PHYSICAL REVIEW D 100, 075033 (2019)
Accessible lepton-number-violating models and negligible neutrino masses
† ‡ Andr´e de Gouvêa ,1,* Wei-Chih Huang,2, Johannes König,2, and Manibrata Sen 1,3,§ 1Northwestern University, Department of Physics and Astronomy, 2145 Sheridan Road, Evanston, Illinois 60208, USA 2CP3-Origins, University of Southern Denmark, Campusvej 55, DK-5230 Odense M, Denmark 3Department of Physics, University of California Berkeley, Berkeley, California 94720, USA
(Received 18 July 2019; published 25 October 2019)
Lepton-number violation (LNV), in general, implies nonzero Majorana masses for the Standard Model neutrinos. Since neutrino masses are very small, for generic candidate models of the physics responsible for LNV, the rates for almost all experimentally accessible LNV observables—except for neutrinoless double- beta decay—are expected to be exceedingly small. Guided by effective-operator considerations of LNV phenomena, we identify a complete family of models where lepton number is violated but the generated Majorana neutrino masses are tiny, even if the new-physics scale is below 1 TeV. We explore the phenomenology of these models, including charged-lepton flavor-violating phenomena and baryon- number-violating phenomena, identifying scenarios where the allowed rates for μ− → eþ-conversion in nuclei are potentially accessible to next-generation experiments.
DOI: 10.1103/PhysRevD.100.075033
I. INTRODUCTION Experimentally, in spite of ambitious ongoing experi- Lepton number and baryon number are, at the classical mental efforts, there is no evidence for the violation of level, accidental global symmetries of the renormalizable lepton-number or baryon-number conservation [5]. There Standard Model (SM) Lagrangian.1 If one allows for are a few different potential explanations for these (neg- generic nonrenormalizable operators consistent with the ative) experimental results, assuming degrees-of-freedom SM gauge symmetries and particle content, lepton number beyond those of the SM exist. Perhaps the new particles are and baryon number will no longer be conserved. Indeed, either very heavy or very weakly coupled in such a way that lepton-number conservation is violated by effective oper- phenomena that violate lepton-number or baryon-number ators of dimension five or higher while baryon-number conservation are highly suppressed. Another possibility is conservation (sometimes together with lepton number) is that the new interactions are not generic and that lepton- violated by effective operators of dimension six or higher. number or baryon-number conservation are global sym- In other words, generically, the addition of new degrees-of- metries of the beyond-the-Standard-Model Lagrangian. freedom to the SM particle content violates baryon-number Finally, it is possible that even though baryon number or and lepton-number conservation. lepton number are not conserved and the new degrees-of- freedom are neither weakly coupled nor very heavy, only a subset of baryon-number-violating or lepton-number- violating phenomena are within reach of particle physics *[email protected] † experiments. This manuscript concentrates on this third [email protected] ‡ option, which we hope to elucidate below. [email protected] §[email protected] The discovery of nonzero yet tiny neutrino masses is 1At the quantum level these symmetries are anomalous, i.e., often interpreted as enticing—but certainly not definitive— they are violated by nonperturbative effects [1,2]. These are only indirect evidence for lepton-number-violating new physics. relevant in extraordinary circumstances (e.g., very high temper- In this case, neutrinos are massive Majorana fermions and atures) much beyond the reach of particle physics experiments one can naturally “explain” why the masses of neutrinos [3,4]. Nonperturbative effects still preserve baryon-number- minus-lepton number, the nonanomalous possible global sym- are much smaller than those of all other known massive metry of the renormalizable SM Lagrangian. particles (see, e.g., [6–8] for discussions of this point). Searches for the nature of the neutrino—Majorana fermion Published by the American Physical Society under the terms of versus Dirac fermion—are most often searches for lepton the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to number violation (LNV). The observation of LNV implies, the author(s) and the published article’s title, journal citation, generically, that neutrinos are Majorana fermions [9], and DOI. Funded by SCOAP3. while Majorana neutrino masses imply nonzero rates for
2470-0010=2019=100(7)=075033(21) 075033-1 Published by the American Physical Society DE GOUVÊA, HUANG, KÖNIG, and SEN PHYS. REV. D 100, 075033 (2019)
Al −14 lepton-number-violating phenomena. The most powerful ∶ − þ ≳ 10 ð Þ COMET Phase-I Rμ e : 1:3 probes of LNV are searches for neutrinoless double-beta decay (0νββ, see [10] for a review); several of these are For a recent, more detailed discussion, see [20]. ongoing, e.g., [11–13]. The growing excitement behind There are several recent phenomenological attempts at searches for 0νββ is the fact that these are sensitive enough understanding whether there are models consistent with to detect LNV mediated by light Majorana neutrino current experimental constraints where the rate for exchange if the neutrino masses are above a fraction on μ− → eþ-conversion in nuclei is sizable [19,21,22]. The an electronvolt. In many models that lead to Majorana main challenges are two-fold. On the one hand, the light- neutrino masses, including, arguably, the simplest, most Majorana-neutrino exchange contribution to μ− → eþ- elegant, and best motivated ones, LNV phenomena are conversion in nuclei is tiny. On the other hand, while it predominantly mediated by light Majorana neutrino is possible to consider other LNV effects that are not exchange. Hence, we are approaching sensitivities to captured by light-Majorana-neutrino exchange, most of 0νββ capable of providing nontrivial, robust information these scenarios lead, once the new degrees of freedom are on the nature of the neutrino. integrated out, to Majorana neutrino masses that are way Other searches for LNV are, in general, not as sensitive too large and safely excluded by existing neutrino data. 0νββ as those for . Here, we will highlight searches for In [19], an effective operator approach, introduced and μ− → eþ-conversion in nuclei, for a couple of reasons. One – − þ exploited in, e.g,, [23 26], was employed to both diagnose is that, except for searches for 0νββ, searches for μ → e - the problem and identify potentially interesting directions conversion in nuclei are, arguably, the most sensitive to for model building. generic LNV new physics.2 Second, several different − − New-physics scenarios that violate lepton-number con- experiments aimed at searching for μ → e -conversion servation at the tree level in a way that LNV low-energy in nuclei are under construction, including the COMET phenomena are captured by the “all-singlets” dimension- [15] and DeeMe experiments [16] in J-PARC, and the nine operator: Mu2e experiment [17] in Fermilab. These efforts are expected to increase the sensitivity to μ− → e−-conversion 1 L ⊃ O ; where O ¼ ecμcucucdc dc; ð1:4Þ by, ultimately, four orders of magnitude and may also be Λ5 s s able to extend the sensitivity to μ− → eþ-conversion in nuclei by at least a few orders of magnitude. and Λ is the effective scale of the operator, were flagged as − þ The best bounds on the μ → e -conversion rate relative very “inefficient” when it comes to generating neutrino − to the capture rate of a μ on titanium were obtained by the Majorana masses. According to [19], the contribution SINDRUM II experiment [18] over twenty years ago: to Majorana neutrino masses from the physics that leads to Eq. (1.4) at the tree level saturates the upper bound on Γðμ− þ Ti → eþ þ CaÞ neutrino masses for Λ ∼ 1 GeV. This means that, for Ti ≡ Rμ−eþ − Λ ≫ 1 Γðμ þ Ti → νμ þ ScÞ GeV, the physics responsible for Eq. (1.4) will lead to neutrino masses that are too small to be significant 1.7 × 10−12 ðGS; 90% CLÞ < ; ð1:1Þ while the rates of other LNV phenomena, including 3.6 × 10−11 ðGDR; 90% CLÞ μ− → eþ-conversion in nuclei, may be within reach of next-generation experiments. According to [19], this where GS considers scattering off titanium to the ground happens for Λ ≲ 100 GeV. state of calcium, whereas GDR considers the transition to The effective operator approach from [23–26] is mostly a giant dipole resonance (GDR) state. Next-generation powerless when it comes to addressing lepton-number- experiments like Mu2e, DeeMe, and COMET have the conserving, low-energy effects of the same physics that potential to be much more sensitive to μ− → eþ-conversion. leads to Eq. (1.4). One way to understand this is to The authors of [19] naively estimated the future sensitivities appreciate that lepton-number-conserving phenomena are of these experiments to be captured by qualitatively different effective operators and, in general, it is not possible to relate different “types” of Al −16 operators in a model-independent way. Concrete results can Mu2e∶ R − þ ≳ 10 ; ð1:2Þ μ e only be obtained for ultraviolet (UV)-complete scenarios. In this manuscript, we systematically identify all possible UV-completemodels that are predominantly captured, when O 2 it comes to LNV phenomena, by s at the tree level. All It was recently pointed out that searches for nonstandard these models are expected to have one thing in common: neutrino interactions from long-baseline neutrino experiments are also sensitive to certain LNV new physics and involve all lepton potentially large contributions to LNV processes combined flavors [14]. In some cases, the resulting limits are stronger than with insignificant contributions to the light neutrino masses. those from μ− → eþ-conversion. Such models are expected to manifest themselves most
075033-2 ACCESSIBLE LEPTON-NUMBER-VIOLATING MODELS AND … PHYS. REV. D 100, 075033 (2019) efficiently in LNV phenomena like μ− → eþ-conversion in These different contractions, however, lead to estimates nuclei, lepton-number-conserving phenomena, including for the rates of the processes of interest which are roughly charged-lepton flavor-violating (CLFV) observables, or the same. baryon-number-violating phenomena, including neutron– An effective operator of mass dimension d is suppressed antineutron oscillations. Furthermore, if the rates for by (d − 4) powers of the effective mass-scale Λ of the new μ− → eþ-conversion in nuclei are indeed close to being physics, i.e., accessible, we find that all tree-level realizations of Os g require the existence of new degrees-of-freedom with L ⊃ Od þ H:c:; ð2:1Þ masses that are within reach of TeV-scale colliders like Λd−4 the LHC. The following sections are organized as follows. where gs are dimensionless coupling constants. Note that g Λ In Sec. II, we study the all-singlets effective operator and and are not independently defined; one can resolve this Λ illustrate its contributions to neutrino masses, 0νββ, and issue, e.g., by defining such that the largest g is one. The − þ Λ μ → e -conversion in nuclei. In Sec. III, we list the effective scale indicates the maximum laboratory energy different UV-complete models that are associated to the beyond which the effective-operator description breaks all-singlets effective operator at tree level. We discuss down, i.e., the effective-theory description is valid at energy Λ various bounds arising from searches for baryon-number- scales which are at most of order . violating and CLFV processes. In Sec. IV, we comment on With this arsenal, the dimension-nine all-singlets oper- some salient collider signatures of the different new particles ators are proposed in this work. Finally, in Sec. VI, we briefly αβ c c c c c c comment on possible extensions of these scenarios which Os ¼ lαlβu u d d ð2:2Þ can account for the observed neutrino masses, summarize c c c c our results, and conclude. where lα ≡ e , μ or τ . Os are formed from all the ð2Þ SU L-singlet fields. If all quarks are of the same II. THE EFFECTIVE ALL-SINGLETS generation, there is only one independent Lorentz con- αβ c σ c c ρ c c c σ_ OPERATOR Os traction: ðlαÞ ðlβÞσðu Þ ðu Þρðd Þσ_ ðd Þ , where σ, ρ and σ_ are the Lorentz indices; all other possible contractions are In the context of particle physics phenomenology, differ- related to this via Fierz transformations.3 ent notations are prevalent in the literature. Before pro- Oαβ ceeding, we outline the notation used in this paper, which At different loop-orders, s will contribute to Majorana follows that in [24,25]. The SM is constructed using only neutrino masses as well as different LNV processes. In what follows, we estimate in some detail the contributions left-chiral Weyl fields: Q ≡ ðuL;dLÞ, L ≡ ðνL;lLÞ are the ð2Þ c c lc of these operators to Majorana neutrino masses, 0νββ left-chiral SU L doublets, while u , d and are the left- ð2Þ and μ− → eþ-conversion in nuclei. The idea [24] is to chiral SU L singlet fields. The corresponding Hermitian- conjugated fields are identified with a bar (e.g., L;¯ ec). start with the effective operator, and add SM interactions to generate the relevant processes. The results presented in Thus, unbarred fields Lσ correspond to the ð1=2; 0Þ representation of the Lorentz algebra, while barred fields this section agree with those in [19]. ¯ † Neutrino Majorana masses are generated by the LNV Lσ_ ≡ Lσ transform under the ð0; 1=2Þ representation of the Weinberg operator [27], algebra. In this terminology, the familiar four-component Dirac spinor consisting of the electron and the positron can fαβ ¼ð cÞT L ⊃ ð α Þð β Þ ð Þ be written as e eL; e . Throughout, color indices are Λ L H L H : 2:3 implicit and hence omitted. Also, the SM Higgs doublet is W taken to be H ≡ ðHþ;H0ÞT, where H0 acquires a vacuum ð2Þ ð1Þ These are dimension-five operators, violate lepton number expectation value (vev) v to break the SU L ×U Y ð1Þ by two units, and, after electroweak symmetry breaking, gauge-symmetry spontaneously to U EM. α β L ⊃ mαβν ν Gauge singlets can be formed by either contracting the lead to neutrino Majorana mass terms, , m ¼ fv2=Λ . Λ is the effective scale of the Weinberg SUð2Þ indices using the antisymmetric tensor ϵij or the W W L operator, related to but not the same as Λ, the effective scale Kronecker δij (for conjugated fields). Additionally, flavor couplings are, unless explicitly shown, implicitly con- tracted. The flavor structure of the effective operators 3If we consider up-type and down-type quarks of different gene- can be used to infer contributions to different new-physics rations, there are two independent contractions. One can choose c c c c c c c c c μ c c c those to be ðe μ Þðu t Þðd b Þ and ðe u Þðμ σ d Þðt σμb Þ, processes, as we shall see. We also do not explicitly c where, for convenience, we fix the two different lα to be the show the Lorentz structure of the different operators. electron and the muon and the two different generations of quarks Note that, for the same operator, there can be different to be the first and third generations. All other contractions can be contractions associated with the gauge and Lorentz indices. expressed as combinations of these two.
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Neutrino oscillation data constrain only the neutrino mass-squared differences. Nonetheless, one can use the atmospheric and the solar mass-squared differences to set lower bounds on the masses of the heaviest and the next-to- heaviest neutrinos. The atmospheric mass-squared differ- ence, for example,p dictatesffiffiffiffiffiffiffiffiffiffiffiffiffiffi that at least one neutrino has 2 to be heavier than jΔm32j ≃ 0.05 eV [28]. On the other FIG. 1. Four-loop contribution to Majorana neutrino masses hand, cosmic surveys limit the sum of masses of the Oee from the dimension-nine all-singlets operator s . Given the neutrinos to be ≲0.12 eV [29–31]. For concreteness, we large loop suppression, the contribution to neutrino masses is assume that the largest element of the neutrino mass matrix only relevant for very low effective scales. The blob represents lies between mν ∈ ð0.05 − 0.5Þ eV. In this case, Eq. (2.4) the effective operator while the × represents the Higgs-boson Oαβ vacuum expectation value. implies that the effective scale of s [19] is
αβ Λ ∈ ð100 MeV − 1 GeVÞ: ð2:5Þ of Os . Experimental information on neutrino masses point 14 to ΛW ∼ 10 GeV. Starting from the all-singlets operator, Fig. 1 illustrates how the Weinberg operator is obtained Figure 2 depicts the tree-level, two-loop and four-loop 0νββ Oee at the four-loop level. In Fig. 1, the blob represents the contributions to from s . The half-life for such a ee ee decay is estimated as [19] effective operator Os , for concreteness. Clearly, since Os involves only SUð2Þ -singlet fields, neutrino masses L ð2Þ Λ2 4 1 2 2 2 2 2 2 require six Yukawa insertions so one can “reach” the ln GF yt ybyev T0νββ ¼ pffiffiffi L jg j2 Q11 2 q2 ð16π2Þ4 corresponding lepton-doublets and the Higgs-doublet ee H. The contribution to the neutrino mass matrix can be 2 1 2 1 −1 þ pGFffiffiffi ytybyev þ ð Þ estimated as 2 2 2 2 8 : 2:6 2 q ð16π Þ Λ Λ 2 gαβ yαyβðy y vÞ ¼ t b ð Þ The effective Q-value of the decay process can be extracted mαβ 2 4 ; 2:4 Λ ð16π Þ from analyses of the data from the KamLAND-Zen experi- ment [32] and turns out to be Oð10 MeVÞ. The factor of where y are the different charged-lepton and quark Yukawa ð1=q2Þ comes from the neutrino propagator and is typically of couplings, Λ and g are the effective scale and couplings of order 100 MeV,the inverse distance-scale between nucleons. αβ Os , respectively, and we assumed third-generation quarks, Combining these, our estimate for the half-life as a function of as these are associated to the largest Yukawa couplings. Λ is depicted in the left panel of Fig. 3.ForOð1Þ couplings, Note that the α, β indices in Eq. (2.4) are not summed over. the current lifetime lower-bound—Λ ≳ 5 TeV—and the
ee FIG. 2. Feynman diagrams contributing to 0νββ from the dimension-nine all-singlets operator Os at the tree level (left), two-loop level (middle), and four-loop level (right). The blob represents the effective operator while the × represents the Higgs-boson vacuum expectation value.
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FIG. 3. Left: The lifetime associated to 0νββ, T0νββ, as a function of the cutoff scale Λ, from the dimension-nine all-singlets operator ee 4 10 Os . For values Λ ≲ 10 TeV the lifetime is dominated by the tree-level contribution and scales like ∝ Λ , whereas for larger values of Λ, the lifetime is dominated by the four-loop contribution and scales ∝ Λ2. The current experimental bound from KamLAND-Zen is depicted as a horizontal black line. Right: The normalized rate Rμ−eþ of muon to positron conversion as a function of the cutoff scale Λ, μe 2 from the dimension-nine all-singlets operator Os . For scales Λ ≲ 10 TeV, the tree-level contribution dominates and the rate scales like ∝ Λ−10. For scales Λ ≳ 104 TeV the four-loop contribution is most relevant and the rate scales like ∝ Λ−2. Between those regions, the two-loop contribution is most important and the rate scale like ∝ Λ−6. The current experimental bound from SINDRUM II and the sensitivity of Mu2e are depicted as a horizontal black and purple lines, respectively.
— — 2 3 neutrino mass requirements Eq. (2.5) are incompatible. GF Z 2 Γ − ∝ pffiffiffi eff ð Þ μ 3 Q ; 2:7 This strongly suggests that if there is new physics that 2 πða0m =mμÞ ee e manifests itself via Os at the tree level, this new physics is not responsible for generating the observed nonzero neutrino masses. where Zeff is the effective atomic number, a0 the Bohr Figure 4 depicts the tree-level, two-loop and four-loop radius, and Q the estimated typical energy of the process, of μ− → þ Oeμ contributions to e -conversion from s . In order to order the muon mass mμ. While estimating Rμ−eþ , the term estimate Rμ−eþ , as defined in Eq. (1.1), we estimate the in the second parentheses in Eq. (2.7) cancels out in the muon capture rate, as outlined in [19],tobe ratio, yielding
− þ μe FIG. 4. Feynman diagrams contributing to μ → e -conversion from the dimension-nine all-singlets operator Os at the tree level (left), two-loop level (middle), and four-loop level (right). The blob represents the effective operator while the × represents the Higgs- boson vacuum expectation value.
075033-5 DE GOUVÊA, HUANG, KÖNIG, and SEN PHYS. REV. D 100, 075033 (2019) 6 2 1 2 2 2 2 2 2 Q GF yt ybyμyev Rμ− þ ¼jg μj pffiffiffi e e Λ2 2 q2 ð16π2Þ4 pffiffiffi 2 2 1 y y yμv 2 1 þ t b þ ð Þ 2 2 2 2 8 : 2:8 q ð16π Þ Λ GF Λ
The normalized conversion rate for this process as a function of Λ is depicted in Fig. 3 along with the current bounds on the process from the SINDRUM II collaboration [33], and the expected Mu2e sensitivity, Eq. (1.2). The current bound from SINDRUM II implies that Λ ≳ 10 GeV FIG. 5. Topologies that realize the all-singlets dimension-nine operator O at tree level. Topology 1 (left) involves only new for Oð1Þ couplings. Again, the neutrino mass requirements s μ− → þ bosons while Topology 2 (right) requires both new fermions and are inconsistent with the existing e -conversion bosons. In both topologies, the bosons can be scalars or vectors. bounds. If all gαβ are of the same magnitude, current constraints new-physics boson or couple to a new-physics on Λ from 0νββ—Λ ≳ 1 TeV for gee of order one—would translate into unobservable rates for μ− → eþ-conversion in boson and a new-physics fermion. This is depicted nuclei. However, there are no model-independent reasons in the right panel of Fig. 5. Again, the new-physics bosons can be scalars or vectors. to directly relate, e.g., gμe to gee, hence the bounds from 0νββ need not apply directly to searches for μ− → eþ- In order to systematically analyze the different internal conversion. Model-dependent considerations are required particles that can appear in Fig. 5, we determine the quantum numbers of pairs and triplets of the external in order to explore possible relations between gee and gμe. − þ SM fermions of interest. The different combinations of On the other hand, observable rates for μ → e -conver- pairs of fermions determine the possible quantum numbers sion require Λ ≲ 100 GeV and hence new particles with of the bosons in the internal lines in Fig. 5. Similarly, masses around (or below) the weak scale. It is natural to different combinations of triplets of fermions determine the suspect that models associated to such small effective quantum numbers of the potential new fermions in the scales are also vulnerable to lepton-number conserving, internal fermion line in Fig. 5 (right). low-energy observables, especially searches for CLFV. Table I lists all possible ways of pairing up any two As argued in the introduction, these phenomena can only SUð2Þ -singlet SM fermions.4 Generation indices, for both be addressed within UV-complete models, which we L leptons and quarks, have been omitted. Topology 1 can be introduce and discuss in the next section. realized by choosing three bosons with the same quantum numbers as these pairs, keeping in mind that there are two III. ULTRAVIOLET COMPLETIONS c c c αβ αβ fermions of each type—u , d , l —in Os . For bilinear OF THE EFFECTIVE OPERATOR Os combinations of the same generation of quarks, only Here we discuss tree-level UV-completions of the all- products symmetric in the color indices, i.e., forming a Oαβ 6¯ ð3Þ ð cÞαið cÞj ¼ singlets dimension-nine operator s , introduced in the 6or of SU c, exist since, e.g., u u α c i c αj c αj c i previous section, Eq. (2.2). As all fields in the effective −ðu Þαðu Þ ¼ðu Þ ðu Þα, where α is the dummy ð Þ ð3Þ operator are fermions, all new interactions involving SM Lorentz index and i; j are the SU c indices. Here, fields are either Yukawa or gauge interactions, i.e., they we will be concentrating on new-physics involving first- are all 3-point vertices. Furthermore, relevant interactions generation quarks, as we are interested in models that involving only new-physics fields are at most also 3-point mediate μ− → eþ-conversion at the tree level (left panel of vertices. This is due to the fact that the operator in question Fig. 4). Unless otherwise noted, we will not consider has six fermions in the final state and we are only interested models that “mix” different generations of the same quark- αβ in tree-level realizations of Os . Since only 3-point vertices flavor. αβ There are five different “minimal” realizations of are possible, there are only two topologies that lead to Os at the tree level [34,35]: Topology 1. Two of them involve heavy scalar bosons (1) All new particles are bosons. Each boson couples to only, while the remaining three require new-physics vector “ a pair of SM fermions, and three new-physics bosons and scalar bosons. Of course, one can consider less- ” define a new interaction vertex. This is depicted in minimal scenarios where one includes bosons with differ- the left panel of Fig. 5. The new-physics bosons can ent quantum numbers associated to the same fermion-pair, be scalars or vectors. (2) All new interactions involve one boson and two fermions. The new particles are bosons and fermi- 4Excluding left-handed antineutrinos νc. We will comment on ons and SM fields either couple pair-wise with a those later in this section.
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ð2Þ TABLE I. Quantum numbers of all possible pairs of the SU L TABLE III. Pairs of Standard Model fermions that share the gauge singlet Standard Model fermions lc, uc, dc. same gauge quantum numbers. The pairs of interest here are in bold. The pair lclc does not transform like any other pair of Pairs (Lorentz) Representation under ðSUð3Þ ; SUð2Þ Þ ð1Þ c c C L U Y SM fields; the same is true of the color-symmetric pairs of u u c c c c and d d . l l (scalar) ð1; 1Þ1 × ð1; 1Þ1 ¼ð1; 1Þ2 lc c ð1 1Þ ð3¯ 1Þ ¼ð3¯ 1Þ u (scalar) ; 1 × ; −2=3 ; 1=3 ð ð3Þ ð2Þ Þ Fermion pairs transforming as SU C; SU L Uð1Þ c c ð1 1Þ ð3 1Þ ¼ð3 1Þ Y l d (vector) ; 1 × ; −1=3 ; 2=3 c c ¯ ¯ ¯ lc νc ð1; 1Þ−1 scalar u u (scalar) ð3; 1Þ−2 3 × ð3; 1Þ−2 3 ¼ð3 ; 1Þ−4 3 þð6 ; 1Þ−4 3 LL, = = a = s = c c c c c c ¯ d u , l ν ð1; 1Þ−1 vector u d (vector) ð3; 1Þ−2 3 × ð3; 1Þ−1 3 ¼ð1; 1Þ−1 þð8; 1Þ−1 = = lcuc, uc dc, Q2, L¯ Q¯ , dcνc ð3¯ 1Þ c c ¯ ; 1=3 scalar d d ð3; 1Þ−1 3 × ð3; 1Þ−1 3 ¼ð3 ; 1Þ−2 3 þð6 ; 1Þ−2 3 (scalar) = = a = s = c c ð6 1Þ u d , QQ ; 1=3 scalar dcdc c νc ð3 1Þ , u ; 2=3 scalar dclc ¯ cνc ð3 1Þ , LQ, u ; 2=3 vector c c ucuc c lc ð3 1Þ e.g., the combination u d can connect to vector bosons in , d ; −4=3 scalar ð3Þ c c c c ð1 1Þ two different SU c representations. ν ν , ν ν ; 0 scalar ¯ ¯ Similarly, Table II lists all possible combinations of three LL, QQ, lclc, dcdc, ucuc, νcνc ð1; 1Þ0 vector ð2Þ ¯ c c c c ð8 1Þ SU L-singlet SM fermions. The different new-physics QQ, d d , u u ; 0 vector fermions that can make up Topology 2 must have the same quantum numbers as the combinations listed in the table. This list is exhaustive, and to get all possible diagrams, complete list, see Tables I, II, and III in [19]). Unlike one needs to consider all allowed, distinct permutations of the all-singlets operator, all other dimension-nine operators the triplets. In order to realize Topology 2, for each such saturate the constraints associated to nonzero neutrino combination, one needs to consider the possible ways of masses for Λ values that translate into tiny rates for arranging fermion pairs, listed in Table I. It can be shown μ− → eþ-conversion, see Fig. 7 in [19]. that this yields eighteen different “minimal” realizations of In order to systematically address this issue, we list all Topology 2, not considering the different representations the relevant SM fermion pairs that transform in the same for the same combination of SM fermions. αβ way in Table III. The pairs relevant for Os are shown in Next, we want to ensure that, at the tree level, the bold. From the table, one can see that a new particle that different new-physics scenarios lead to the all-singlets couples to, e.g., lc with uc or d¯c can also couple to L¯ Q¯ , operator but not to other dimension-nine (or lower dimen- and so on. The table reveals that there are two avenues for sional) LNV operators. New particles with the same avoiding unwanted couplings. One is to have one of the quantum numbers as some of the combinations in new bosons couple to the pair lclc, which is not degen- Table I can also couple to pairs of SM fermions that erate, quantum-number-wise, with any other pair of SM ð2Þ contain the SU L-doublets L, Q. For example, the pair fermions. The other is to add a new fermion and a new lc c ð3¯ 1Þ u transforms like a ; 1=3. A scalar that couples to this boson such that lc couples to them in Topology 2. The ¯ ¯ pair of SM fermions can also couple to L Q, since the latter reason for this is that all other pairings involving lc have an has identical quantum numbers. These new bosons would unwanted “match,” see Table III. This extra requirement lead to, along with the all-singlets operator, other six- drastically reduces the total number of minimal models for fermion operators, including ðL¯ Q¯ ÞðL¯ Q¯ Þðdc dcÞ (for a the two topologies, and allows us to write down all possible
ð2Þ lc c TABLE II. Quantum numbers of all the possible triplets of SU L gauge singlet Standard Model fermions , u , dc (with at most two identical fields).
Triplets Representation under ðSUð3Þ ; SUð2Þ Þ ð1Þ C L U Y lclc c ð1 1Þ ð1 1Þ ð3¯ 1Þ ¼ð3¯ 1Þ u ; 1 × ; 1 × ; −2=3 ; 4=3 c c c ð1 1Þ ð1 1Þ ð3 1Þ ¼ð3 1Þ l l d ; 1 × ; 1 × ; −1=3 ; 5=3 lc c c ð1 1Þ ð3¯ 1Þ ð3¯ 1Þ ¼ð3 1Þ þð6¯ 1Þ u u ; 1 × ; −2=3 × ; −2=3 a; −1=3 s; −1=3 c c c ð1 1Þ ð3 1Þ ð3 1Þ ¼ð3¯ 1Þ þð6 1Þ l d d ; 1 × ; −1=3 × ; −1=3 a; 1=3 s; 1=3 c c c ð1 1Þ ð3¯ 1Þ ð3 1Þ ¼ð1 1Þ þð8 1Þ l u d ; 1 × ; −2=3 × ; −1=3 ; 0 ; 0 c c c ð3¯ 1Þ ð3¯ 1Þ ð3 1Þ ¼½ð3 1Þ þð6¯ 1Þ ð3 1Þ u u d ; −2=3 × ; −2=3 × ; −1=3 a; −4=3 s; −4=3 × ; −1=3 ¼ð3¯ 1Þ þð6 1Þ þð3¯ 1Þ þð15¯ 1Þ ; −5=3 ; −5=3 ; −5=3 ; −5=3 c c c ð3¯ 1Þ ð3 1Þ ð3 1Þ ¼ð3¯ 1Þ ½ð3¯ 1Þ þð6 1Þ u d d ; −2=3 × ; −1=3 × ; −1=3 ; −2=3 × a; −2=3 s; −2=3 ¼ð3 1Þ þð6¯ 1Þ þð3 1Þ þð15 1Þ ; −4=3 ; −4=3 ; −4=3 ; −4=3
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TABLE IV. All new particles required for all different tree-level Table IV. Explicitly, they are (1) ζΦΣ, (2) χΔΣ, (3) ψΔΦ, Oαβ αβ realizations of the all-singlets dimension-nine operator s , and (4) ΦΣΔ. The first three realize Os via topology 2 αβ according to the restrictions discussed in the text. All particles [Fig. 5(right)] while the last one realizes O via topology 1 are SUð2Þ singlets. The fermions ψ, ζ, and χ come with a partner s L [Fig. 5(left)]. (ψ c, ζc, and χc respectively), not listed. We do not consider fields that would couple to the antisymmetric combination of same- flavor quarks since these cannot couple quarks of the same 1. Model ζΦΣ generation. Here, the SM particle content is augmented by a couple ¯ New particles ðSUð3Þ ; SUð2Þ Þ ð1Þ Spin ζ ≡ ð3 1Þ ζc ≡ ð3 1Þ C L U Y of vectorlike fermions ; −5=3 and ; 5=3, Φ ∼ ð1 1Þ Φ ≡ ðlc lcÞ ð1; 1Þ−2 Scalar the color-singlet scalar ; −2, and the colored c c ð6 1Þ scalar Σ ∼ ð6; 1Þ4 3. The most general renormalizable Σ ≡ ðu u Þ ; 4=3 Scalar = c c ð6 1Þ Δ ≡ ðd d Þ ; −2=3 Scalar Lagrangian is c c C ≡ ðu d Þ ð1; 1Þ1; ð8; 1Þ1 Vector c c c c ψ ≡ ð c c cÞ ð3¯ 1Þ LζΦΣ ¼ L þ L þ yΦαβΦlαl þ yΣ Σu u u l l ; 4=3 Fermion SM kin β u ¯ ζ ≡ ð c c cÞ ð3; 1Þ Fermion c c c c d l l −5=3 þ yΦζc Φζ d þ yΣζΣζd þ mζζζ c c c ¯ χ ≡ ðl u u Þ ð6; 1Þ−1 3 Fermion = þ VðΦ; Σ; 0ÞþH:c:; ð3:1Þ N ≡ ðlcdcucÞ ð1; 1Þ0, ð8; 1Þ0 Fermion L L where SM is the SM Lagrangian, kin contains the kinetic- energy terms for the new particles, and VðΦ; Σ; 0Þ is the UV completions with no more than three new particles. The Φ Σ final allowed combinations and the corresponding new most general scalar potential involving the scalars , , particles are listed in Table IV. The list is exhaustive, and all written out explicitly in Appendix A. By design, lepton Oαβ number is violated by two units but it is conserved in the possible UV completions of s at the tree level can be limit where any of the new Yukawa couplings vanishes. On implemented with a subset of less than or equal to three of the other hand, baryon number is conserved. In units where these particles. the quarks have baryon-number one, Σ can be assigned It is also important to consider whether new interactions þ2 ζ ζc −1 þ1 ð2Þ νc baryon-number , ; baryon-number ; , respec- would materialize if neutrino SU L-singlet fields, , Φ νc tively, and baryon-number zero. were also present. Pairings that include are also included Oαβ in Table III. Given all constraints discussed above, there are It is easy to check that this model realizes s via no new couplings involving νc other than the neutrino topology 2 [Fig. 5(right)] and c Yukawa coupling and ν Majorana masses for new-physics μ gαβ yΦαβyΦζc yΣζyΣu models that do not contain the vector C ∼ ð1; 1Þ1 field. ≡ : ð3:2Þ μ 5 2 2 In models that contain C , one need also consider the Λ MΦMΣmζ lcσ¯ μνc interaction term i Cμ. We return to the left-handed antineutrinos and the mechanism behind neutrino masses Here, yΦαβ controls the lepton-flavor structure of the model. μ− → þ j j2 in Sec. VI. e -conversion rates are proportional to yΦeμ , while 2 In the following subsections we list all the different those for 0νββ are proportional to jyΦeej . models. We divide them into different categories. Some The new-physics states will also mediate CLFV phe- models contain new vector bosons, others contain only nomena, sometimes at the tree level. In what follows, new-physics scalars or fermions. Since all new particles we write down the effective operators that give rise to need to be heavy, including potential new vector bosons, different CLFV processes, and estimate bounds on the no-vectors models are easier to analyze since, as is well- effective scales of these operators. The CLFV observables known, consistent quantum field theories with massive of interest are: ∓ vector bosons require extra care. There are, altogether, eight (1) μ → e e e decay: The effective Lagrangian models: four with and four without new massive vector giving rise to this decay, generated at the tree fields. We discuss the no-vectors models first. We will also level, is broadly distinguish models based on whether they also lead yΦ μy to the violation of baryon-number conservation and L ¼ e Φee ðμc cÞð c cÞ ð Þ μ→3e 2 e e e ; 3:3 whether any flavor-structure naturally arises. MΦ
and the relevant Feynman diagram is depicted in A. No-vectors models the left panel of Fig. 6. The strongest bounds on Here, all no-vectors models are discussed in turn. Models μþ → eþe−eþ come from the SINDRUM spectrom- are named according to the new-physics field content, see eter experiment [36]:
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FIG. 6. Feynman diagrams contributing to the CLFV processes μ → 3e (left), μþ → eþγ (middle), and μ− → e−-conversion (right) in model ζΦΣ.
Brðμþ → eþe−eþÞ < 1.0 × 10−12: ð3:4Þ as depicted in the right panel of Fig. 6. The effective Lagrangian can be estimated as Assuming the phase-space distributions are similar μ ðμ → ν¯ ν Þ to those of ordinary -decay e e μ , this y yΦ βyΦζc y c L ¼ Φμβ e Φζ ðμc cÞð c cÞ ð Þ translates into [37,38] μ→e 16π2Λ2 e d d ; 3:9 j j2 yΦeμyΦee −22 −4 ≤ 1.4 × 10 GeV ; ð3:5Þ where Λ is the effective scale, a function of MΦ and M4 Φ Mζ, and the lepton-index β is summed over. Note that this operator is also sensitive to the yΦeτ and or MΦ ≥ 290 TeV for Oð1Þ couplings. The Mu3e yΦμτ couplings. An extra contribution comes from experiment, under construction at PSI, aims to reach the middle panel of Fig. 6, where the photon is put sensitivities better than 10−15 on this channel [39] and offshell, and radiates a qq¯ pair. hence sensitivity to Φ-masses around 1000 TeV [7]. þ þ The SINDRUM II experiment at PSI constrains (2) μ → e γ decay: At the one-loop level, Φ-exchange − − μ → e -conversion in gold [33]: also mediates, as depicted in the middle panel of Fig. 6, μþ → eþγ. The effective operator governing Γðμ− þ → − þ Þ μ → eγ is Au Au e Au Rμ−e− ≡ − Γðμ þ Au → νμ þ PtÞ ð2 Þ yΦμμyΦμe e yμ αβ −13 L þ þ ¼ ð ¯ Þσ c ð Þ 7 10 ð90% Þ ð Þ μ →e γ 2 2 LH e Fαβ; 3:6 < × CL : 3:10 16π MΦ
where yμ is the muon Yukawa coupling. Experi- Using Eq. (2.7), we estimate [37] mentally, the most stringent constraints come from pffiffiffi 2 the MEG experiment at PSI [40] 2 yΦμβyΦeβyΦζc yΦζc − − ¼ ð Þ Rμ e 2 2 : 3:11 GF 16π Λ Brðμþ → eþγÞ¼4.2 × 10−13: ð3:7Þ Oð1Þ Λ ≥ 30 Using results from [41], we get For couplings, this yields TeV. Stronger sensitivity is expected from the next-gen- 2 eration experiments COMET [15], DeeMe [16], jyΦμμyΦμej ðμþ → eþγÞ ≈ 5 3 10−6 and Mu2e [17], as discussed in the introduction. Br . × 4 ð Þ MΦ TeV Ultimately, one would be sensitive to Λ scales up to < 4.2 × 10−13; ð3:8Þ a few 100 TeV. (4) Muonium-antimuonium oscillations ðμþe− → μ−eþÞ: − þ which leads to MΦ ≳ 60 TeV, given Oð1Þ cou- Muonium ðMuÞ is the bound state of an e and a μ , plings. As expected, the μþ → eþγ bound is weaker whereas its anti-partner, the antimuonium ðMuÞ is than that of μ → 3e as the former is loop-suppressed. the bound state of an eþ and a μ−. Muonium- The upgraded MEG-II experiment plans to reach antimuonium oscillation is a process where muonium a sensitivity of 10−14 with three years of data converts to antimuonium, thereby changing both taking [42]. electron-number and muon-number by two units (3) μ− → e−-conversion in nuclei: In this model, [37]. Here, the effective Lagrangian governing this μ− → e−-conversion occurs at the one-loop level, process at the tree level is
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