagram for theu quark usingl8. ~d! Barr-Zee type graph foru quarkEDM.

095002-3

’sewM

diothr-t

he

-io

c-ent

to

u-

CDomrere

t

s,

aint

the

te

CHANG, CHANG, FRANK, AND KEUNG PHYSICAL REVIEW D62 095002

S ddg

e Dmb

56edeb2S aem

asD

mb

S ddg

gsD

mb

. ~12!

Now we address the QCD evolution of these Wilsoncoefficients. As an effective theory, the four-fermion verticof the form (bb)(dd) arise first in the energy scale beloM n i

when n are integrated out of the theory. Then the ED

and the CEDM of thed quark arise belowmb scale. There-fore, thel8 couplings in the above equations are evaluatethe mb scale. We ignore the dressing of these four-fermvertices because of the small value of their couplings andslow running ofas at such high energy scale. In this pespective, thel8 factors in Eq.~9! are defined at the shordistance scale nearM n . Below mb , the CEDM and theEDM of light quarks appear and they evolve down to thadronic scaleLH by

S ddg

gsD

LH

Y S ddg

gsD

mb

5S gs~mb!

gs~mc!D 4/25S gs~mc!

gs~LH! D4/27

5Zg,

~13!

S ddg

e DLH

Y S ddg

e Dmb

5S gs~mb!

gs~mc!D 8/25S gs~mc!

gs~LH! D8/27

5Zg.

~14!

Note that in some references@17#, a light quark mass coefficient has been factored out so that the form of evolutequation looks different from above. We denote byDn

g (Dng)

the neutron EDM due to the CEDM~EDM! of light quarks.The SU~6! relation gives

Dng

e5F4

9 S ddg

gsD

LH

12

9 S dug

gsD

LH

G ,

~15!

Dng

e5F4

3 S ddg

e DLH

21

3 S dug

e DLH

G .

FIG. 2. A typical two-loop diagram of the Barr-Zee type. Nothat there are three ways to insert mass.

09500

s

atne

n

For as(MZ)50.12 andgs(LH)/(4p)51/A6, the QCD evo-lution factorsZg and Zg are about 0.71 and 0.84, respetively. Our formulas and numerical values are consistwith those in Ref.@17# but differ from those in Ref.@18#.

For completeness, we add another large contributionthe d quark EDM due to thet lepton replacing theb quarkinside the first loop. We obtain two independent contribtions as:

S ddg

e Dmb

~b-loop!52aem

16p3 (i 51,2,3

3edeb2mb

M n i

2

3Im~l i338* l i118 !•FS mb2

M n i

2 D , ~16!

S ddg

e Dmt

~t loop!52aem

16p3 (iÞ3

edmt

M n i

2

3Im~l i33* l i118 !•FS mt2

M n i

2 D . ~17!

The latter contribution from thet-loop is induced at themtscale and we need to adjust the minor change in the Qevolution. There are also other Barr-Zee type diagrams frthe exchange ofW6 or Z gauge bosons. However, they aknown to be giving smaller contributions and thus we ignothem in our numerical study@14–16#.

As uR is not directly involved in theR” interaction, theuquark CEDM does not appear throughl8 in the form of Fig.2. Nonetheless, there are two-loop diagrams Figs. 1~a! ~ii !,1~b! ~ii !, 1~c! ~ii !, and 1~d! which are suppressed by the lighquark mass and mixing angles. Therefore, theR” contributionto the neutron EDM is dominated by thed quark CEDM andEDM. Assuming allM n i

are equal and taking typical value

M n i'300 GeV andmb'4.5 GeV, we have

Dng.5.46310221~e cm!3(

iIm~l i338* l i118 !, ~18!

Dng.21.03310222~e cm!3(

iIm~l i338* l i118 !

21.92310222~e cm!3(iÞ3

Im~l i33* l i118 !.

~19!

Our numerical result shows that the strongest constrcomes from the CEDM of thed quark. Using the up-to-datedexperimental@19# bounduDnu,6.3310226e cm and barringaccidental cancellation among contributions, we deriveconstraints

(i

Im~l i338* l i118 !,1.231025, ~20!

2-4

NEUTRON ELECTRIC DIPOLE MOMENT ANDCP- . . . PHYSICAL REVIEW D 62 095002

FIG. 3. The neutron EDMDn versusM n with( i Im(li338* l i118 ) or ( i Im(li33* l i118 ) scaled to 1025.

ns

nhoo

,p

-

ns,

(iÞ3

Im~l i33* l i118 !,3331025, ~21!

for M n5300 GeV.In Fig. 3 we plot both the photon and gluon contributio

to the neutron EDM versus the sneutrino massM n in theregion of interest~100 to 600 GeV! with ( i Im(li338* l i118 ) or( i Im(li33* l i118 ) scaled to 1025. One could see that the gluocontribution consistently dominates the corresponding pton one by at least an order of magnitude over the whparameter space explored.

The electron EDM can arise via bothl8 or l-typeR-parity violating coupling Ref.@4#. Based on above studythe analytical formula for the electron EDM at the two-loolevel is

09500

-le

S deg

e D 52aem

16p3 F(iÞ1

3eb2mb

M n i

2 Im~l i338* l i11!•FS mb2

M n i

2 D1

mt

M n2

2 Im~l233* l211!•FS mt2

M n2

2 D G . ~22!

In Fig. 4 we assume allM n ito be equal and plot contribu

tions to the electron EDM versus the sneutrino massM n inthe region of interest~100 to 600 GeV!. Using the up-to-dated experimental@20# bound udeu,0.43310226e cm andbarring from accidental cancellation among contributiowe derive constraints

Im~l233* l211!,0.7431025, ~23!

FIG. 4. The electron EDMde versusM n .

2-5

leM

linreon

euct

ce

ofs

CHANG, CHANG, FRANK, AND KEUNG PHYSICAL REVIEW D62 095002

(iÞ1

Im~l i338* l i11!,1.331025, ~24!

for M n5300 GeV.In conclusion, we have presented an exact and comp

calculation of the dominant contribution to the neutron EDin a minimal supersymmetric model withoutR parity due tothe couplingsl and l8. The CP violation does not dependon the complex phasesfm and fA0

~the phases of theHiggsino mass parameter and the trilinear scalar coupA0) in minimal supergravity models, and therefore is unlated to the restrictive bounds or complicated cancellati

kin

.

.

ya

y

v

09500

te

g-s

necessary in MSSM. The leadingR” contribution to the neu-tron EDM occurs at two-loop level through the Barr-Zemechanism. We obtain stringent bounds on the prodIm li338* l i118 ,O(1025).

This work was supported in part by National ScienCouncil of R.O.C., by U.S. Department of Energy~GrantNo. DE-FG02-84ER40173! and by NSERC of Canada~Grant No. SAP0105354!. M.F. and W.F.C. would like tothank the High Energy Physics Group at the UniversityIllinois at Chicago for their hospitality while this work wainitiated.

. B

,

s.

ev.

,

D

@1# H. P. Nilles, Phys. Rep.110, 1 ~1984!; H. E. Haber and G. L.Kane, ibid. 117, 75 ~1985!; R. N. Mohapatra,Unification andSupersymmetry~Springer-Verlag, Berlin, 1991!; S. Dawson,hep-ph/9612229; M. Drees, hep-ph/9611409; M. Peshep-ph/9705479.

@2# J. Ellis et al., Phys. Lett.150B, 142 ~1985!; G. G. Ross and JW. F. Valle, ibid. 151B, 375 ~1985!; S. Dawson, Nucl. PhysB261, 297 ~1985!; S. Dimopoulos and L. Hall, Phys. Lett. B207, 210 ~1987!.

@3# H. Dreiner, hep-ph/9707435, 1997; G. Bhattacharrhep-ph/9709395, 1997; B. Allanachet al., hep-ph/9906224,1999.

@4# R. M. Godbole, S. Pakvasa, S. D. Rindani, and X. Tata, PhRev. D 61, 113003~2000!; S. A. Abel, A. Dedes, and H. K.Dreiner, J. High Energy Phys.05, 013 ~2000!.

@5# L. Hall and M. Suzuki, Nucl. Phys.B231, 419 ~1984!; R. N.Mohapatra, Phys. Rev. D34, 909 ~1986!; V. Barger, G. F.Guidice, and T. Han,ibid. 40, 2987 ~1989!; R. Godbole, P.Roy, and X. Tata, Nucl. Phys.B401, 67 ~1993!; M. Hirsch, H.V. Klapdor-Kleingrothaus, and S. G. Kovalenko, Phys. ReLett. 75, 17 ~1995!; K. S. Babu and R. N. Mohapatra,ibid. 75,2276 ~1995!.

@6# B. Brahmachari and P. Roy, Phys. Rev. D50, R39 ~1994!.@7# J. L. Goity and M. Sher, Phys. Lett. B346, 69 ~1995!; D.

Chang and W.-Y. Keung,ibid. 389, 294 ~1996!.@8# F. Zwirner, Phys. Lett.132B, 103 ~1983!.@9# R. Barbieri and A. Masiero, Nucl. Phys.B267, 679 ~1986!.

,

,

s.

.

@10# G. Bhattacharyya, D. Choudhury, and K. Sridhar, Phys. Lett355, 193 ~1995!.

@11# R. Barbieri, A. Strumia, and Z. Berezhiani, Phys. Lett. B407,250 ~1997!.

@12# K. Choi, E. J. Chun, and K. Hwang, Phys. Rev. D~to bepublished!, hep-ph/0004101; Y. Y. Keum and O. C. W. Konghep-ph/0004110.

@13# S. M. Barr and A. Zee, Phys. Rev. Lett.65, 21 ~1990!; D.Chang, W.-Y. Keung, and T. C. Yuan, Phys. Rev. D43, 14~1991!; R. G. Leigh, S. Paban, and R. M. Xu, Nucl. PhyB352, 45 ~1991!; C. Kao and R.-M. Xu, Phys. Lett. B296, 435~1992!.

@14# D. Bowser-Chao, D. Chang, and W.-Y. Keung, Phys. RLett. 79, 1988~1997!.

@15# D. Chang, W.-F. Chang, and W.-Y. Keung, Phys. Lett. B478,239 ~2000!.

@16# A. Pilaftsis, Phys. Lett. B471, 174 ~1999!.@17# D. Chang, W.-Y. Keung, and T. C. Yuan, Phys. Lett. B251,

608~1990!; D. Chang, W.-Y. Keung, C. S. Li, and T. C. Yuanibid. 241, 589 ~1990!; J. F. Gunion and D. Wyler,ibid. 248,170 ~1990!.

@18# R. Arnowitt, J. L. Lopez, and D. V. Nanopoulos, Phys. Rev.42, 2423~1990!.

@19# P. G. Harriset al., Phys. Rev. Lett.82, 904 ~1999!.@20# K. Abdullah et al., Phys. Rev. Lett.65, 2347~1990!; E. Com-

mins et al., Phys. Rev. A50, 2960 ~1994!; B. E. Sauer, J.Wang, and E. A. Hinds, Phys. Rev. Lett.74, 1554 ~1995!; J.Chem. Phys.105, 7412~1996!.

2-6