15
LMU-ASC 22/15, IFIC/15-23, FLAVOUR(267104)-ERC-95 Family non-universal Z 0 models with protected flavor-changing interactions Alejandro Celis, 1, * Javier Fuentes-Mart´ ın, 2, Martin Jung, 3, 4, and Hugo Serˆ odio 5, § 1 Ludwig-Maximilians-Universit¨ at M¨ unchen, Fakult¨at f¨ ur Physik, Arnold Sommerfeld Center for Theoretical Physics, 80333 M¨ unchen, Germany 2 Instituto de F´ ısica Corpuscular, Universitat de Val` encia - CSIC, Apt. Correus 22085, E-46071 Val` encia, Spain 3 TUM Institute for Advanced Study, Lichtenbergstr. 2a, D-85747 Garching, Germany. 4 Excellence Cluster Universe, Technische Universit¨ at M¨ unchen, Boltzmannstr. 2, D-85748 Garching, Germany. 5 Department of Physics, Korea Advanced Institute of Science and Technology, 335 Gwahak-ro, Yuseong-gu, Daejeon 305-701, Republic of Korea (Dated: June 29, 2015) We define a new class of Z 0 models with neutral flavor-changing interactions at tree level in the down-quark sector. They are related in an exact way to elements of the quark mixing matrix due to an underlying flavored U(1) 0 gauge symmetry, rendering these models particularly predictive. The same symmetry implies lepton-flavor non-universal couplings, fully determined by the gauge structure of the model. Our models allow to address presently observed deviations from the SM and specific correlations among the new physics contributions to the Wilson coefficients C (0)9,10 can be tested in b s‘ + - transitions. We furthermore predict lepton-universality violations in Z 0 decays, testable at the LHC. I. INTRODUCTION The Standard Model (SM) of electroweak interac- tions [1], based on the gauge group G SM SU(2) L × U(1) Y , has been tested to very high accuracy over the last decades. This has strong implications for new physics (NP) scenarios, which are then required to in- volve a very high mass scale, a highly non-trivial fla- vor structure, or both. Recently the LHCb collaboration has performed two measurements involving semileptonic b s‘ + - transitions which show deviations with re- spect to the SM expectations: The ratio R K = Br(B + μ - )/Br(B Ke + e - ) has been measured with a central value indicating a violation of lepton universal- ity at the 25% level [2], implying a 2.6σ deviation, and the observable P 0 5 obtained from the angular analysis of B K * μ + μ - decays differs from the SM expectation with 2.9σ significance [3]. Taking these measurements at face value, they require the NP to have the following features: (i) Sizable contributions to b s‘ + - transitions, (ii) lepton non-universal couplings. Extensions of the SM gauge group by an additional U(1) 0 factor are among the possible NP scenarios that could explain these deviations [4–10] (other NP interpre- tations have been discussed e.g. in Refs. [11–14]). Such U(1) 0 models have been popular extensions of the SM for many years, see Ref. [15] and references therein. How- ever, the majority of the extensions considered in the * [email protected] javier.fuentes@ific.uv.es [email protected] § [email protected] literature are family universal in the quark (and charged- lepton) sector, and therefore do not meet condition (ii). Models with departures from family universality can give rise to large flavor changing Z 0 interactions, which are strongly constrained by current flavor data [9, 16, 17]. The conditions (i) and (ii) therefore limit considerably the viable U(1) 0 gauge symmetries. Starting a new construction with the minimal particle content, i.e. the SM one without right-handed neutrinos, the only possible extension is gauging one of the combi- nations of family-specific lepton number, L α - L β (with α, β = e, μ, τ and α 6= β) [18]. Since the resulting Z 0 boson couples only to leptons, these models do not meet requirement (i) and have been discussed mostly in the context of neutrino phenomenology, usually considering the L μ - L τ symmetry [19]. Recent models [4, 5] cir- cumvent this problem by introducing additional fermions (vector-like quarks). This yields the required couplings at an effective level. In order to avoid such exotic vector-like quarks, the U(1) 0 symmetry has to involve both quarks and leptons, and should be family-dependent in order to satisfy condi- tions (i) and (ii). However, such a non-trivial flavor sym- metry in the quark sector requires the extension of the scalar sector in order to accommodate the quark masses and mixing angles [20]. It has been shown in Ref. [6] that this option can be realized by including an additional complex scalar doublet. This model generates flavor- changing phenomena in the down-quark sector which are related in a first approximation to the Cabibbo– Kobayashi–Maskawa (CKM) mixing matrix [21]. Flavor- changing interactions are also present in the up-quark sector of this model, but these are not related to CKM matrix elements or quark masses. We would like our model to have all of its fermion couplings related exactly to elements of the CKM ma- trix. To that aim, we note that there is a class of two- Higgs-doublet models (2HDM) that achieves this, known arXiv:1505.03079v2 [hep-ph] 26 Jun 2015

arXiv:1505.03079v2 [hep-ph] 26 Jun 2015 · Alejandro Celis,1, Javier Fuentes-Mart n,2, yMartin Jung,3,4, zand Hugo Ser^odio5, x 1Ludwig-Maximilians-Universit at Munchen, Fakult at

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Page 1: arXiv:1505.03079v2 [hep-ph] 26 Jun 2015 · Alejandro Celis,1, Javier Fuentes-Mart n,2, yMartin Jung,3,4, zand Hugo Ser^odio5, x 1Ludwig-Maximilians-Universit at Munchen, Fakult at

LMU-ASC 22/15, IFIC/15-23, FLAVOUR(267104)-ERC-95

Family non-universal Z′ models with protected flavor-changing interactions

Alejandro Celis,1, ∗ Javier Fuentes-Martın,2, † Martin Jung,3, 4, ‡ and Hugo Serodio5, §

1Ludwig-Maximilians-Universitat Munchen, Fakultat fur Physik,Arnold Sommerfeld Center for Theoretical Physics, 80333 Munchen, Germany

2Instituto de Fısica Corpuscular, Universitat de Valencia - CSIC, Apt. Correus 22085, E-46071 Valencia, Spain3TUM Institute for Advanced Study, Lichtenbergstr. 2a, D-85747 Garching, Germany.

4Excellence Cluster Universe, Technische Universitat Munchen, Boltzmannstr. 2, D-85748 Garching, Germany.5Department of Physics, Korea Advanced Institute of Science and Technology,

335 Gwahak-ro, Yuseong-gu, Daejeon 305-701, Republic of Korea(Dated: June 29, 2015)

We define a new class of Z′ models with neutral flavor-changing interactions at tree level in thedown-quark sector. They are related in an exact way to elements of the quark mixing matrix dueto an underlying flavored U(1)′ gauge symmetry, rendering these models particularly predictive.The same symmetry implies lepton-flavor non-universal couplings, fully determined by the gaugestructure of the model. Our models allow to address presently observed deviations from the SM and

specific correlations among the new physics contributions to the Wilson coefficients C(′)`9,10 can be

tested in b→ s`+`− transitions. We furthermore predict lepton-universality violations in Z′ decays,testable at the LHC.

I. INTRODUCTION

The Standard Model (SM) of electroweak interac-tions [1], based on the gauge group GSM ≡ SU(2)L ×U(1)Y , has been tested to very high accuracy over thelast decades. This has strong implications for newphysics (NP) scenarios, which are then required to in-volve a very high mass scale, a highly non-trivial fla-vor structure, or both. Recently the LHCb collaborationhas performed two measurements involving semileptonicb → s`+`− transitions which show deviations with re-spect to the SM expectations: The ratio RK = Br(B →Kµ+µ−)/Br(B → Ke+e−) has been measured with acentral value indicating a violation of lepton universal-ity at the 25% level [2], implying a 2.6σ deviation, andthe observable P ′5 obtained from the angular analysis ofB → K∗µ+µ− decays differs from the SM expectationwith 2.9σ significance [3]. Taking these measurementsat face value, they require the NP to have the followingfeatures:

(i) Sizable contributions to b→ s`+`− transitions,

(ii) lepton non-universal couplings.

Extensions of the SM gauge group by an additionalU(1)

′factor are among the possible NP scenarios that

could explain these deviations [4–10] (other NP interpre-tations have been discussed e.g. in Refs. [11–14]). SuchU(1)

′models have been popular extensions of the SM for

many years, see Ref. [15] and references therein. How-ever, the majority of the extensions considered in the

[email protected][email protected][email protected]§ [email protected]

literature are family universal in the quark (and charged-lepton) sector, and therefore do not meet condition (ii).Models with departures from family universality can giverise to large flavor changing Z ′ interactions, which arestrongly constrained by current flavor data [9, 16, 17].The conditions (i) and (ii) therefore limit considerablythe viable U(1)

′gauge symmetries.

Starting a new construction with the minimal particlecontent, i.e. the SM one without right-handed neutrinos,the only possible extension is gauging one of the combi-nations of family-specific lepton number, Lα − Lβ (withα, β = e, µ, τ and α 6= β) [18]. Since the resulting Z ′

boson couples only to leptons, these models do not meetrequirement (i) and have been discussed mostly in thecontext of neutrino phenomenology, usually consideringthe Lµ − Lτ symmetry [19]. Recent models [4, 5] cir-cumvent this problem by introducing additional fermions(vector-like quarks). This yields the required couplingsat an effective level.

In order to avoid such exotic vector-like quarks, theU(1)

′symmetry has to involve both quarks and leptons,

and should be family-dependent in order to satisfy condi-tions (i) and (ii). However, such a non-trivial flavor sym-metry in the quark sector requires the extension of thescalar sector in order to accommodate the quark massesand mixing angles [20]. It has been shown in Ref. [6] thatthis option can be realized by including an additionalcomplex scalar doublet. This model generates flavor-changing phenomena in the down-quark sector whichare related in a first approximation to the Cabibbo–Kobayashi–Maskawa (CKM) mixing matrix [21]. Flavor-changing interactions are also present in the up-quarksector of this model, but these are not related to CKMmatrix elements or quark masses.

We would like our model to have all of its fermioncouplings related exactly to elements of the CKM ma-trix. To that aim, we note that there is a class of two-Higgs-doublet models (2HDM) that achieves this, known

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2

as Branco–Grimus–Lavoura (BGL) models [22]. Thesemodels have flavor-diagonal interactions in the up-quarkand charged-lepton sectors, together with flavor-changingneutral currents (FCNCs) in the down-quark sector. Thelatter are suppressed by quark masses and/or off-diagonalCKM elements in an exact way, thereby providing an al-ternative solution to the flavor problem in 2HDMs whichdiffers radically from the hypothesis of natural flavor con-servation [23].

While in the original BGL model the flavor symme-try is global, in this work we promote it to a local one.This is achieved by charging also the leptons under thesymmetry, thereby enabling anomaly cancellation. Inthis gauged BGL framework (U(1)

′BGL), the properties

of the BGL models are transferred to the gauge bosonsector: we obtain FCNCs mediated at tree-level by theneutral scalar and massive gauge vector bosons of thetheory, all of which are suppressed by off-diagonal CKMelements and/or fermion masses, and therefore naturallysuppressed. This class of models necessarily exhibits de-viations from lepton universality due to its gauge struc-ture. Note that this form of flavor suppression in thedown-quark sector also appears in certain 3-3-1 mod-els [7]. However, in our framework this is not a choice,but a consequence of the gauge symmetry.

This paper is organized as follows: We formulate theU(1)

′BGL models in Sec. II. In Sec. III we discuss the con-

straints from flavor and collider data, testing the strongcorrelations present in these models, specifically with re-spect to the deviations observed by LHCb. We concludein Sec. IV. The appendices include technical details onanomaly cancellation and the scalar sector.

II. GAUGED BGL SYMMETRY

A characteristic feature of BGL models [22]1 is thepresence of FCNCs at tree level, which are howeversufficiently suppressed by combinations of CKM ma-trix elements. This is a consequence of specific pat-terns of Yukawa couplings, generated by correspond-ing charge assignments under a horizontal, family-non-universal (BGL-)symmetry.

The quark Yukawa sector of the model reads (i = 1, 2)

−LquarkYuk = q0

L Γi Φid0R + q0

L ∆i Φiu0R + h.c. , (1)

where Γi and ∆i denote the Yukawa coupling matri-ces for the down- and up-quark sectors, respectively,

and Φi ≡ iσ2Φ∗i , with the Pauli matrix σ2. The neu-tral components of the Higgs doublets acquire vacuumexpectation values (vevs) |〈Φ0

i 〉| = vi/√

2. Definingv ≡ (v2

1 + v22)1/2, measurements of the muon lifetime fix

1 Their extension to include neutrino masses has been discussed inRef. [24].

v = (√

2GF )−1/2 ' 246 GeV. We further define tanβ =v2/v1 and use the following abbreviations: cosβ ≡ cβ ,sinβ ≡ sβ , tanβ ≡ tβ .

Choosing an abelian symmetry under which a field ψtransforms as

ψ → eiXψ

ψ , (2)

the most general symmetry transformations in the quarksector yielding the required textures are of the form

X qL =1

2[diag (XuR, XuR, XtR) +XdR 1] ,

X uR = diag (XuR, XuR, XtR) ,

X dR = XdR 1 ,

(3)

with XuR 6= XtR. The Higgs doublets transform as

XΦ = diag (XΦ1 , XΦ2)

=1

2diag (XuR −XdR, XtR −XdR) .

(4)

There are several possible implementations of this sym-metry, related by permutations in flavor space and ex-changing up- and down-quark sectors; here, for definite-ness, the top quark has been singled out, yielding thepatterns

Γ1 =

∗ ∗ ∗∗ ∗ ∗0 0 0

, Γ2 =

0 0 00 0 0∗ ∗ ∗

,

∆1 =

∗ ∗ 0∗ ∗ 00 0 0

, ∆2 =

0 0 00 0 00 0 ∗

.

(5)

These textures give rise to FCNCs in the down-quarksector, which are however suppressed by quark massesand off-diagonal elements of the third CKM row [22].This is related to the fact that the CKM mixing ma-

trix V ≡ U†uLUdL has a direct correlation in this modelwith the elements of the third row of the rotation ofthe left-handed down quarks, i.e. (UdL)3i = V3i. Thechoice of the top quark in Eq. (3) implies a particularlystrong suppression of flavor-changing phenomena in light-quark systems. Present constraints from ∆F = 1 and∆F = 2 quark flavor transitions are accommodated evenwhen the scalars of the theory are light, with masses ofO(102) GeV [25].

While this model can be implemented through anabelian discrete symmetry, this always yields an acci-dental continuous abelian symmetry which introduces anundesired Goldstone boson into the theory [22]. Severalsolutions to this problem have already been proposed inthe literature [22, 26]; in the following we provide a newsolution, promoting the BGL symmetry to a local one.

When gauging a symmetry, special attention mustbe paid to whether it remains anomaly-free.2 BGL

2 In this work we consider only symmetries as “good” if all gauge

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3

models are automatically free of QCD anomalies, i.e.U(1)

′[SU(3)C ]2 [26]. However, we also need to fulfill the

anomaly conditions for the following combinations:

U(1)′[SU(2)L]2 , U(1)

′[U(1)Y ]2 , [U(1)

′]2U(1)Y ,

[U(1)′]3 , U(1)

′[Gravity]2 . (6)

We find that there is no solution for this system withinthe quark sector alone with the charge assignments inEq. (3). Satisfying these anomaly conditions is highlynon-trivial and requires, in general, additional fermions.However, the implementation of the BGL symmetry asa local symmetry is possible by adding only the SM lep-tonic sector when allowing for lepton-flavor non-universalcouplings. As in the SM, the cancellation of the gaugeanomalies then occurs due to a cancellation betweenquark and lepton contributions; the cancellation willhowever involve all three fermion generations, contraryto the SM gauge group, for which the anomaly cancella-tion occurs separately within each fermion generation.

Gauging the BGL symmetry therefore not only re-moves the unwanted Goldstone boson, which is “eaten”by the Z ′, but also provides a consistent Z ′ model with-out extending the particle content beyond the additionalscalars, i.e. no vector-like quarks are necessary. Theflavor structure is extended to the Z ′ couplings, yield-ing again strongly suppressed FCNCs in the down-typequark sector, while the up-type-quark couplings remaindiagonal. Especially, since the flavored gauge symmetryfixes also the charged-lepton Yukawa matrices to be diag-onal, we can obtain large deviations from lepton univer-sality without introducing lepton-flavor violation. Ourmodels provide thereby explicit examples for which thegeneral arguments given in Refs. [11, 28, 29] do not hold.

A. Lepton sector

As emphasized above, the anomaly constraints can befulfilled by assuming that leptons are also charged underthe U(1)

′symmetry. The resulting charge constraints are

given in Appendix A.For XΦ2

= 0 the mixing between the neutral mas-sive gauge bosons is suppressed for large tanβ. Withthis choice, we obtain only one possible solution to theanomaly conditions up to lepton-flavor permutations, im-plying the following charge assignments:

X dR = 1 , X uR = diag

(−7

2,−7

2, 1

),

X qL = diag

(−5

4,−5

4, 1

), X `L = diag

(9

4,

21

4,−3

),

anomalies are canceled. It would be also possible to con-sider anomalous U(1) extensions in the low-energy theory whoseanomaly graphs get canceled via the so-called Green-Schwarzmechanism [27].

X eR = diag

(9

2,

15

2,−3

), XΦ = diag

(−9

4, 0

).

(7)

We have normalized all U(1)′

charges by setting XdR =1, thereby fixing also the normalization for the gaugecoupling g′. In addition to the top, this particular modelsingles out the tau lepton as the only one coupling to Φ2.Permutations of the charges in X `L and X eR give rise to 5more models.

With the charge transformations in Eq. (7), thecharged-lepton Yukawa sector takes the form

−Lc-leptonsYuk = `0L Πi Φie

0R + h.c. , (8)

with

Π1 =

∗ 0 00 ∗ 00 0 0

, Π2 =

0 0 00 0 00 0 ∗

, (9)

while the quark Yukawa sector remains unchanged.We call to attention that no reference to the neutrino

sector has been made in the previous arguments. In thiswork we are mostly interested in the properties of thequark and charged-lepton sectors in the presence of anew gauge boson, while we leave a detailed discussion ofthe neutrino sector to future work. For a possible imple-mentation with the SM fermion content we can build thed = 5 Weinberg effective operator (`Φa)(ΦTb `

c), which af-ter spontaneous symmetry breaking induces a Majoranamass term for the neutrinos. If this effective operatoris invariant under the new flavored gauge symmetry inEq. (7), we are led to a Lµ − Lτ symmetric d = 5 ef-fective operator and, consequently, Majorana mass term.This structure has been studied in Refs. [19], and while itis not capable of fully accommodating the neutrino data,it can serve as a good starting point.

If we want to improve on this scenario while keepingour solution to the anomaly conditions, we may want amechanism that at the effective level already breaks theaccidental Lµ − Lτ symmetry. For instance, we may ex-tend the model with 3 right-handed neutrinos, where oneof them is not charged while the other two have oppositecharges. In this way the anomaly solutions remain un-changed. Choosing the charges of the right-handed neu-trinos appropriately, the Dirac mass term for the neutri-nos can be made diagonal and the Majorana mass for theright-handed ones Lµ − Lτ symmetric. Along the linesof Ref. [6], coupling an additional scalar to the right-handed neutrinos could break the accidental symmetryat the effective level.

We can also envisage other mechanisms that do changethe anomaly conditions and, therefore, introduce new so-lutions.

B. Gauge boson sector

In order to avoid experimental constraints on a Z ′ bo-son, the U(1)

′symmetry must be broken at a relatively

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4

high scale, rendering the new gauge boson significantlyheavier than the SM ones [15]. This can be achievedthrough the introduction of a complex scalar singlet S,charged under the BGL symmetry with charge XS , whichacquires a vev |〈S〉| = vS/

√2 � v. The charge of the

scalar singlet is fixed once the scalar potential is speci-fied, in our case XS = −9/8, see Appendix B for details.

As a consequence of the gauge symmetry breaking,GSM×U(1)

′ → U(1)em, the neutral massive gauge bosonsmix, giving rise to a Lagrangian of the form3

L = − 1

4AµνA

µν − 1

4ZµνZ

µν − 1

4Z ′µνZ

′µν

+1

2M2ZZµZ

µ +1

2M2Z′Z

′µZ′µ + ∆2Z ′µZ

µ

− J µAAµ − JµZ Zµ − J

µZ′Z

′µ ,

(10)

where J µA and J µZ are the SM currents of the photonand the Z, respectively. The fermionic piece of the newcurrent takes the form

J µZ′ ⊃ g′ ψiγ

µ

[(XψL)ijPL +

(XψR)ijPR

]ψj , (11)

with PL,R = (1 ∓ γ5)/2 denoting the usual chiral pro-

jectors, g′ the U(1)′

gauge coupling, and XψX the phasetransformation matrices in the fermion mass basis, i.e.

XψR = XψR , X uL = X qL , X eL = X `L , and

X dL = −5

41 +

9

4

|Vtd|2 VtsV∗td VtbV

∗td

VtdV∗ts |Vts|2 VtbV

∗ts

VtdV∗tb VtsV

∗tb |Vtb|2

.(12)

The neutral gauge boson mass and mass-mixing pa-rameters in this model are given by

M2Z =

e2v2

4s2W c

2W

,

M2Z′ = g′ 2

(v2iX

2Φi + v2

SX2S

),

∆2 = − e g′

2cW sWXΦiv

2i ,

(13)

where e =√

4πα is the electromagnetic charge and its ra-

tio with the SU(2)L coupling g defines θW ≡ arcsin (e/g),which differs from the experimentally measured weak an-gle due to mixing effects [30]: sW cW MZ = sW cWMZ ,where MZ is the physical Z mass. We rotate to thephysical eigenbasis by performing the following orthogo-nal transformation:(

ZµZ ′µ

)= O

(ZµZ ′µ

), with O =

(cξ sξ−sξ cξ

)and

3 We neglect here a possible mixing coming from the gauge ki-netic Lagrangian as the mass mixing shows already all relevantqualitative effects [15].

tan 2ξ =2∆2

M2Z − M2

Z′

. (14)

Since we assume v � vS , we obtain M2Z , ∆2 � M2

Z′ andthe resulting mixing angle is small [15]:

g′ξ ' e

2cW sW

XΦ1v2

1 +XΦ2v2

2

X2Sv

2S

' − 9e

8cW sW

(g′cβv

MZ′

)2

.

(15)

Expanding in this small parameter, we obtain the fol-lowing leading expression for the hatted weak angle interms of physical quantities

s2W ' s2

∗ ≡ s2W −

c2W s2W

c2W − s2W

ξ2

(M2Z′

M2Z

− 1

). (16)

In the physical basis the neutral gauge boson massesread

M2Z,Z′ =

1

2

[M2Z′ + M2

Z ∓√(

M2Z′ − M2

Z

)2

+ 4∆4

],

(17)

and their fermionic currents are given by

JµZ(′) ⊃ ψiγµ

[ε(′)ψL,ijPL + ε

(′)ψR,ijPR

]ψj , (18)

with the couplings (up to O(ξ2))

εψX,ij =e

cW sW

[1 +

ξ2

2

(M2Z′

M2Z

− 1

)]×[(TψX3 − s2

∗Qψ

)1 + ξ

g′cW sWe

XψX]ij

,

ε′ψX,ij =e

cW sW

[g′cW sW

eXψX − ξ

(TψX3 − s2

WQψ

)1

]ij

.

(19)

Here TψL3 is the third component of weak isospin for the

left-handed fields (TψR3 = 0) and Qψ the electric charge.We also define the vector and axial-vector combinationsof the Z(′) couplings,

ε(′)ψV,ij ≡ ε

(′)ψL,ij + ε

(′)ψR,ij , ε

(′)ψA,ij ≡ ε

(′)ψR,ij − ε

(′)ψL,ij . (20)

The coefficients εψV (A),ij encode corrections to the SM

Z couplings due to mixing with the Z ′ which are pro-portional to g′ξ at leading order in the mixing an-gle. Such corrections are restricted to be small (g′ξ .10−4) [31, 32]. In addition to our initial assumption,vS � v, which already gives a small ξ, we will assumethat the mixing angle receives an additional suppression,because tanβ is large.4 This also guarantees that flavor-changing effects mediated by the Z are negligible com-pared with those of the Z ′.

4 This limit is quite natural in our model since Φ2 is coupled to thetop quark, while Φ1 is coupled to the light first two generations.Therefore, the hierarchy v2 > v1 accommodates well the quarkmass spectrum.

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5

Another important theoretical constraint is obtainedwhen requiring the absence of a low-energy Landau pole,i.e. an energy scale ΛLP at which perturbativity is lost.This scale can be found from the renormalization-grouprunning of the U(1)

′coupling, we have:

dα′

d ln q2= b α′ 2 +O(α′ 3) , (21)

where the one-loop beta function b contains the chargeinformation of the model. It reads

b =1

2

3

∑f

X2fL,R +

1

3

(2∑i

X2Φi +X2

S

) , (22)

with f including all fermion degrees of freedom and i =1, 2. The Landau pole can be extracted from the pole ofα′(q2) = g′ 2(q2)/4π, we obtain

ΛLP 'MZ′ exp

[1

2 b α′(M2Z′)

]. (23)

For the charges in our model we have b ' 12.90, seeEq. (7). Taking MZ′ ' 4 TeV, we get a Landau pole atthe Planck scale, ΛLP

>∼ 1019 GeV, for g′ <∼ 0.12. Noticethat this bound is stronger than the naıve perturbativitybound α′(M2

Z′)<∼ O(1/max{|Xi|}2), which in our model

gives g′ <∼ 0.47. We can relax this condition by assum-ing that additional NP will appear at the see-saw or theGrand Unification scale. This way we obtain g′ <∼ 0.14for ΛLP ≥ 1014 GeV and g′ <∼ 0.13 for ΛLP ≥ 1016 GeV.The extension of the model to these scales is beyond thescope of this work.

C. Scalar sector

Here we discuss the main features of the Higgs sec-tor of the model, a detailed derivation of these results isgiven in Appendix B. It consists of two complex Higgsdoublets and a complex scalar gauge singlet. Their prop-erties are largely determined by the fact that v/vS � 1.The spectrum contains four would-be Goldstone bosonsgiving mass to the electroweak (EW) gauge vector bosons{MW ,MZ ,MZ′}, a charged Higgs H± and four neutralscalars (three CP-even {H1, H2, H3} and a CP-odd A).

We obtain a decoupling scenario with a light SM-like Higgs boson, M2

H1∼ O(v2), three heavy quasi-

degenerate states coming mainly from the scalar dou-blets M2

H2' M2

A ' M2H± ∼ O(v2

S) and another heavyCP-even Higgs coming mainly from the scalar singletM2H3∼ O(v2

S).5 The Yukawa interactions of the scalar

5 It is also possible to motivate scenarios that avoid decouplingbased on an enhanced Poincare symmetry protecting the weakscale [33]. These can give rise to a rich scalar sector at the EWscale and a pseudo-Goldstone boson in the spectrum.

bosons reflect this decoupling. They can be written as

−LY ⊃∑

ϕ=Hk,A

ϕ[dL Y

ϕd dR + uL Y

ϕu uR + `L Y

ϕ` eR

]+

√2

vH+

(uLNddR − uRN†udL + `LN`eR

)+ h.c.

(24)

Neglecting corrections of O(v2/v2S) we obtain

Y H1

f =Df

v, Y H2

f = −Nfv,

Y Au = iNuv, Y Ad,` = −iNd,`

v,

(25)

with (f = u, d, `). Here fermions have been rotated to themass eigenbasis. The diagonal matrices Df=u,d,` containthe fermion masses, and the matrices Nf are given as

(Nd)ij =v2

v1(Dd)ij −

(v2

v1+v1

v2

)(V †)i3(V )3j(Dd)jj ,

Nu =v2

v1diag(mu,mc, 0)− v1

v2diag(0, 0,mt) ,

N` =v2

v1diag(me,mµ, 0)− v1

v2diag(0, 0,mτ ) . (26)

The couplings of the scalar H3 to the fermions areadditionally suppressed, since they are generated onlythrough mixing with the doublet degrees of freedom:Y H3

f ' O(v/vS). The matrix Nd is non-diagonal in flavorspace, giving again rise to tree-level FCNCs in the down-quark sector controlled by the CKM matrix V . Further-more, as shown in Appendix B, the constraints from theU(1)

′symmetry render the scalar potential CP invariant.

CP violation in our model is therefore uniquely controlledby the CKM phase, like in the SM.6

D. Model variations

As mentioned in section II A, we have six model imple-mentations according to the different lepton flavor per-mutations of the U(1)

′charges, with identical quark and

scalar charges given in Eq. (7). These permutations areperformed in the basis where the lepton mass matrix isdiagonal and the eigenvalues are correctly ordered. Thisway each permutation corresponds to the simultaneousinterchange of the charges of both left- and right-handedleptons. It is straightforward to check that the permu-tation of just one set of charges, while satisfying theanomaly conditions as well, would give rise to a non-diagonal mass matrix and reduce to one of the six casesconsidered here after diagonalization.

6 We do not consider strong CP violation in this work.

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6

In order to present the predictions for each of thesemodels, we introduce the generic lepton charges

X1L =9

4, X2L =

21

4, X3L = −3 ,

X1R =9

2, X2R =

15

2, X3R = −3 ,

(27)

such that each implementation is labeled by (e, µ, τ) =(i, j, k). For instance, the model presented in Eq. (7) isnow labeled as (1, 2, 3).

The additional possibilities to implement the quarkand neutrino sectors have been discussed in Secs. IIand II A, respectively.

III. DISCUSSION

In this section we discuss the phenomenology of thegauged BGL models introduced in the previous section.The phenomenology of a scalar sector with a flavor struc-ture identical to the one of our model has been analyzedin Ref. [25]. Since we are assuming a decoupling scalarsector, we can naturally accommodate a SM-like Higgsat 125 GeV; the heavy scalars are not expected to yieldsizable contributions to flavor observables in general. Wetherefore focus on the phenomenological implications ofthe Z ′ boson for this class of models. In the cases wherethe constraints depend on the choice of lepton chargesin our model, we give here the most conservative boundand discuss the differences in Secs. III C and III D.

A. Low-energy constraints

Despite the large mass of several TeV, the Z ′ bo-son yields potentially significant contributions on fla-vor observables, due to its flavor-violating couplingsin the down-type quark sector. However, because ofM2W /M

2Z′ ≤ 0.1% and the CKM suppression of the flavor-

changing Z ′ couplings, these contributions can only berelevant when the corresponding SM amplitude has astrong suppression in addition to GF . This is specificallythe case for meson mixing amplitudes and electroweakpenguin processes which we will discuss below. Furtherexamples are differences of observables that are small inthe SM, for example due to lepton universality or isospinsymmetry.

The particular flavor structure of the model impliesa strong hierarchy for the size of different flavor transi-tions: |V ∗tsVtd| ∼ λ5 � |V ∗tdVtb| ∼ λ3 � |V ∗tsVtb| ∼ λ2

(where λ ' 0.226). However, since the SM amplitudesoften show a similar hierarchy, the relative size of the Z ′

contribution has to be determined on a case-by-case ba-sis. We obtain for example similar bounds from the massdifferences ∆md,s in the Bd,s systems and εK . Here weinclude exemplarily the constraint from Bs mixing, whileleaving a detailed phenomenological analysis for futurework.

Given the high experimental precision of ∆ms [34], thestrength of the corresponding constraint depends com-pletely on our capability to predict the SM value. Thelimiting factors here are our knowledge of the hadronic

quantity fBs

√Bs (for which substantial progress is ex-

pected soon, see Ref. [35]) and the relevant CKM ele-ments. Using the corresponding values from Refs. [36]and [37], respectively, we conclude that contributions to∆ms up to 20% remain possible at 95% confidence level(CL); from this we obtain the limit MZ′/g

′ & 16 TeV.Tree-level scalar contributions have been neglected, sincetheir effect cancels to a very good approximation in thedecoupling limit considered here [38].

Regarding the input for the CKM parameters, we makethe following observations in our models: (i) Charged-current tree-level processes receive negligible contribu-tions. (ii) The mixing phase in Bd,s mixing and the ratio∆ms/∆md remain SM-like. (iii) The additional directCP violation in B → ππ, ρπ, ρρ and B → J/ΨK is neg-ligible. These observations imply that in our context theglobal fits from Refs. [37, 39] remain valid to good ap-proximation.

In our models the Z ′ boson couples to muons andwill contribute to neutrino trident production (NTP),νµN → νNµ+µ−. We expect dominance of the Z ′ vec-tor current for our models. The NTP cross section nor-malized to the SM one was calculated in Refs. [4, 9, 40].Using a combination of the latest NTP cross-section mea-surements we obtain a bound on the parameter combina-tion MZ′/g

′ [41], which is however weaker than the onefrom Bs mixing.

Atomic parity violation (APV) measurements alsoplace bounds on additional neutral gauge bosons couplingto electrons and light quarks. In particular, the precisemeasurement of the 133Cs weak charge from APV exper-iments is in a reasonable agreement with the predictionof the SM and can be used to set bounds on the Z ′ bo-son of our models [42]. The bound we obtain on MZ′/g

from the latest determination of the 133Cs weak chargeis however again weaker than the limit from Bs mixing.

Further potentially strong bounds stem from electricdipole moments (EDMs) and the anomalous magneticmoment of the muon. EDMs from the scalar sector oc-cur at the two-loop level; while this alone does not renderthem necessarily sufficiently small, the additional sup-pression and cancellations in the decoupling limit implyvery small effects [25, 43]. Anomalous magnetic momentscan be present at the one loop level, but are again toosmall in 2HDMs near the decoupling limit [25, 44]. Con-cerning the new gauge boson, one-loop contributions toEDMs require different phases for left- and right-handedZ ′ couplings to quarks and/or leptons [45]; this featureis not present in our model, therefore the Z ′ contribu-tions are again at the two-loop level and sufficiently sup-pressed, given the large Z ′ mass. In the case of anoma-lous magnetic moments we have non-vanishing one-loop

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7

contributions, which for the muon read [46]

aNPµ '

m2µ

4π2

g′2

M2Z′

(1

3X2µV −

5

3X2µA

), (28)

where XµV ≡ (XµL + XµR)/2 and XµA ≡ (XµR −XµL)/2. Using the bound on MZ′/g

′ from B0s −B0

s mix-ing, we get aNP

µ < 1.3× 10−11 for all charge assignments,which is smaller than the current theory uncertainty inthe prediction of aSM

µ [31].

B. Direct searches

The obvious way to search directly for a Z ′ is via aresonance peak in the invariant-mass distribution of itsdecay products. At the LHC this experimental analysisis usually performed by the ATLAS [47] and CMS [48]collaborations for Z ′ production in the s-channel in arather model-independent way, but assuming validity ofthe narrow-width approximation (NWA), negligible con-tributions of interference with the SM [49], and flavor-universal Z ′ couplings to quarks. Under these assump-tions, the cross section for pp → Z ′X → ffX takes thesimplified form [50, 51]

σ =π

48s

[cfuwu

(s, M2

Z′)

+ cfdwd(s, M2

Z′)], (29)

where the functions wu,d are hadronic structure factorsthat encode the information of the Drell-Yan productionprocesses of the Z ′ and their QCD corrections (for a pre-cise definition of these functions we refer the reader toRef. [51]). The model-dependent part of the cross sec-tion is contained in the coefficients cu,d:

cfu ' g′ 2(X2uL +X2

uR

)Br(Z ′ → ff

),

cfd ' g′ 2 (X2

uL +X2dR

)Br(Z ′ → ff

).

(30)

While the assumptions for these expressions are not ex-actly fulfilled in our model, they are applicable when ne-glecting the small contributions proportional to the off-diagonal CKM matrix elements. The reason is that underthis approximation the Z ′ couplings to the first two gen-erations - which yield the dominant contribution to theDrell-Yan production of the Z ′ - are universal and fla-vor conserving in the quark sector, see Eqs. (7) and (12).Note that XuL ' XdL up to small corrections propor-tional to the off-diagonal CKM matrix elements that weare neglecting.7

For high values of g′ the ratio ΓZ′/MZ′ can be quitelarge, spoiling the NWA. The constraint is therefore only

7 Flavor changing Z′ couplings between the first two quark gen-erations are suppressed by |VtdV ∗ts| ∼ λ5 while violations of uni-

versality are suppressed by |Vtd|2 ∼ λ6 and |Vts|2 ∼ λ4, withλ ' 0.226.

applicable for g′ <∼ 0.2, such that ΓZ′/MZ′ does not ex-ceed 15%. However, for the mass range accessible so farsuch a large coupling is typically excluded by the con-straint RK , as will be shown below. Combined exclusionlimits on the Z ′ at 95% CL using the dimuon and dielec-tron channels have been provided by the CMS collabo-ration in the (cu, cd) plane [48]. Using these bounds to-gether with the constraint from RK , we find that a Z ′ bo-son is excluded in our models forMZ′ . 3-4 TeV, depend-ing on the lepton charge assignments, while g′ should beO(10−1). These bounds are stronger than those frommany Z ′ benchmark models, for which current LHC datatypically give a lower bound of MZ′ & 2-3 TeV [47, 48].The reason is a combination of a sizable value for g′/MZ′

required by the constraint from RK and the combinationof Z ′ couplings to fermions appearing in our model, seeEq. (30).

When the Z ′ is too heavy to be produced at a givencollider, M2

Z′ � s, indirect searches can be carriedout by looking for effects from contact interactions,i.e. effective operators generated by integrating outthe heavy Z ′. At the LHC, the corresponding expres-sions hold for MZ′ � 4.5 TeV, and limits can be ex-tracted e.g. from searches for the contact interactions(qγµPL,Rq)(¯γµPL,R`) [52]. These are presented in termsof benchmark scenarios considering a single operator witha specific chirality structure. From the 95% CL limit pro-vided in Ref. [52] for the operator (qγµPLq)(eγ

µPRe) weextract MZ′/g

′ & 22 TeV. Searches for contact interac-tions of the type (eγµPL,Re)(fγ

µPL,Rf) were performedat LEP [53]. These are sensitive to a Z ′-boson couplingto electrons assuming MZ′ � 210 GeV and the result-ing limits are again given for benchmark scenarios. Inthis case we extract MZ′/g

′ & 16 TeV from the 95% CLbound on the operator (eγαPRe)(µγαPRµ). It is impor-tant to note that the extracted bounds from contact in-teractions using benchmark scenarios do not capture thefull dynamics of our models once the Z ′ boson is inte-grated out. Interference effects due to operators withdifferent chirality structures will be relevant in general,a detailed analysis of these effects is however beyond thescope of this work. These bounds should therefore betaken as a rough guide to the sensitivity of contact inter-actions searches at LEP and the LHC to the Z ′ of ourmodels. However, in general they do not put relevantbounds as long as g′ is not too large.

C. Discriminating the different models

The constructed class of models has two important fea-tures which imply specific deviations from the SM: con-trolled FCNCs in the down-quark sector and violationsof lepton universality. Thanks to the very specific fla-vor structure, the two are strongly correlated in each ofour models. While the flavor-changing couplings are uni-versal in the models we discuss here, the lepton chargesdiffer. Correspondingly the models can be discriminated

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8

by processes involving leptons, specifically rare leptonicand semileptonic decays ofB mesons, which can test bothfeatures.

The effective Hamiltonian describing these b→ s`+`−

transitions reads

Heff = −GF√2

α

πVtbV

∗ts

∑i

(C`iO`i + C ′`i O′`i

)+Hb→sγeff ,

(31)

where

O`9 = (sγµPLb)(`γµ`

), O′`9 = (sγµPRb)

(`γµ`

),

O`10 = (sγµPLb)(`γµγ5`

), O′`10 = (sγµPRb)

(`γµγ5`

),

O`S = mb(sPRb)(¯ ) , O′`S = mb(sPLb)(¯ ) ,

O`P = mb(sPRb)(¯γ5`) , O′`P = mb(sPLb)(¯γ5`) .

(32)

The piece Hb→sγeff is the effective Hamiltonian for the ra-diative transitions including dipole operators [17]. New

physics contributions to Hb→sγeff arise in our models fromone-loop diagrams mediated by Z ′ and Higgs bosons.Both of them are very small due to the assumed massscale of several TeV [17].

At the b-quark scale, the SM contribution to the re-maining part reads CSM

9 ' −CSM10 ' 4.2 ∀ `, while all

other contributions are negligible. The chirality-flippedoperators O′9,10 receive negligible contributions also in

our models since ε′ dR,sb = 0, while all others receive con-

tributions from Z ′ or Higgs exchanges [17, 38]. The Z ′

contribution to C`9,10 is given by

CNP`9 '− πv2

αV ∗tsVtb

ε′ dL,sbε′ eV,``

M2Z′

,

CNP`10 '− πv2

αV ∗tsVtb

ε′ dL,sbε′ eA,``

M2Z′

,

(33)

where C`i ≡ CSMi +CNP`

i . In Table I we show the correla-tions between the Wilson coefficients CNP`

9,10 in our models

and provide CNPµ9 as a function of g′/MZ′ by introducing

a conveniently normalized parameter κµ9 :

CNPµ9 ≡ κµ9 × 104

(g′v

MZ′

)2

= κµ9 × 605 TeV2

(g′

MZ′

)2

.

(34)This allows the direct estimation of CNP`

9,10 in terms ofg′/MZ′ , useful for phenomenological purposes.

The CP-even Higgs H2 and the CP-odd Higgs A cangive sizable contributions to O`S and O`P , respectively.For muons we have8

CNPµS ' −CNPµ

P '−2π (tβ + t−1

β )(N`)µµ

αM2H

. (35)

8 The correlation CS = −CP was expected given the assumeddecoupling in the scalar sector [54].

Table I. Correlations among the NP contributions to the ef-fective operators O`9,10.

Model CNPµ10 /CNPµ

9 CNPe9 /CNPµ

9 CNPe10 /CNPµ

9 κµ9

(1,2,3) 3/17 9/17 3/17 −1.235

(1,3,2) 0 −9/8 −3/8 0.581

(2,1,3) 1/3 17/9 1/3 −0.654

(2,3,1) 0 −17/8 −3/8 0.581

(3,1,2) 1/3 −8/9 0 −0.654

(3,2,1) 3/17 −8/17 0 −1.235

Here we have denoted the quasi-degenerate masses of H2

and A by MH ≡MH2'MA, see Appendix B for details

of the scalar sector. The coupling (N`)µµ is again model-dependent: (N`)µµ = tβmµ for models (1, 2, 3), (2, 1, 3),

(3, 1, 2) and (3, 2, 1), while (N`)µµ = −t−1β mµ for (1, 3, 2)

and (2, 3, 1). The suppression by the muon mass rendersthese contributions negligible, apart from observables inwhich also the SM and Z ′ contributions receive this sup-pression, e.g. Bs → µ+µ−. Higgs contributions to O′`S,Pwill be additionally suppressed by a factor ms/mb com-pared to the corresponding non-primed operators and areneglected in the following.

The angular distributions of neutral-current semilep-tonic b → s`+`− transitions allow for testing these coef-ficients in global fits. Furthermore, they provide precisetests of lepton universality when considering ratios of thetype

RM ≡Br(B → Mµ+µ−)

Br(B → Me+e−)

SM= 1 +O(m2

µ/m2b) , (36)

with M ∈ {K,K∗, Xs,K0(1430), . . .} [55], where manysources of uncertainties cancel when integrating overidentical phase-space regions.

Additional sensitivity to the dynamics of NP can beobtained via double-ratios [56],

RM ≡RMRK

. (37)

It was shown in Ref. [56] that the dependence on the

NP coupling to left-handed quarks cancels out in RM .

Since C ′`9,10 = 0 in our models we have RK∗ = RXs =

RK0(1430) = 1, providing an important test of the flavorstructure of our models.

The possible hadronic final states for these ratios yieldsensitivity to different NP structures, thereby providingcomplementary information. The discriminating powerof these observables has been shown recently in Ref. [12]within the framework of leptoquark models and in moregeneral contexts in Refs. [13, 56, 57].

To analyze the deviations from flavor-universality wedefine RM ' 1+∆+Σ, where Σ is the pure contributionfrom NP and ∆ the one from the interference with the

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9

SM. These quantities are given by

∆ =2

|CSM9 |2 + |CSM

10 |2[Re{CSM

9

(CNPµ

9

)∗}+ Re

{CSM

10

(CNPµ

10

)∗}− (µ→ e)

],

Σ =

∣∣∣CNPµ9

∣∣∣2 +∣∣∣CNPµ

10

∣∣∣2∣∣CSM9

∣∣2 +∣∣CSM

10

∣∣2 − (µ→ e) ,

(38)

and are valid to a very good approximation given thepresent experimental uncertainties.

Our models also give clean predictions for the rare de-cay modes B → {K,K∗, Xs}νν [17]. Tree-level Z ′-bosoncontributions to these decays are generically expected ofthe same size as in b → s`` transitions. However, themodes with neutrino final states do not distinguish be-tween our different models, since there is no sensitivity tothe neutrino species. We obtain again a universal valuefor all ratios RνM = Br(B → Mνν)/Br(B → Mνν)|SM,due to the fact that ε′ dR,sb = 0. For the same reason theaverage of the K∗ longitudinal polarization fraction inB → K∗νν is not affected by the Z ′ exchange contribu-tion [17]. The enhancement of RνM turns out to be rel-atively small, O(10%) for g′ ∼ 0.1 and MZ′ ∼ O(TeV).The reason is again the sum over the different neutrinospecies: due to the different charges, the Z ′ contributioninterferes both constructively and destructively, leaving anet effect that is smaller than in the modes with chargedleptons.

The leptonic decays B0s,d → `+`− constitute another

sensitive probe of small NP effects. Within the SM, thesedecays arise again at the loop level and are helicity sup-pressed. Due to the leptonic final state, the theoreticalprediction of these processes is very clean. They receiveZ ′- and Higgs-mediated contributions at tree-level in ourmodel through the operators Oµ10,S,P [13],

Br(Bs → µ+µ−)

Br(Bs → µ+µ−)SM'∣∣∣1− 0.24CNPµ

10 − yµCNPµP

∣∣∣2+ |yµCNPµ

S |2 ,(39)

where yµ ' 7.7mb. For the range of model parametersrelevant here, the Z ′ contribution to Bs → µ+µ− is verysmall with respect to the SM, ∼ 1% for MZ′ ∼ 5 TeVand g′ ∼ 0.1. Larger contributions are possible due toscalar mediation for the models (1, 2, 3), (2, 1, 3), (3, 1, 2)and (3, 2, 1), given that CS ' −CP ∝ t2β in these

cases. Taking MH ∼ 10 TeV and tβ ∼ 30 for exam-ple, one obtains a suppression of Br(Bs → µ+µ−) ofabout 10% relative to the SM. In our model the ratioBr(Bd → µ+µ−)/Br(Bs → µ+µ−) remains unchangedwith respect to the SM to a very good approximation.

If a Z ′ boson is discovered during the next runs of theLHC [58], its decays to leptons can be used to discrimi-nate the models presented here. We define the ratios

µf/f ′ ≡σ(pp→ Z ′ → ff)

σ(pp→ Z ′ → f ′f ′), (40)

Table II. Model-dependent predictions for the ratio µ`/`′ .

Model µe/µ µe/τ µµ/τ

(1,2,3) 45/149 45/32 149/32

(1,3,2) 45/32 45/149 32/149

(2,1,3) 149/45 149/32 45/32

(2,3,1) 149/32 149/45 32/45

(3,1,2) 32/45 32/149 45/149

(3,2,1) 32/149 32/45 149/45

where again the dominant sources of uncertainty can-cel, rendering them particularly useful to test leptonuniversality. This possibility has also been discussed inRefs. [59]. In our models we have

µb/t 'X2bL +X2

bR

X2tL +X2

tR

, µ`/`′ 'X2`L +X2

`R

X2`′L +X2

`′R

. (41)

The first ratio is fixed in our models, µb/t ' 1, whilelarge deviations from µ`/`′ = 1 are possible. The model-specific predictions for the ratio µ`/`′ are shown in Ta-ble II. We note that there is a correlation between RKand µe/µ: an enhancement of RK (as present in models(1, 3, 2), (2, 1, 3) and (2, 3, 1)) implies an enhancementof µe/µ and the other way around. Violations of leptonuniversality can therefore be tested by complementarymeasurements of flavor observables at LHCb or Belle IIand Z ′ properties to be measured at ATLAS and CMS.

D. Interpretation of b→ s`+`− anomalies

The LHCb collaboration recently performed two mea-surements of decays with b → s`+`− transitions thatshow a tension with respect to the SM expectations.The first measurement is that of the ratio RK introducedin the last section, where LHCb measures [2] RLHCb

K =

0.745+0.090−0.074± 0.036 for q2 ∈ [1, 6] GeV2, a 2.6σ deviation

with respect to the SM prediction [55, 60, 61]. The secondmeasurement is the angular analysis of B → K∗µ+µ−

decays [3], where an excess of 2.9σ is observed for theangular observable P ′5 in the bin q2 ∈ [4, 6] GeV2,9 whichhas been constructed to reduce the influence of form fac-tor uncertainties [62].

Attributing the measurement of RK solely to NP, i.e.assuming that it will be confirmed with higher signifi-cance in the next run of the LHC and/or by additionalRM measurements, it is the first way to exclude some ofour models, since it requires sizable non-universal contri-butions with a specific sign. The flavor structure in each

9 The bin q2 ∈ [6, 8] GeV2 shows nominally a tension with identi-cal significance; however, this bin is considered less theoreticallyclean, due to the larger influence of charm resonances.

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10

of our models is fixed, so half of them cannot accom-modate RK < 1, namely (1, 3, 2), (2, 1, 3) and (2, 3, 1).This is illustrated in Fig. 1, where it is additionally seenthat a large deviation from RK = 1, as indicated by thepresent central value and 1σ interval, can actually onlybe explained in two of the remaining models. This strongimpact shows the importance of further measurements ofRM ratios.

Figure 1. Model-dependent predictions for RK as a func-tion of g′/MZ′ . The recent measurement of RK by the LHCbcollaboration is shown at 1σ and 2σ. Constraints from Bsmixing are also shown at 95% CL.

In Fig. 2 we show the constraints from the RK mea-surement for the remaining models (1, 2, 3), (3, 1, 2) and(3, 2, 1). The allowed regions are consistent with the con-straint from B0

s -meson mixing. LHC searches for a Z ′

boson exclude values of MZ′ below 3-4 TeV, as discussedin Sec. III B; the corresponding areas are shown in gray.We also show the theoretical perturbativity bounds ob-tained from the requirement that the Landau pole forthe U(1)

′gauge coupling appears beyond the see-saw or

the Grand Unification scales, i.e. ΛLP > 1014 GeV andΛLP > 1016 GeV, respectively.

Regarding the angular analysis in B → K∗µ+µ−, thesituation is more complicated. The wealth of informa-tion provided in this and related measurements requiresa global analysis, which is beyond the scope of this work.However, a number of model-independent studies havebeen carried out [8, 63–67]. These analyses differ in termsof the statistical methods used, treatment of hadronicuncertainties (see also Ref. [68]), and consequently in thesignificance they find for the NP hypothesis over the SM

one. However, they agree that a contribution CNPµ9 ∼ −1

can fit the data for P ′5 without conflicting with other ob-

servables. Additional contributions from e.g. CNPµ10 can

Table III. Model-dependent bound on CNPµ9 from the RK mea-

surement. The constraint from Bs mixing is taken into ac-count.

Model CNPµ9 (1σ) CNPµ

9 (2σ)(1,2,3) – [−2.92,−0.61]

(3,1,2) [−0.93,−0.43] [−1.16,−0.17]

(3,2,1) [−1.20,−0.53] [−1.54,−0.20]

be present, but are less significant and tend to be smaller.When using Table I to translate the RK measurement

into a bound on CNPµ9 in our models, see Table III, the

ranges are perfectly compatible with the values obtainedfrom P ′5, as also observed for other Z ′ models [8, 64, 67].This is highly non-trivial given the strong correlations inour models and will allow for decisive tests with addi-tional data.

Let us further comment on the implications of the re-cent measurements of B0

d,s → µ+µ− decays [69],

Br(Bs → µ+µ−)exp

Br(Bs → µ+µ−)SM= 0.76+0.20

−0.18 ,

Br(Bd → µ+µ−)exp

Br(Bd → µ+µ−)SM= 3.7+1.6

−1.4 .

(42)

Both results seem to hint at a deviation from the SM,however in opposite directions. A confirmation of this sit-uation with higher significance would rule out our modelswhich predict these ratios to be equal; however, the un-certainties in the Bd mode are still large. Regarding theBs mode, which is measured consistent with the SM pre-diction, it should be noted that the result depends sen-sitively on the value adopted for |Vcb|, where the valuefrom inclusive B → Xc`ν decays was chosen in the SMcalculation [70]. In any case, as discussed in Sec. III C,a potential shift could be explained in the context of ourmodels by scalar contributions, which are, however, notdirectly related to the Z ′ contributions discussed above.

The models that accommodate the b → s`+`− datacan be further discriminated using the observables de-scribed in the last section, notably using the ratios µ`/`′ ,provided a Z ′ boson is discovered at the LHC.

IV. CONCLUSIONS

The class of family-non-universal Z ′ models presentedin this article exhibits FCNCs at tree level that are inaccordance with available flavor constraints while stillinducing potentially sizable effects in various processes,testable at existing and future colliders. This is achievedby gauging the specific (BGL-)symmetry structure, in-troduced in Ref. [22] for the first time, which renders theresulting models highly predictive.

The particle content of the models is minimal in thesense that the extension of the U(1)

′symmetry to the lep-

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Figure 2. Regions allowed at 1σ and 2σ by the RK measurement in the {MZ′ , g′} plane for the models (1, 2, 3), (3, 1, 2) and

(3, 2, 1). Exclusion limits from Z′ searches at the LHC are shown in gray. The black lines indicate bounds from perturbativityof g′.

ton sector allows to restrict the fermion content to theSM one. The only additional particles are then a secondHiggs doublet, a scalar singlet and the Z ′ boson, all ofwhich are heavy after spontaneous symmetry breaking,due to the large mass scale for the singlet. The anomalyconditions largely determine the charge assignments un-der the U(1)

′symmetry; the remaining freedom is used

for two phenomenologically motivated choices, leavingonly six possible models which are related by permuta-tions in the lepton sector.

The main phenomenological features of these modelscan be summarized as follows:

1. FCNCs at tree level in the down-quark sector,which are mediated by heavy Z ′ gauge bosons andneutral scalars, controlled by combinations of CKMmatrix elements and/or fermion mass factors.

2. Non-universal lepton couplings determined by thecharges under the additional U(1)

′symmetry.

3. No FCNCs in the charged-lepton or up-quark sec-tors.

4. Complete determination of the U(1)′

sector up totwo real parameters, MZ′ and g′, where all observ-ables at the electroweak scale and below dependonly on the combination g′/MZ′ .

Present data already strongly restrict the possible pa-rameter ranges in our models: direct searches excludeZ ′ masses below 3 − 4 TeV and the constraint from Bmixing implies MZ′/g

′ ≥ 16 TeV (95% CL). Theoreticalbounds from perturbativity give an upper bound on thevalue of the gauge coupling, e.g. g′ <∼ 0.14 for a Landaupole beyond the see-saw scale. Nevertheless, three of ourmodels can explain the deviations from SM expectationsin b → s`+`− transitions seen in LHCb measurements[2, 3], while the other three are excluded (at 95% CL) byRK < 1. These findings are illustrated in Figs. 1 and 2.

Any significant deviation from the SM in an observablewith Z ′ contributions allows for predicting all other ob-servables, for instance the values for CNP`

9,10 obtained fromRK , see Tables I and III. Further characteristic predic-tions in our models include the following:

• The absence of flavor-changing Z ′ couplings to

right-handed quarks implies RM = 1, i.e. all ra-tios defined in Eq. (36) are expected to be equal,RK = RK∗ = RXs = . . . The same holds for theratios RνM in B →Mνν decays.

• If a Z ′ is discovered at the LHC, measurements ofσ(pp → Z ′ → `i ¯i)/σ(pp → Z ′ → `j ¯

j) can beused to discriminate between our models, due tothe specific patterns of lepton-non-universality, seeTable II.

• Leptonic down-quark FCNC decays are sensitiveto the Higgs couplings in our model, specificallyBd,s → `+`−. Double ratios of Bs and Bd decaysare again expected to equal unity.

In the near future we will therefore be able to dif-ferentiate our new class of models from other Z ′ mod-els as well as its different realizations from each other.This will be possible due to a combination of directsearches/measurements at the LHC and high-precisionmeasurements at low energies, e.g. from Belle II andLHCb. Further progress can come directly from theory,e.g. by more precise predictions for ∆md,s or εK .

As a final remark, we recall that in this minimal imple-mentation of gauged BGL symmetry neutrinos are mass-less. Additional mechanisms to explain neutrinos massescan introduce new solutions to the anomaly equations;these new variants are subject to future work.

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ACKNOWLEDGMENTS

The work of A.C. is supported by the Alexander vonHumboldt Foundation. The work of J.F. has been sup-ported in part by the Spanish Government and ERDFfrom the EU Commission [Grants No. FPA2011-23778,FPA2014-53631-C2-1-P, No. CSD2007-00042 (ConsoliderProject CPAN)]. J.F. also acknowledges VLC-CAMPUSfor an “Atraccio del Talent” scholarship. The work ofM.J. was financially supported by the ERC AdvancedGrant project “FLAVOUR” (267104) and the DFG clus-ter of excellence “Origin and Structure of the Universe”.H.S.’s work was supported by the National ResearchFoundation of Korea (NRF) grant funded by the Ko-rea government (MEST) (No. 2012R1A2A2A01045722).A.C. is grateful to A. Vicente and J. Virto for discussionsabout the b→ s`+`− anomalies.

Appendix A: Anomaly cancellation conditions

In this appendix we present the restrictions on thecharges derived from the requisite gauge anomaly can-cellation for quarks transforming according to Eq. (3)and allowing the leptons to transform in the most gen-eral way:

X `L = diag (XeL, XµL, XτL) ,

X eR = diag (XeR, XµR, XτR) .(A1)

As mentioned in Sec. II, the QCD anomaly condition isautomatically satisfied within BGL models. On the otherhand, the anomaly conditions involving a single U(1)

gauge boson together with SU(2)L or U(1)Y ones, and the

mixed gravitational-U(1)′

anomaly are non-trivial andread

A221′ = 3XuR +3

2XtR +

9

2XdR +

∑α=e,µ,τ

XαL ,

A111′ = − 5

2XuR −

5

4XtR −

3

4XdR

+∑

α=e,µ,τ

(1

2XαL −XαR

),

AGG1′ =∑

α=e,µ,τ

(2XαL −XαR) .

(A2)

The triangle diagrams involving two or three U(1)′gauge

bosons result in more complicated conditions for the BGLcharges, which include a quadratic and a cubic equation:

A11′1′ = − 7

2X2uR −

7

4X2tR +

15

4X2dR +XuRXdR

+1

2XtRXdR −

∑α=e,µ,τ

(X2αL −X2

αR

),

A1′1′1′ = − 9

4

[2X3

uR +X3tR + 3X3

dR

−XdR

(2X2

uR +X2tR

)−X2

dR (2XuR +XtR)]

+∑

α=e,µ,τ

(2X3

αL −X3αR

). (A3)

Satisfying these conditions with rational charges is non-trivial and there is only one class of solutions giving ananomaly-free model, up to lepton flavor permutations:

XuR = −XdR −1

3XµR , XtR = −4XdR +

2

3XµR ,

XeL = XdR +1

6XµR , XµL = −XdR +

5

6XµR ,

XτL =9

2XdR −XµR ,

XeR = 2XdR +1

3XµR , XτR = 7XdR −

4

3XµR .

(A4)

At this point we have two free charges in the above rela-tions, i.e. XdR and XµR. Using XΦ2 = 0, as discussedin Sec. II, yields one relation between the two charges.The remaining free charge, e.g. XdR, is fixed by somenormalization convention.

Appendix B: Scalar potential

The Higgs doublets are parametrized as

Φi =

(Φ+i

Φ0i

)= eiθi

(ϕ+i

1√2

(vi + ρi + iηi)

)(i = 1, 2) .

(B1)Their neutral components acquire vevs given by 〈Φ0

j 〉 =

eiθjvj/√

2 with vi > 0 and (v21 + v2

2)1/2 ≡ v. In fullgenerality we can rotate away the phase of Φ1, leavingthe second doublet with the phase θ = θ2 − θ1. Weparametrize the complex scalar singlet as

S = e−iαS/2(vS +R0 + iI0)√

2, (B2)

with vS > 0.Since we have in our model three scalar fields,{Φ1,Φ2, S}, the phase-blind part of the scalar potential

has a U(1)3

global invariance. In order to avoid masslessGoldstone bosons, we need to charge the S field in sucha way that the phase-sensitive part breaks this symme-try down to U(1)

2= U(1)Y × U(1)

′. Gauge-invariant

combinations can be built only from Φ†1Φ2 and S, leav-

ing us with the possibilities Φ†1Φ2S, Φ†1Φ2S2 and com-

binations involving complex conjugates. For concrete-

ness we choose Φ†1Φ2S2 to be invariant, which imposes

XS = −9/8. The scalar potential then reads

V =m2i |Φi|2 +

λi2|Φi|4 + λ3|Φ1|2|Φ2|2

+ λ4|Φ†1Φ2|2 +b22|S|2 +

d2

4|S|4 +

δi2|Φi|2|S|2

− δ34

(Φ†1Φ2S

2 + Φ†2Φ1(S∗)2).

(B3)

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All the parameters of the scalar potential but δ3 are realdue to hermiticity. The parameter δ3 has been chosento be real and positive by rephasing the scalar field Sappropriately.

The vacuum expectation value of the potential is givenby

V0 =v4

16

[8m2

1

v2c2β + 2λ1c

4β + 4s2

β

(2m2

2

v2+ (λ3 + λ4)c2β

)+ 2λ2s

4β + 2v2

(2b2v2

+ δ1c2β + δ2s

)+ d2v

4

− 2 δ3 cβsβ v2 cos(αS − θ)

]. (B4)

Here we have defined the ratio v = vS/v. The stabilityof the vacuum requires that

0 =∂V0

∂θ= −δ3v

2v2S

16s2β sin(αS − θ) . (B5)

By convention we choose αS = θ, the other possibili-ties in αS = θ mod 2π simply amount to an unphysicalrephasing of the scalar field S. Stability also requires∂V0/∂vi = 0, to which the only non-trivial solution reads

b2 =v2

2

[−δ1c2β + δ3cβsβ − δ2s2

β − d2v2],

m21 =

v2

8

[−4 (λ3 + λ4) s2

β − 4λ1c2β + δ3tβ v

2 − 2δ1v2],

m22 =

v2

8

[−4 (λ3 + λ4) c2β − 4λ2s

2β + δ3t

−1β v2 − 2δ2v

2].

(B6)

The scalar potential is then determined in terms of 10unknown parameters {vS , β, λ1−4, d2, δ1−3}, since θ = αSdoes not appear explicitly.

The masses of the physical CP-odd boson A and thecharged scalar are given by

M2A =

δ3 v2S

4

(s−1

2β +s2β

v2

)' δ3 v

2S

4s2β,

M2H± =

v2S

4

(δ3s2β− 2λ4

v2

)' δ3v

2S

4s2β,

(B7)

respectively. The physical states H1,2,3 are expressed interms of {ρ1, ρ2, R0} via an orthogonal transformation,H1

H2

H3

= RS

ρ1

ρ2

R0

. (B8)

The mass matrix for the CP-even bosons can be diago-nalized analytically in a perturbative expansion around

1/v � 1. Including the leading corrections in 1/v oneobtains

RS '

cβ sβ ω13

−sβ cβ ω23

ω23sβ − ω13cβ −(ω23cβ + ω13sβ) 1

,

(B9)with

ω13 = −2δ1c

2β − δ3s2β + 2δ2s

2vd2,

ω23 =δ3s4β + 2(δ1 − δ2)s2

2v(2d2s2β − δ3).

(B10)

The resulting masses for the CP-even scalars are givenby

M2H1' λv2

2d2, M2

H2' δ3v

2S

4s2β, M2

H3' d2v

2S

2, (B11)

with

λ = (2d2λ1 − δ21)c4β + (δ1c

2β + δ2s

2β)δ3s2β

− 2δ1δ2 + δ23

4s2

2β − (δ22 − 2d2λ2)s4

β

+ d2(λ3 + λ4)s22β .

(B12)

The exact expression for their Yukawa couplings inEq. (24) is

v Y Hkf = [cβ(RS)k1 + sβ(RS)k2]Df

+ [sβ(RS)k1 − cβ(RS)k2]Nf .(B13)

Finally, the vacuum solution in our models allow forcomplex vevs but that is not sufficient to have sponta-neous CP violation. In the weak gauge sector CP viola-tion is manifest through the invariant Tr [Hd, Hu]

3[71].

In the CP-invariant scenario, i.e. with real Yukawa ma-trices, the Hermitian combinations Hu,d are given by

2Hu = v21∆1∆T

1 + v22∆2∆T

2 + v1v2(∆1∆T2 + ∆2∆T

1 )cθ

+ iv1v2(∆1∆T2 −∆2∆T

1 )sθ ,

2Hd = v21Γ1ΓT1 + v2

2Γ2ΓT2 + v1v2(Γ2ΓT1 + Γ1ΓT2 )cθ

+ iv1v2(Γ2ΓT1 − Γ1ΓT2 )sθ .

(B14)

In our model we get Tr [Hd, Hu]3

= 0, implying the ab-sence of CP violation in the gauge interactions when theonly phase is carried by the scalar vev. As a consequence,the source of CP violation for the weak currents in ourmodel is present in the Yukawa couplings and will appearin the observables through the CKM mechanism.

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