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(1)

Nonommutative Supersymmetri Field Theories

Vitor O.Rivelles

Instituto deFsia,UniversidadedeS~aoPaulo

CaixaPostal66318, 05315-970,S~aoPaulo-SP, Brazil

E-mail: rivellesfma.if.usp.br

Reeivedon19February,2001

Wedisusssomepropertiesofnonommutativesupersymmetrieldtheorieswhihdonotinvolve

gaugeelds. Weonentrateontherenormalizabilityissueofthesetheories.

I Introdution

Although stringtheory isquitewellunderstoodin the

perturbativeregimeitsformulationinabakground

in-dependent way is almost unknown. There are many

reasons for that. String theory has toomany degrees

of freedom. It is quite diÆult to handle all of them

together. It alsoinludes thegravitationaleld whih

may havequantum utuations. And there are many

souresfornonloalitywhihisalsotroublesomeinany

theory. Oneway outof thesediÆulties is toonsider

limitsofstringtheorywhihhavesomeofthetroubles

raisedabovebutnotallofthem. Thismayallowusto

understand bettersomeaspetsof stringtheory

with-outtheompliationsofthefull theory.

Onesuh alimitis the zeroslopelimitof the

D3-braneinthepreseneofaonstantNS-NSeld[1℄. The

lowenergyeetivetheoryisaquantumeldtheory

de-formed intermsoftheMoyalprodutoverspae-time.

In nonommutativeeld theoriestheusual produtof

elds isreplaed bytheMoyalprodutof eldsgiving

risetononloaleldtheories[2℄. Usuallynonloaleld

theoriesturn outto benotwelldened butthe

nonlo-alityinduedbytheMoyalprodutisstilltratable. It

wasfoundthatthemainharateristiof

nonommuta-tiveeldtheoriesisthemixingofultraviolet(UV)and

infrared (IR)divergenes due toits nonloalstruture

[3℄. As aonsequene it is notlear that the

proper-ties of the usual ommutative eld theories are kept,

without modiations,in theirnonommutative

oun-terparts. Thisgaverisetoanintensiveresearhof

non-ommutative eld theories in Eulidean orMinkowski

spae-time.

Oneof themanifestationsof theUV/IR mixing in

the 4

theoryisasaninfraredquadratisingularityin

the propagator at one loop [3℄. Although

renormaliz-ableupto twoloops[4℄itbeomesnon-renormalizable

at higher loop orders. Models involving a omplex

salareldmaybenon-renormalizableevenatoneloop

harateristi of ommutativeeld theories, i.e., their

renormalizability.

Inwhat followswewill disuss theinlusion of

su-persymmetry in suh models and how it restores the

renormalizability. We will onentrate on the

Wess-Zumino model in 3+1dimensions [6℄ and the

super-symmetrinon-linearsigmamodelin2+1dimensions

[7℄. Inthislast asewewillseethat the

nonommuta-tivityalsodestroysthemehanismfordynamialmass

generation of the fermioni setor, and we will show

howsupersymmetryhelpstox it.

II Nonommutative Spaes

Inquantummehaniswehavetheusualommutation

relations

^ q i

;p^ j

= i~g ij

; (1)

^ q i

;q^ j

=

^ p i

;p^ j

=0: (2)

It is natural to onsider nonommutative oordinates

withommutationrelations

^ q i

;q^ j

=i ij

; (3)

where

ij

is aonstantof dimensionL 2

whih denes

anonommutativity sale. This breaks rotational (or

Lorentz)symmetrybutinthelimit!0thesymmetry

isreovered. This isanexampleof anonommutative

spae. It an be extended to spae-time but we will

onsider nonommutativity only in thespatial

oordi-natessineotherwisethereareproblemswithunitarity

[8℄.

We an understand heuristially how the UV and

IR physis gets mixed. From Eq.(1) it follows that

^q i

p^ j

ig ij

. In a similar way, from Eq.(3) it

fol-lowsthatq^ i

^q j

i ij

so weexpet thatq^^p.

Thismeansthathighenergymodeshavedrastieets

(2)

itselfalreadyatonelooplevelinthepropagatorofthe

elds.

Fields dened on suh spaes are operator valued

objets. It turns out to be more onvenient to use

elds whih are not operator valued objets but just

funtions. Thisanbeahievedthroughtheuseofthe

Weyl-Moyalorrespondene[2℄

^

(^q)!(x): (4)

We assoiate to the operator valued eld ^

(^q) a

las-sial funtion (x)through itsFouriertransform ~

(p)

as

^

(^q)= Z

dpe ipq^

~

(p): (5)

Theoperatorvaluedeld ^

satises

^

1 (^q)

^

2 (^q)=

Z

dp

1 dp

2 e

i(p

1 +p

2 )^q

1

2 p

1 p

2

1 (p

1 )

2 (p

2

); (6)

hene

^

1 (^q)

^

2

(^q)$(

1 ?

2

)(x); (7)

where

(

1 ?

2 )(x)

h

e i

1

2

x

y

1 (x)

2 (y)

i

y=x

; (8)

is the Moyal(or star) produt. Then we an work on aommutative spae in whih the usual produt of eld

is replaed by the Moyalprodut. Notie that thederivatives in the denition Eq.(8) makes theMoyalprodut

non-loal. Also,theMoyalommutatoroftheommutativeoordinatesx

gives

[x

;x

MB =x

?x

x

?x

=i

: (9)

It anbeeasilyveriedthefollowingpropertiesoftheMoyalprodut:

a) e ik x

?e iqy

=e i(k +q)x

e ik ^q

; (10)

wherek^q= 1

2 k

q

.

b) (f?g)(x)= Z

dk dq ~

f(k)~g(q)e ik ^q

e i(k +q)x

; (11)

where ~

f andg~aretheFourieromponentsof f and g,respetively.

) [(f?g)?h℄(x)=[f?(g?h)℄(x): (12)

d) Z

dx(f?g)(x)= Z

dx(g?f)(x)= Z

dxf(x)g(x): (13)

e) Z

dx(f

1 ?f

2 ?:::f

n )(x)=

Z

dx(f

n ?f

1 ?:::f

n 1

)(x): (14)

f) (f?g)

=g

?f

: (15)

III Nonommutative Salar Field Theory

Letusonsiderthemassivesalareld inD=3+1dimensions

[3℄,whoseationis

S= Z

d 4

x

1

2

?

m

2

2 ?

g 2

4!

???

: (16)

Usingpropertyd)itisseenthatthepropagatorisnotaetedbytheMoyalprodut. Thisisageneripropertyof

nonommutativeeld theories. Thevertex,however,mustbesymmetrized. Inmomentum spaewehave

g 2

2 Z

d 4

x???= g

2

6 Z

dk

1 dk

2 dk

3 dk

4 Æ(k

1 +k

2 +k

3 +k

4 )

[os( 1

2 k

1 ^k

2 )os(

1

2 k

3 ^k

4

)+os( 1

2 k

1 ^k

3 )os(

1

2 k

2 ^k

4 )+

os( 1

k

1 ^k

4 )os(

1

k

2 ^k

3 )℄(k

1 )(k

2 )(k

3 )(k

4

(3)

Then,theonelooporretionforthetwo-pointfuntionis

g 2

3(2) 4

Z

d 4

k

1+ 1

2

os(k^p)

1

k 2

+m 2

: (18)

The rst term is the usual one loop mass orretion of the ommutative theory (up to a fator 1=2) whih is

quadratiallydivergent. Theseond termisnotdivergentdue tothe osillatorynature ofos(k^p). This shows

that thenonloalityintroduedbytheMoyalprodutisnotbadandleavesuswiththesamedivergenestruture

of theommutativetheory. Totakeintoaounttheeet oftheseondtermweregularizetheintegralusingthe

Shwingerparametrization

1

k 2

+m 2

= Z

1

0 d e

(k 2

+m 2

)

e 1

2

; (19)

where autowasintrodued. Wend

(2)

= g

2

48 2

[( 2

m 2

ln(

2

m 2

)+:::)+ 1

2 (

2

eff m

2

ln(

2

eff

m 2

)+:::)℄; (20)

where

2

eff =

1

1

2

+p~ 2

; p~

=

p

: (21)

Notethatwhentheutoisremoved,!1,thenonommutativeontributionremainsniteprovidinganatural

regularization. Also 2

eff =

1

~ p 2

whih divergeseither when!0orwhenp~!0.

Theoneloopeetiveationisthen

Z

d 4

p 1

2 (p

2

+M 2

+

g 2

96 2

(~p 2

+1= 2

) g

2

M 2

96 2

ln

1

M 2

(~p 2

+1= 2

)

+:::)(p)( p); (22)

whereM istherenormalizedmass. Letustakethelimits!1andp~!0. Ifwetakerstp~!0thenp~ 2

<< 1

2

and

eff

= showingthat wereovertheeetiveommutativetheory

Z

d 4

p 1

2 p

2

+M 02

(p)( p): (23)

If,however,wetake!1thenp~ 2

>> 1

2

and 2

eff =

1

~ p 2

andweget

Z

d 4

p 1

2

p 2

+M 2

+ g

2

96 2

~ p 2

g 2

M 2

96 2

ln

1

M 2

~ p 2

+:::

(p)( p); (24)

d

whih is singular when p~ ! 0. This shows that the

limit !1 doesnotommutewith thelow

momen-tum limitp~! 0so that there is amixing of UV and

IR limits.

Thetheoryisrenormalizableatonelooporderifwe

do nottake p~! 0. What about higher loop orders?

Suppose we have insertions of one loop mass

orre-tions. Eventuallywe will haveto integrate over small

values of p~whih diverges when ! 1. Then we

nd an IR divergene in a massivetheory. This

om-bination of UV and IR divergenes makesthe theory

non-renormalizable.

Therearealsoexamplesofnon-renormalizable

the-oriesalreadyatonelooporder[5℄. Foraomplexsalar

theoryisone-loopnon-renormalizablewhile

??

?

givesaonelooprenormalizablemodel.

Then the questionis whether it would be possible

tondatheorywhih isrenormalizableto allloop

or-ders. Sinethe UV/IR mixing appearsat the level of

quadrati divergenes a andidate theory would be a

supersymmetri theory beause it does nothave suh

divergenes[9,10℄. Asweshallseethisindeedhappens.

IV Nonommutative W

ess-Zumino model

(4)

L

0 =

1

2

A

A+

1

2

B

B+

1

2

i6 ; (25)

L

m =

1

2 F

2

+ 1

2 G

2

+mFA+mGB 1

2

m ; (26)

L

g

= g(F?A?A F?B?B+G?A?B+G?B?A

? ?A ?i

5

?B); (27)

d

where A and B are bosoni elds, F and G are

aux-iliary elds and is a Majorana spinor. The ation

is invariant under the usual supersymmetry

transfor-mations. TheyarenotmodiedbytheMoyalprodut

sine they are linearin the elds. The elimination of

the auxiliary elds through their equations of motion

produesquartiinterations. Intermsoftheomplex

eld =A+iB we get

?

?? whih is

non-renormalizableinthenonommutativease. Thisasts

doubtsabouttherenormalizabilityofthemodelbutas

weshallseesupersymmetrysavestheday.

Asusual,thepropagatorsarenotmodiedby

non-ommutativityduetothepropertyd). Theyaregiven

by

AA

(p) = (p) i

p 2

m 2

+i

; (28)

FF

(p) = p 2

(p); (29)

AF

(p) =

FA

(p)= m(p); (30)

S(p) = i

6p m

: (31)

Takingintoaountthesymmetriesthevertiesare

FA 2

vextex: igos(p

1 ^p

2

); (32)

FB 2

vextex: igos(p

1 ^p

2

); (33)

GAB vertex: 2igos(p

1 ^p

2

); (34)

A vertex: igos(p

1 ^p

2

); (35)

B vertex: ig

5 os(p

1 ^p

2

): (36)

The degree of superial divergene for ageneri 1PI

graphisthen

d()=4 I

AF I

BF N

A N

B 2N

F 2N

G 3

2

N ; (37)

d

whereN

O

denotesthenumberofexternallines

assoi-ated totheeld O andI

AF and I

BF

are thenumbers

of internal lines assoiated to the mixed propagators

AF and BF, respetively. Inallaseswewill

regular-ize the divergentFeynman integralsby assuming that

asupersymmetri regularizationshemedoesexist.

The one loop analysis an be done in a

straight-forwardway. As in theommutativeaseall tadpoles

ontributionsadduptozero. Wehaveveriedthis

ex-pliitly. Theself-energyofAanbeomputedandthe

divergentpartisontainedin theintegral

16g 2

Z

d 4

k

(2) 4

(1+ 1

2

os(k^p))

(pk) 2

(k 2

m 2

) 3

: (38)

The rst term is logarithmially divergent. It diers

thisdivergeneiseliminatedbyawavefuntion

renor-malization. TheseondtermisUV onvergentandfor

smallpitbehavesasp 2

ln(p 2

=m 2

)andatuallyvanishes

forp=0. ThenthereisnoIRpole. Thesameanalysis

anbearriedoutfortheothers elds. ForF wend

that thedivergentpartis

4g 2

Z

d 4

k

(2) 4

(1+ 1

2

os(k^p)) 1

(k 2

m 2

) 2

: (39)

Thersttermislogarithmiallydivergentandanalso

beeliminatedbyawavefuntionrenormalization. The

seond term diverges as ln (p 2

=m 2

) as p goes to zero.

However its multiple insertions is harmless. For the

(5)

Thetermontainingos(k^p)behavesas6pln(p 2

=m 2

)

and vanishes aspgoes to zero. Therefore, there is no

UV/IR mixingintheself-energyasexpeted.

Toshowthat themodel isrenormalizablewemust

also look into the interations verties. The A 3

ver-tex hasnodivergentpartsasintheommutativease.

Thesamehappensfortheotherthree pointfuntions.

For the four point verties no divergene is found as

in the ommutativease. Hene,thenonommutative

Wess-Zuminomodelisrenormalizableatoneloopwith

awave-funtionrenormalizationandnoUV/IRmixing.

To go to higher loop orders we proeed as in the

ommutativease[11℄. Wederivedthesupersymmetry

Ward identities for the n-point vertex funtion. Then

weshowedthat thereisarenormalizationpresription

whihisonsistentwiththeWardidentities. Theyare

the same as in the ommutativease. Andnally we

xed theprimitivelydivergentvertex funtions. Then

we found that there is only a ommon wave funtion

renormalizationasintheommutativease. Ingeneral

weexpet

'

R =Z

1=2

'; m

R

=Zm+Æm; g

R =Z

3=2

Z 0

g:

(40)

Atoneloopwefound Æm=0andZ 0

=1. Weshowed

thatthisalsoholdstoallordersandnomass

renormal-izationisneeded.

Being the only onsistent nonommutative

quan-tum eld theory in 3+1 dimensions known so far

it is natural to study it in more detail. As a rst

stepin this diretion weonsidered thenonrelativisti

limitof thenonommutativeWess-Zumino model[12℄.

We foundthelowenergyeetivepotentialmediating

thefermion-fermionandboson-bosonelastisattering

in the nonrelativistiregime. Sine nonommutativity

breaks Lorentz invarianeweformulatedthetheoryin

theenterofmassframeofreferenewherethe

dynam-is simplies onsiderably. Forthe fermions we found

thatthepotentialissigniativelyhangedbythe

non-ommutativitywhilenomodiationwasfoundforthe

bosonisetor. Themodiationsfoundgiverisetoan

anisotropidierentialrosssetion.

V Nonommutative

Gross-Neveu and Nonlinear Sigma

Models

Anothermodelwherenonrenormalizabilityisspoiledby

thenonommutativityistheO(N)Gross-Neveumodel.

Thismodelisperturbativelyrenormalizablein1+1

di-mensions and 1=N renormalizablein 1+1and 2+1

dimensions. In both asesit presentsdynamial mass

generation. ItisdesribedbytheLagrangian

L= i

2 i

6

i +

g

4N (

i i

)(

j j

); (41)

where

i

;i = 1;:::N, are two-omponent Majorana

spinors. Sine it is renormalizable in the 1=N

expan-sionin1+1and2+1dimensionswewillonsiderboth

ases. Asusual, weintrodueanauxiliaryeld and

theLagrangianturnsinto

L= i

2 i

6

i

2 (

i i

) N

4g

2

: (42)

Replaing by +M where M is the VEV of the

originalwegetthegapequation(inEulideanspae)

M

2g Z

d D

k

(2) D

M

k 2

E +M

2

=0: (43)

ToeliminatetheUVdivergeneweneedtorenormalize

theouplingonstantby

1

g =

1

g

R +2

Z

d D

k

(2) D

1

k 2

E +

2

: (44)

In2+1dimensionswend

1

g

R =

jMj

2

; (45)

and thereforeonly for 1

gR +

2

> 0it is possible to

haveM 6=0,otherwiseM isneessarilyzero. Nosuh

arestrition exists in 1+1 dimensions. In any ase,

wewillfousonlyinthemassivephase. The

propaga-torfor isproportionaltotheinverseofthefollowing

expression

iN

2g iN

Z

d D

k

(2) D

k(k+p)+M 2

(k 2

M 2

)[(k+p) 2

M 2

; (46)

whihisdivergent. Takingintoaountthegapequationtheaboveexpressionreduesto

(p 2

4M 2

)N

2

Z

d D

k

(2) D

1

(k 2

M 2

)[(k+p) 2

M 2

; (47)

(6)

Thenonommutativemodelisdenedby

S

GN =

Z

d D

x

i

2

6

M

2

1

2

?( ? ) N

4g

2 N

2g M

: (48)

d

Elimination of the auxiliary eld results in a

four-fermioninterationofthetype

i ?

i ?

j ?

j

. However

amoregeneral four-fermioninteration may involvea

termlike

i ?

j ?

i ?

j

. This lastombination does

nothaveasimple1=N expansionand wewillnot

on-siderit. TheMoyalprodutdoesnotaetthe

propa-gatorsand thetrilinearvertexaquiresaorretionof

os(p

1 ^p

2

)withregardtotheommutativease. Hene

thegapequationisnotmodied,whilethepropagator

forthe isnowproportionaltotheinverseof

iN

2g N

Z

d D

k

(2) D

os 2

(k^p)

k(k+p)+M 2

(k 2

M 2

)[(k+p) 2

M 2

: (49)

d

Now thedivergentpartis nolonger aneledand this

turnsthemodelinto anonrenormalizableone.

Onthe other side, the nonlinear sigmamodel also

presents troublesin its nonommutative version. The

nonommutativemodelisdesribedby

L= 1

2 '

i (

2

+M 2

)'

i +

1

2 ?'

i ?'

i N

2g

; (50)

where '

i

, i = 1;:::;N, arereal salarelds, is the

auxiliaryeldandM isthegeneratedmass. The

lead-ingorretiontothe'self-energyis

i Z

d 2

k

(2) 2

os 2

(k^p)

(k+p) 2

M 2

(k); (51)

where

is the propagatorfor . As for the aseof

the salar eld this an be deomposed as a sum of

a quadratially divergent part and a UV nite part.

Again there is the UV/IR mixing destroying the 1=N

expansion.

VI Nonommutative

Super-symmetri Nonlinear Sigma

Model

The Lagrangian for the ommutative supersymmetri

sigmamodelisgivenby

L= 1

2

'

i

'

i +

i

2 i

6

i +

1

2 F

i F

i +'

i F

i +

1

2 '

i '

i 1

2 i

i i

'

i N

2g

; (52)

whereF

i

,i=1;:::;N,areauxiliaryelds. Furthermore,;and aretheLagrangemultiplierswhihimplement

thesupersymmetrionstraints. Afterthehangeofvariables!+2M,F !F M'whereM=< >,and

theshifts!+M and!+

0

, where

0

=<>,wearriveatamoresymmetriformfortheLagrangian

L =

1

2 '

i (

2

+M 2

)'

i +

1

2 i

(i6 M)

i +

1

2 F

2

i +M

2

' 2

i +

1

2

0 '

2

i

+ 1

2 '

2

i +'

i F

i 1

2 i

i

i '

i N

2g

N

g

M: (53)

Nowsupersymmetryrequires

0

= 2M 2

andthegapequationis

Z

d D

k

D i

2 2

= 1

(7)

soaoupling onstantrenormalizationis required. We nowmust examinewhether thepropagatorfor depends

onthethisrenormalization. Wendthatthetwopointfuntion for isproportionaltotheinverseof

(p 2

4M 2

)N

2

Z

d D

k

(2) D

1

(k 2

M 2

)[(k+p) 2

M 2

; (55)

whihisidentialtotheGross-Neveuase. Notiethat thegapequationwasnotused. Thenitenessoftheabove

expressionis aonsequeneofsupersymmetry.

Thenonommutativeversionofthesupersymmetri nonlinearsigmamodelisgivenby

L =

1

2 '

i (

2

+M 2

)'

i +

1

2 i

(i6 M)

i +

1

2 F

2

i +

2 ?'

i ?'

i

1

2 F

i

?(?'

i +'

i ?)

1

2 ?

i ?

i 1

2 (

?

i ?'

i +

?'

i ?

i )

N

2g

NM

g

: (56)

Notie that supersymmetryditates theform of thetrilinear verties. Also, the supersymmetrytransformations

arenotmodiedbynonommutativitysinetheyarelinearandnoMoyalprodutsarerequired.

Thepropagatorsare thesameasin the ommutativease. Theverties haveosine fatorsdue to theMoyal

produt

' 2

vertex:

i

2 os(p

1 ^p

2

); (57)

'F vertex: ios(p

1 ^p

2

); (58)

vertex:

i

2 os(p

1 ^p

2

); (59)

' vertex: ios(p

1 ^p

2

): (60)

We again onsider the propagatorsfor the Lagrange multiplier elds. Now the propagator is modied by the

osine fatorsandisproportionalto theinverseof

(p 2

4M 2

)N

2

Z

d D

k

(2) D

os 2

(k^p)

(k 2

M 2

)[(k+p) 2

M 2

: (61)

It iswellbehavedbothin UVandIR regions. Thepropagatorsforand areproportionaltotheinverseof

N

2 Z

d D

k

(2) D

os 2

(k^p)

1

[(k+p) 2

M 2

℄[k 2

M 2

; (62)

and

N

(6p+2M)

2 Z

d D

k

(2) D

os 2

(k^p)

1

[(k+p) 2

M 2

℄[k 2

M 2

; (63)

respetively. Theyarealsowellbehavedin UVandIR regions.

Thedegreeofsuperialdivergeneforageneri1PIgraphis

d()=D

(D 1)

2 N

(D 2)

2 N

' D

2 N

F N

3

2 N

2N

; (64)

d

whereN

O

isthenumberofexternallinesassoiatedto

the eld O. Potentiallydangerousdiagrams are those

ontributingto theself{energiesof the 'and elds

sine, in priniple,they are quadrati and linearly

di-vergent,respetively. Forthe self-energiesof ' and

wendthat theydivergelogarithmiallyand theyan

respetive eld. The same happens for the auxiliary

eld F. The renormalizationfatorsfor them are the

same so supersymmetry is preserved in the

nonom-mutativetheory. Thisanalysisanbeextendedto the

n-point funtions. In 2+1 dimensions we nd

(8)

leading order of 1=N. However, in 1+1 dimensions

there some peuliarities. Sine the salar eld is

di-mensionless in 1+1 dimensions any graph involving

anarbitrarynumberofexternal'linesisquadratially

divergent. In the four-point funtion there is a

par-tialanellationofdivergenesbutalogarithmi

diver-genestillsurvives. Theountertermneededtoremove

itannotbewrittenintermsof R

d 2

x'

i ?'

i ?'

j ?'

j

and R

d 2

x'

i ?'

j ?'

i ?'

j

. A possible wayto remove

this divergeneis bygeneralizingthedenition of 1PI

diagram alongthe lines suggestedin [13℄ forthe

om-mutative nonlinear sigma model. However the osine

fators do not allow us to use this mehanism whih

astsdoubtabouttherenormalizabilityofthe

nonom-mutativesupersymmetriO(N)nonlinearsigmamodel

in1+1dimensions.

VII Conlusions

We have shown that it is possibleto build onsistent

quantum eld theories in nonommutative spae. It

seemsthatsupersymmetryisanessentialingredientfor

renormalizability. The models studied heredonot

in-volvegauge elds and this onsiderably simplies the

situation. All verties are deformed in the same way

bytheMoyalprodutandthiswasessentialtoanalyze

theamplitudes. Withgaugeeldsthesituationismuh

moreompliatedbeausethevertiesaredeformedin

dierent ways. However, supersymmetri gauge

theo-riesmaystillhaveabetterbehavior.

Aknowledgments

This work was done in ollaboration with H. O.

Girotti,M.Gomes andA.J.daSilva. Itwaspartially

supported by Funda~ao deAmparo aPesquisa do

Es-tado de S~ao Paulo (FAPESP), Conselho Naional de

DesenvolvimentoCientoeTenologio(CNPq),and

PRONEXunderontratCNPq66.2002/1998-99.

Referenes

[1℄ N. Seiberg and E. Witten, \String Theory and

Non-ommutativeGeometry",hep-th/9908142,JHEP9909,

032(1999).

[2℄ T.Filk,Phys.Lett.B376,53(1996).

[3℄ S. Minwalla, M. Van Raamsdonk and N. Seiberg,

\Nonommutative Perturbative Dynamis",

hep-th/9912072.

[4℄ I.Y.Aref'eva,D.M.BelovandA.S.Koshelev,

\Two-loop Diagrams in Nonommutative 4

4

Theory",

hep-th/9912075.

[5℄ I. Y. Aref'eva, D. M. Belov and A. S.Koshelev, \A

note onUV/IR for NonommutativeComplex Salar

Field",hep-th/0001215.

[6℄ H. O. Girotti, M. Gomes, V. O. Rivelles, A. J. da

Silva, \A Consistent Nonommutative Field Theory:

theWess-ZuminoModel",hep-th/0005272,Nul.Phys.

B587,299(2000).

[7℄ H. O. Girotti, M. Gomes, V. O. Rivelles, A. J. da

Silva,\TheNonommutativeSupersymmetri

Nonlin-earSigmaModel",hep-th/0102101.

[8℄ N. Seiberg, L. Susskind, N. Toumbas, \Spae/Time

Non-Commutativity and Causality", hep-th/0005015,

JHEP0006(2000)044.

[9℄ I.ChepelevandR.Roiban,\Renormalizationof

Quan-tumeldTheoriesonNonommutativeR d

.I:Salars,"

hep-th/9911098.

[10℄ S. Ferrara and M. A. Lledo, \Some aspets of

De-formations of Supersymmetri Field Theories,"

hep-th/0002084.

[11℄ J.IliopoulosandB.Zumino,\Brokensupergauge

sym-metry and renormalization", Nul. Phys. B 76, 310

(1974).

[12℄ H.O.Girotti, M.Gomes,V.O.Rivelles, A.J.daSilva,

\TheLowEnergyLimitoftheNonommutative

Wess-ZuminoModel",hep-th/0101159.

[13℄ I. Ya. Aref'eva, Theor. Math. Phys. 36, 573 (1979);

Ann.Phys.(NY)117,393(1979);I.Ya.Aref'eva,E.

R.NissimovandS.J.Paheva,Commun.Math.Phys.

71, 213 (1980). See also J.H. Lowenstein and E. R.

Referências

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