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Contents lists available atScienceDirect

Physics Letters B

www.elsevier.com/locate/physletb

Leptonic CP violation in flipped SU(5) GUT from Z 12 − I orbifold compactification

Junu Jeong

a,b

, Jihn E. Kim

a,c,d,

, Soonkeon Nam

c

aCenterforAxionandPrecisionPhysicsResearch(InstituteofBasicScience),KAISTMunjiCampus,193Munjiro,Daejeon34051,RepublicofKorea bDepartmentofPhysics,KAIST,291Daehakro,Yuseong-Gu,Daejeon,14141,RepublicofKorea

cDepartmentofPhysics,KyungHeeUniversity,26Gyungheedaero,Dongdaemun-Gu,Seoul02447,RepublicofKorea dDepartmentofPhysicsandAstronomy,SeoulNationalUniversity,1Gwanakro,Gwanak-Gu,Seoul08826,RepublicofKorea

a r t i c l e i n f o a b s t ra c t

Articlehistory:

Received9January2019

Receivedinrevisedform4February2019 Accepted21February2019

Availableonline26February2019 Editor:M.Cvetiˇc

Keywords:

Stringcompactification FlippedSU(5)GUT PMNSmatrix Kim-Seoform Jarlskogdeterminant

We obtain a phenomenologically acceptable PMNS matrix in a flipped SU(5) model, possessing the Z4R discretesymmetry, fromthe compactification ofheterotic string E8×E8.To analyze the Jarlskog determinantefficiently,weincludethesimpleKim-SeoformforthePontecorbo-Maki-Nakagawa-Sakata matrix.Wealsonotedthat|δPMNS|63oforthenormalhierarchyofneutrinomasseswiththePDGbook parametrization.

©2019TheAuthor(s).PublishedbyElsevierB.V.ThisisanopenaccessarticleundertheCCBYlicense (http://creativecommons.org/licenses/by/4.0/).FundedbySCOAP3.

1. Introduction

The most urgent theoretical issue in the standard model(SM) is probing the symmetry structure from which the observed flavor phenomenacan beunderstood.It isdesirableifsuchsymmetry resultsfromanultra-violet completedtheory.Atpresent, stringtheory isconsidered tobethemostattractiveoneamongvariousultra-violetcompletedtheories,chieflybecauseitunifiesgravityonthesame groundasgaugetheories.TheSMisobtainedfromcompactificationofsixextradimensions[1–6],andthesymmetrystructureofflavors istheonerealizedbelowthecompactificationscale.

Previously,moststudiesalongthisdirectionwerecenteredonobtainingthreefamiliesinthestandard-likemodels[7,8].1 Sincethere aretoomanyYukawacouplingsinstandard-likemodels,hereweattempttoworkina grandunification(GUT) models.TheGUTgroup weusehereisthe rank5flippedSU(5)GUT[11,12],SU(5)flipSU(5)×U(1)X,which wasobtainedfromcompactifications viafermionic string[13] andZ12I orbifold[14].The simplestGUTSU(5)fromstringcompactification isnotaccompanying an adjointrepresentation atthelevel1constructionwheretheHiggsmultipletneededforbreakingSU(5)downtotheSMislacking.Therank5SU(5)flip requires 1010forbreakingitdowntotherank4SMgaugegroup,andthemodelof[10] containsthem.

Timeis ripe enough to study the details of the flavor structure fromstring compactification to see whether they convergeto the observeddata.The studyisnowpossibleintheZ4R model[9] basedon[10] wheretheneededZ4R quantumnumbersofalllightchiral fields are presented.In the quark sector, the Cabibbo-Kobayashi-Maskawa matrix [15,16] has been studied in ourprevious paper[17].

Inthispaper,wepresentanumericalstudyonthePontecorbo-Maki-Nakagawa-Sakata (PMNS)matrix[18,19] viamanyU(1)’sarising in stringcompactification.Theheterotic stringE8×E8 hasrank16gaugesector.Themodelpresentedin[10] hastheSU(5)flipfromE8 and

*

Correspondingauthor.

E-mailaddress:[email protected](J.E. Kim).

1 Formorereferences,see[9].

https://doi.org/10.1016/j.physletb.2019.02.035

0370-2693/©2019TheAuthor(s).PublishedbyElsevierB.V.ThisisanopenaccessarticleundertheCCBYlicense(http://creativecommons.org/licenses/by/4.0/).Fundedby SCOAP3.

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Fig. 1.A neutrino interaction with the SM fields only.

Table 1

U(1)chargesofmatterfieldsintheflippedSU(5).ξiandη¯icontaintheleft-handedquarkandleptondoublets,respectively,inthei-thfamily.

State(P+kV0) i RX(Sect.) QR Q1 Q2 Q3 Q4 Q5 Q6 Qanom Q18 Q20 Q22

ξ3 (+ + + − −; − − +)(08) 0 101(U3) +166 +6 0 0 013 +11 +1

¯

η3 (+ − − − −; + − −)(08) 0 5+3(U3) +1 +666 0 0 01 +11 +1

τc (+ + + + +; − + −)(08) 0 15(U3) +16 +66 0 0 0 +5 +11 +1

ξ2 (+ + + − −; −16,16,16)(08) +41 101(T40)1222 0 0 03111

¯

η2 (+ − − − −; −16,16,16)(08) +41 5+3(T04)1222 0 0 03111

μc (+ + + + +; −16,16,16)(08) +41 15(T04)1222 0 0 03111

ξ1 (+ + + − −; −16,16,16)(08) +41 101(T40)1222 0 0 03111

¯

η1 (+ − − − −; −16,16,16)(08) +41 5+3(T04)1222 0 0 03111

ec (+ + + + +; −16,16,16)(08) +41 15(T04)1222 0 0 03111

HuL (+1 0 0 0 0;0 0 0)(05;21 +1

2 0) +31 2·52(T6)2 0 0 012 0 0 0111

HdL (1 0 0 0 0;0 0 0)(05;+21 1

2 0) +31 2·5+2(T6) +2 0 0 0 +12 0 0 0111

SU(5)×SU(2) fromE8,andwe can consider 6extra U(1) gauge groups. Thesemany U(1)’s make itpossible to haveflavor dependent Yukawacouplings.2

StringcompactificationinourexampleallowsalltheneededYukawacouplingsintheSMasnon-renormalizableforms.Therehasbeen an ambitious attempt[21] to relate the originofthe

μ

termwith themagnitudes ofneutrino massesby introducing justone singlet chiral field beyondthe minimal supersymmetricSM. Thistry allowed only renormalizable couplings. Therefore,withso many singlets participatingthroughnon-renormalizableYukawacouplingsinourmodel,thisdesignisnotapplicable.Therelationsinourmodelmight beintertwinedinanelaboratewaysincetheZ4R discretesymmetryautomaticallygivesthe

μ

termattheelectroweakscale[22].Since ourZ4R isasubgroupofanAbeliangaugegroupU(1)6,itcannotbeanon-Abeliandiscretesymmetrysuchastheinteresting A4 symmetry [23].

The massmatrices leading to the Kim-Seo(KS) parametrization [24] ofthe CKM and PMNSmixing matriceshave a smallnumber ofcomplexelements,bymaking onerowconsistofrealnumbers.Attheplaces wherecomplexentriesareallowed,we allocatetheCP phase.TheKSformhasanotheradvantagethattheJarlskogdeterminantis J= −ImV31KSV22KSV13KS [25].Towardamodelbuilding,thenext stepistoobtainphenomenologicallyacceptablemassmatrices.IntheflippedSU(5),theneutrinomassmatrixissymmetric,canbemade real,andhenceweproposeinthispapertoputtheCPphaseinthechargedleptonmassmatrix.

ThestringmodelgivestheYukawacouplingsforthechargedleptonmassesandneutrinomasses.Thus,inSec.2wepresentthelepton massmatricesfromtheflippedSU(5)model,i.e.allowedbythequantumnumbersofRef. [9],intheformsrelatedtotheKSmixingmatrix.

Then,we locatepossiblephasesinthecomplexvacuumexpectationvalues(VEVs)ofthe SMsingletfields

σ

i.NextinSec.3,we relate theseleptonicmassmatriceswiththePMNSmatrixandcompareitwiththedatapresentedintheParticleDataBook[26].InSec.4,we presentnumerical analysesandobtain|δPMNS|<62.8o forthe normalhierarchyofneutrinomasseswiththePDGbookparametrization [26].Section5isaconclusion.ThemagnitudeontheweakCPviolation J [27] isbrieflydiscussedinAppendixA.

2. Suggestionfromtheflipped SU(5)model

IfweconsideronlytheSMparticles,neutrinomassesarisefromthediagramshowninFig.1.Anyfurtherattachmentstothisdiagram areSM singletscalars.Ifwe considerthequantumnumbers underSU(2)W×U(1)Y,two neutrinoshave1131 where ↑means that the 3rd component of the weak isospin is +1. Possible additional scalar attachments to Fig. 1 must carry quantum number 1+1 or 3+1 together withtwo Hu0’s, and 1+1 is ruled out because 1+1 breaks U(1)em. 3+1 allows the scalar attachments, shown as HuHu in Fig. 1. Depending ondetails of highenergyfields, implied by thequestion markinthe gray, two typesof neutrinomassesare named,TypeIseesaw[28] andTypeIIseesaw[29].TypeIIIseesaw[30] requiresmorelightparticlesattheelectroweakscale.Fromthe SU(5)flipspectrashowninRef. [20],wenote thatthereisnoSU(2)tripletrepresentation;henceonlyTypeIseesawisallowed fromour stringcompactification.

2 Amongthese,theanomalousU(1)canworkasaflavorsymmetry[20].NotethatinadditiontotheseweuseU(1)’sfromtheextradimensionstowardZ4Rdiscrete symmetryinRef. [9].

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Table 2

U(1)chargesofL-handedneutralscalars(but σ7,8forR-handed).Wekeptuptooneoscillatorrepresented asNumberofresultingfields(number of oscillating mode).For example,n(11¯)meansthatthereresultsnmultiplicitieswithoneoscillator 125.For Q18,20,22charges,herewelistedonlythoseofL-handedfields,participatinginthe Yukawacouplings.σ2,3,4,11,15,21,22,23,24havephasei=0,whichcanbeusedtobreakZ4RdowntoZ2R.

State(P+kV0) i (NL)j P·RX(Sect.) QR Q1 Q2 Q3 Q4 Q5 Q6 Qanom Q18 Q20 Q22

1 (+ + + − −;03)(05;411 4 +2

4) 0 2(11) 2101(T3)L +4 0 0 0 0 +9 +3 7331 +11

1 (+ + + − −;03)(05;411 4 +2

4) +32 1(13) 1101(T3)L +4 0 0 0 0 +9 +3 7331 +11

2 (+ + − − −;03)(05;+41+1 4 2

4) 0 2(1¯1) 210+1(T3)L4 0 0 0 093 +733111

2 (+ + − − −;03)(05;+41+1 4 2

4) +31 1(1¯3) 110+1(T3)L4 0 0 0 093 +733111

σ1 (05;322 3 2

3)(08) +41 0 2·10(T04)4888 0 0 012111

σ2 (05;32+1 3 +1

3)(08) 0 3(1¯1) 3·10(T04) 08 +4 +4 0 0 02111

σ3 (05;13 2 3

1

3)(08) 0 3(1¯1) 3·10(T04) 0 +48 +4 0 0 08111

σ4 (05;13 1 32

3)(08) 0 3(1¯1) 3·10(T04) 0 +4 +48 0 0 0 +10111

σ5 (05;010)(05;121

2 0) +21 0 2·10(T6) +4 0 +12 0 +12 0 0 +14111

σ6 (05;001)(05;21 1

20) +21 0 2·10(T6) 0 0 0 +1212 0 04111

σ7 (05;010)(05;21 1

20) +21 0 2·10(T6)R +4 0 +12 0 +12 0 0 +141 +11

σ8 (05;001)(05;121

2 0) +21 0 2·10(T6)R2 0 0 +1212 0 041 +11

σ11 (05;211 2 1

2)(05;341 4 1

2) +32 2(11+13,11¯+13¯) 2·10(T3)6666 +1293 730 +1 +11 σ11 (05;211

2 1 2)(05;341

4 1

2) 0 4(11+13,11¯+13¯) 4·10(T3)6666 +1293 7301 +1 +1 σ12 (05;21

1 2 1 2)(05;341

4 1

2) +31 2(11+13,11¯+13¯) 2·10(T3)26 +6 +6 +1293 +740 +1 +11 σ12 (05;21

1 2 1 2)(05;341

4 1

2) +32 2(11+13,11¯+13¯) 2·10(T3)26 +6 +6 +1293 +7401 +1 +1 σ13 (05;12

1 21

2 )(05;41 3 41

2) +31 2(11+13,11¯+13¯) 2·10(T3)6 +6 +661293 +1247 +1 +11 σ13 (05;12

1 21

2 )(05;41 3 41

2) +32 2(11+13,11¯+13¯) 2·10(T3)6 +6 +661293 +12471 +1 +1 σ14 (05;12

1 21

2 )(05;41 1 4

1

2) +32 2(1¯1)+1(13¯) 3·10(T3) +4 +6 +66 0 +9 +3 +7581 +1 +1

σ15 (05;211 2 1

2)(05;+43 1 4 1

2) +32 2(11+13,11¯+13¯) 2·10(T3)6666 +1293 730 +1 +11 σ15 (05;211

2 1

2)(05;+43 1 4 1

2) 0 2(11+13,11¯+13¯) 4·10(T3)6666 +1293 7301 +1 +1 σ16 (05;21+1

2 +1

2)(05;+43 1 4 1

2) +31 2(11+13,11¯+13¯) 2·10(T3)26 +6 +6 +1293 +740 +1 +11 σ16 (05;21+1

2 +1

2)(05;+43 1 4 1

2) +32 2(11+13,11¯+13¯) 2·10(T3)26 +6 +6 +1293 +7401 +1 +1 σ17 (05;+21+1

2 1

2)(05;41 +3 4 1

2) +31 2(11+13,11¯+13¯) 2·10(T3)6 +6 +661293 +1247 +1 +11 σ17 (05;+21+1

2 1

2)(05;41 +3 4 1

2) +32 2(11+13,11¯+13¯) 2·10(T3)6 +6 +661293 +12471 +1 +1 σ18 (05;12 +1

2 1

2)(05;+431 4 1

2) +32 2(1¯1)+1(13¯) 2·10(T3) +4 +6 +66 0 +9 +3 +7581 +1 +1

σ21 (05;611 6 1

6)(05;14 1 4 1

2) 0 1(1¯1) 10(T10) +2222 0 +9 +3 +712111

σ22 (05;65 1 6 1 6)(05;14

1 41

2) 0 1(1¯1+13) 10(T50) +210 +2 +2 0 +9 +3 721 +1 +1

σ23 (05;16 5 6

1 6)(05;14

1 41

2) 0 1(1¯1+13) 10(T50) +210 +2 +2 0 +9 +3 7441 +1 +1

σ24 (05;16 1 65

6)(05;14 1 41

2) 0 1(1¯1+13) 10(T50) +210 +2 +2 0 +9 +3 +7821 +1 +1

TheSM fieldsfrom[9] areshowninTable1,andtheSM singletfields,includingthose in101 and10+1 ofSU(5)flip,areshownin Table2.ConsideringtheSM singletattachments to Fig.1,letusconsidertheneutrinomassoperatorsallowed bythequantumnumbers ofTables1and2.Firstly,thediagonalmassesare

Mν33

M

˜

133

d2

ϑ

5+3

(

U3

,

0

; +

1

)

5+3

(

U3

,

0

; +

1

)

52

(

T6

,

1

3

; −

2

)

52

(

T6

,

1

3

; −

2

)

101

(

T3

,

1

3

; +

4

)

101

(

T3

,

0

; +

4

)

Mν22

M

˜

142

d2

ϑ

5+3

(

T40

,

1

4

; −

1

)

5+3

(

T40

,

1

4

; −

1

)

52

(

T6

,

1

3

; −

2

)

52

(

T6

,

1

3

; −

2

)

101

(

T3

,

1

3

; +

4

)

101

(

T3

,

0

; +

4

)

·

10

( σ

5

,

T6

,

1 2

; +

4

)

(1)

wherethelastnumberafter;isthe QR charge,andM˜3 andM˜2 aredeterminedby?inFig.1.Weneed QR=2 modulo4aboveford2ϑ integration.

11,Mν 12,Mν

21havethesamestructureas

22.Notethattheselectionruleismakingthephaseanintegermultiple,whichis satisfiedabovefori,viz.0+0+13+13+13+0=1 and 14+14+13+13+13+0+12=2.Then,theabovemassesareestimatedas

Mν33

v2E WM

˜

M33210

,

Mν22

v2E WM102

| σ

5

|

M

˜

42

,

(2)

whereM10= 101 = 10+1 .Then,neutrinomixingmassesaregenerallyoforder v2E W/M˜ sincetheSMsingletVEV

σ

5 canbeatthe GUTscalewithoutbreakingZ4R.

Fortheoff-diagonalmassesbetweenU3 andT40neutrinos,weneed QR=0 modulo4ford2ϑd2ϑ¯ integration.

Mν32

,

Mν31

M

˜

16

d2

ϑ

d2

ϑ ¯

5+3

(

U3

,

0

; +

1

)

5+3

(

T40

,

1

4

; −

1

)

52

(

T6

,

1

3

; −

2

)

52

(

T6

,

1 3

; −

2

)

·

101

(

T3

,

0

; +

4

)

101

(

T3

,

0

; +

4

) ·

10

( σ

1

,

T40

,

1

4

; −

4

)

10

( σ

14

,

T3

,

2 3

; +

4

)

.

(3)

(4)

Then,theabovemassmixingisestimatedas Mν13,23

v2E WM210

| σ

1

σ

14

|

M

˜

×5

,

(4)

whereM˜× issomemassscaledeterminedbytheaboveequations.Notethat2,1 and

σ

1 canhavetheGUTscaleVEVsbecauseallof themcarry QR=0 modulo4,andweobtainasimilarorderofmassforallofMν11,12,22,33,13,23.

Comparing

11,22,31,32and 33, Mν11

,

Mν22

Mν33

≈ σ

5

M

˜ ,

M

ν 31

,

Mν32

M33ν

≈ σ

1

σ

14

M

˜

2

,

(5)

wenotethattheneutrinomasshierarchycanbethenormalhierarchy(inthesensethat

ν

τ istheheaviest)iftheVEVsof

σ

singletsare comparablysmall,|

σ

1|,|

σ

5|<M

Sinceweobtainedallentriesintheneutrinomassmatrix,hereweinvestigatehowtheCPphasecanbeinsertedinthemassmatrix ofthe Qem= −1 leptonsandintheneutrinomassmatrix.

2.1. NeutrinomassmatrixinspiredbyflippedSU(5)

InRef. [9] basedontheflippedSU(5)modelof[10],apossibleidentificationZ4R hasbeenachieved,forbiddingdimension-5Bviolating operatorsbutallowing theelectroweakscale

μ

termanddimension-5Lviolating Weinbergoperator.IntheflippedSU(5), theneutrino massesariseintheform

I J

=

fI J(ν)

({ σ })

5+I,i35+J,3j5k2

(

Hu

)

5l2

(

Hu

)[

101

(

HGUT

)

101

(

HGUT

)]

i jkl

+

h

.

c

.,

(6) wherethecouplings f(ν)

I J arecomplexparameters, I and J areflavorindices,i,j,k,l,mareSU(5)indices,andthesubscriptistheU(1)X quantumnumberofSU(5)flip.52 isusuallydenotedasHuL,and101,togetherwith10+1,istheten-pletneededforbreakingtherank 5gaugegroupSU(5)×U(1)ataGUTscaledowntotherank4SMgaugegroup.

Consider 5+I,i35+J,3j inEq. (6) which is symmetricunder I and J.Thus, the neutrino massmatrix is symmetric.The Majorana phase factoredout in Eq. (20) is fromtheheavy neutrinos, whichwill not affectourstudyof CC interactions ofSec. 3.We assume that the neutrinomassmatrix,beingsymmetric,isreal.Thus, V(ν)canbeconsideredtobeanorthogonalmatrix O(ν).

2.2. MassmatrixofchargedleptonsinspiredbyflippedSU(5)

Ascommentedabove, wecanalways take V(ν) asa realmatrix O(ν).Thus,the PMNSmatrixgivenintheKSform, Eq. (25),can be representedas

VKS(l)

=

V(e)O(ν)T

=

q11r11

+

q12r12

+

q13r13

,

q11r21

+

q12r22

+

q13r23

,

q11r31

+

q12r32

+

q13r33

,

q21r11

+

q22r12

+

q23r13

,

q21r21

+

q22r22

+

q23r23

,

q21r31

+

q22r32

+

q23r33

,

q31r11

+

q32r12

+

q33r13

,

q31r21

+

q32r22

+

q33r23

,

q31r31

+

q32r32

+

q33r33

,

(7)

wheretheelements Vi j(l)=qi j andO(ν)

i j =ri j arecomplexandrealnumbers,respectively.Makingthe1strowrealfortheKSform,q11,q12 andq13arerequiredtobereal.

Theunitarymatricesrelatingtheweakeigenstateslamdmasseigenstatesi ofthechargedleptonsarenamedasV forL-handedfields andU forR-handedfields,

lL

=

3

j=1

Vlj(l)l(jLmass)

,

lR

=

3

j=1

Ulj(l)l(j Rmass)

,

(8)

where¯lLmass=(1,2,3)L intermsofmasseigenstates1,2,3,andlmassR =(N1,N2,N3)R.Themassmatrixbecomes

¯

lL

(

Ve(l)MmassU(el)

)

lR (9)

intheweakeigenstatebasis.SinceR-handedleptonsarenotparticipatingintheCCinteractions,theleptonR-handedunitarymatrixU(l) canbetakenastheidentitymatrix.Thus,themassmatrixintheweakbasisbecomes

M(l)

=

V(l)

m

˜

e

,

0

,

0 0

,

m

˜

μ

,

0 0

,

0

,

1

U(l)

=

q11m

˜

e

,

q12m

˜

μ

,

q13

q21m

˜

e

,

q22m

˜

μ

,

q23 q31m

˜

e

,

q32m

˜

μ

,

q33

⎠ =

real

,

real

,

real complex

,

complex

,

complex complex

,

complex

,

complex

(10)

whereVi j(l)=qi j andweobtainedq11,q12andq13arerealnumbers.

We show that the quantumnumbers of themodel presented in[9] allows an effectivemass matrix formEq. (10) forthe charged leptons.

LlI J

=

fI J(l)

({ σ })

5+I,i31J55+2,

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