h - h - h - e - (ν e ) (ν e )

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Chapter 8 Higgs triplet eects in purely leptonic processes We consider the eect of complex Higgs triplets on purely leptonic processes and survey the experimental constraints on the mass and couplings of their single and double charge members. Present day experiments tolerate values of the Yukawa couplings of these scalars at the level of the standard electroweak gauge couplings. We show that the proposed measurement of the ratio R LCD = ( e)=[( e)+( e e)] at LAMPF would allow to explore a large region of the parameter space inaccessible to the usual ratio R = ( e)=( e). 8.1 Motivation Although the Standard Model (SM) of the strong and electroweak interactions seems to agree very well with the experimental data, the Higgs sector still remains practically unexplored and one can therefore consider dierent extensions. Here we will focus our attention on Higgs triplets with non zero hypercharge. They are a common feature in models where the lefthanded neutrinos acquire a Majorana mass through the Higgs mechanism. This is the case, for instance, of the classical version of the Left{Right Symmetric extension of the SM [30{34]. Higgs triplets under the standard SU() L gauge group have some very specic properties. Their vacuum expectation values have to be small in order not to spoil the agreement between 165

166 Chapter 8. Higgs triplet eects in purely leptonic processes the theoretical and the experimental values of the electroweak parameter [0]. Moreover, since they have two units of weak hypercharge, apart from the electrically neutral scalar (h 0 ) there are also singly charged (h + ) and doubly charged (h ++ ) ones. This has an important phenomenological consequence, namely, that they can not couple to quarks and therefore their dominant eects are to be observed only in purely leptonic processes. Moreover, these eects are not necessarily small because the Higgs triplets do not participate in the generation of the lepton Dirac masses and therefore their Yukawa couplings can be large. Another feature displayed by scalar triplets (and, more generally, by any unmixed higher dimension scalar multiplet) is that they exhibit equal mass-squared spacing ordered by the scalar eld electric charges [59, 03]. This implies that, in general, m h ++ >m h +. Several experimental constraints on the couplings and masses of the h ++ have been considered in the literature [59{63]. They include the constraints arising from the value of the anomalous magnetic moment of the electron and the muon, the angular distribution in the Bhabha scattering and the experimental limits on muonium{antimuonium transitions and non standard muon decays. The eects of the singly charged member of the triplet, h +, have not been considered so extensively. The existence of such eld would aect the purely leptonic neutrino processes and precise measurements in this sector, like those of the CHARM II collaboration [66], impose additional constraints. In this respect, there has been a proposal by the Large Cerenkov Detector (LCD) Project collaboration [65] of an experiment at LAMPF that would allow the measurement of the ratio R LCD ( e) ( e)+( e e) (8.1) with a precision of % (corresponding to a 0.9% precision in the measurement of sin W ). Such high precision is due to the particular setup of this experiment which will be almost free of systematic uncertainties [65], making it competitive with the standard CHARM II ratio R = ( e)=( e)fromwhich the value of sin W is obtained with an accuracy at the level of 3.6%. Therefore, the ratio R LCD could be a suitable tool to probe physics beyond the SM. This is the case, for instance, of supersymmetric eects [74, 04]. The existence of h would also aect this ratio and more stringent bounds on its couplings and mass might be imposed from the measured value.

8. Experimental constraints on Left{Right Models 167 In this paper we shall determine the region in the parameter space where the eects of the h bosons could be observed in the measurement ofr LCD. This requires rst an updating of the experimental constraints on the h mass and Yukawa couplings. We shall also comment on the implications for the h mass and couplings. 8. Experimental constraints on Left{Right Models First of all, let us give the dierent constraints on the h and h masses and Yukawa couplings using the notation and conventions dened in Sec..3.1. 8..1 Bounds on h mass and Yukawa couplings Dening ij h ij =m h +,we list now the constraints on ij arising from dierent experimental measurements. Restrictions from the decay! e Parametrizing the e vertex in the usual way, with + A 5 = F 1 F + i F 3 q + q m + m e m + m e A = G 1 G + i G 3 q + q m + m e m + m e the decay width, ; (! e), in the limit m e << m can be written as ;(! e) = m jf j + jg j and the corresponding branching ratio is B(! e) = 96 G F m4 jf j + jg j : (8.) The h ; contribution to F, G arising from the diagram of g. 8.1a is F = G = m 19 [ e ( ee + )+ e ] : (8.3)

168 Chapter 8. Higgs triplet eects in purely leptonic processes µ - ν i h - h - γ e - µ - h - ν µ e - ν e (a) (b) γ ν µ ν µ (ν e ) (ν e ) h - e - e - h - h - ν i e - h - e - e - (µ - ) e - (µ - ) ν µ ν µ (c) (d) Figure 8.1: Diagrams contributing to the dierent observables described in the text: (a) ;! e ; (b) ;! e ; e (c) anomalous magnetic moment of the electron and muon and (d) e, e and e e collisions. From the experimental bound [188] B(! e) < 4:9 10 ;11 (90% C.L.) using eqs.(8.) and (8.3) we obtain j e ( ee + )+ e j < 4: 10 ;8 GeV ; (90% C.L.) :

8. Experimental constraints on Left{Right Models 169 Restrictions from the decay! e e and neutrino oscillation experiments The existence of h ; would allow the non standard decay! e e through the diagram of g. 8.1b. The corresponding width is ;(! e e )= m5 1536 3 ee : From the experimental limit [188] ;(! e e ) ;(! e e ) < 0:01 (90% C.L.) the following bound can be obtained j ee j < 3:6 10 ;6 GeV ; (90% C.L.) : (If we further assume e ; universality thenwewould have j ee j = j j < 1:9 10 ;3.) Recently, it has been pointed out in ref. [05] that the results of the KARMEN experiment [06, 07] on neutrino oscillations lead to the bound GN G F < 3:1 10 ;3 GeV ; (90% C.L.) (8.4) where G F is the Fermi constant andg N is the coupling constant of an eective four fermion interaction of the form L = G N ( P L e) P L e + h.c. with P L =(1; 5 )=. The amplitude of the diagram of g. 8.1b can be written this form after a suitable Fierz reordering with G N ee. Then, from eq. (8.4) we can obtain the more restrictive bound j ee j < 6:5 10 ;7 GeV ; (90% C.L.) : (8.5) (Again, assuming e ; universality wewould have j ee j = j j < 8:1 10 ;4.)

170 Chapter 8. Higgs triplet eects in purely leptonic processes Restrictions from anomalous magnetic moments By explicit calculation of the diagrams of g. 8.1c we nd the following contribution to the anomalous magnetic moment, a i (g ; )=, of the charged lepton i, a i = ; m X i ij : (8.6) 48 j=e The theoretical values of a e and a are [08, 09] a th e = (115965460 17 75) 10 ;1 a th = (116590 0) 10 ;10 and the corresponding experimental values are [188] a exp e = (115965193 10) 10 ;1 a exp = (1165930 84) 10 ;10 : From these values we can obtain the 90% C.L. intervals for any non standard contribution to a i 1, ;5:1 10 ;10 < a e < ;0: 10 ;10 ;1:1 10 ;8 < a < 1:7 10 ;8 : Since the contribution given by eq. (8.6) is negative, the following bounds apply, ja e j < 5:1 10 ;10 ja j < 1:1 10 ;8 : (8.7) Then, the following restrictions are obtained, X ej j=e X j j=e < 0:9 GeV ; (90% C.L.) < 1:5 10 ;4 GeV ; (90% C.L.) from which we can infer the following bounds, j ee j j e j < 0:54 GeV ;1 (90% C.L.) j j j e j j j < 1: 10 ; GeV ;1 (90% C.L.) : (8.8) 1 They are given by a exp ; a th 1:645 ( exp + th) 1=.

8. Experimental constraints on Left{Right Models 171 Restrictions from the value of sin W measured in purely leptonic neutrino interactions Using the ratio R = ( e)=( e), the CHARM II Collaboration [66] has been able to obtain a precise value of sin W from purely leptonic e and e collisions, x W sin W =0:34 0:0083 : (8.9) The SM tree level amplitude for the e scattering is given by M = i G F p e [P L ; x W ] e (1 ; 5 ): (8.10) A similar expression with straightforward modications aecting only the last factor of the r.h.s. of eq. (8.10) can be written for the e amplitude. The two h ; exchanging diagrams of g. 8.1d add new contributions to the e and e amplitudes respectively. With a suitable Fierz transformation one can readily see that the net eect of these h ; contributions consists in replacing the term inside the square brackets of eq. (8.10) by P L ; x W! 1+ e p GF! P L ; x W ' 1+ e p GF!" P L ; x W 1 ; e p GF!# : (8.11) This replacement induces an apparent shift of x W and the parameter given by x W '; x W e p GF = e p GF : The agreement between the results of the CHARM II Collaboration with those obtained from semi{leptonic interactions (where h eects would be absent) suggests that e = p G F is small (of the order of a few percent at most) and thus justies the use of the approximate form given by the last expression of eq. (8.11). The value given by eq. (8.9) coincides with the theoretical prediction, x th W = 0:34 0:001 (see, e.g., ref. [10]). The 90% C.L. interval for x W is therefore jx W j < 0:0138

17 Chapter 8. Higgs triplet eects in purely leptonic processes from which we obtain j e j < 9:9 10 ;4 GeV ;1 (90% C.L.) : (8.1) A similar analysis can be carried out in the case of e e collisions. The experimental study has been done at LAMPF [11] and the obtained experimental value for x W is x W =0:49 0:063 : In this case the SM tree level amplitude can be conveniently written as M = i G F p e [;P L +(P L ; x W )] e (1 ; 5 ): The eect of the h ; contribution is again the substitution (8.11) with e replaced by ee. The extra term, ;P L, (compared to the e case) is due to the W exchange contribution and is unaected by theh ; exchange. The apparent shiftonx W is now x W '; x W ee p GF and the 90% C.L. interval for x W is ;0:09 < x W < 0:1 which leads to the following bound j ee j < :5 10 ;3 GeV ;1 (90% C.L.) : (8.13) An alternative approach in order to obtain bounds on non SM physics from the measured values of the ( e e) is described in ref. [11]. If we write d( e e) dy = 0 ha + B(1 ; y)+c(1 ; y) i where 0 = G F s=4, the h; exchange diagram adds the following contribution to the quantity A, A = ;( + 4x W ) ee p GF

8. Experimental constraints on Left{Right Models 173 90% C.L. bound Process j ee j < :5 10 ;3 GeV ;1 j e j < 9:9 10 ;4 GeV ;1 j j < 1: 10 ; GeV ;1 j ee j < 6:5 10 ;7 GeV ; e e e e (g ; ) osc. Table 8.1: Best bounds on ij. and from the experimental value of ( e e) the following bound on ee can be derived (see ref. [11] for details ), j ee j < 7: 10 ;3 GeV ;1 (90% C.L.) which is less restrictive than the bound of eq. (8.13). Summary of experimental restrictions on h The restrictions imposed by the above observables on ee, and e are summarized in table 8.1 where only the most restrictive ones, given by eqs. (8.5), (8.8), (8.1) and (8.13), are listed. The combined bounds on ij are also shown in g. 8.. 8.. Bounds on h mass and Yukawa couplings If the inequality m h + < m h ++ holds, as it happens in practically all Higgs triplet models, both the measurement ofr LCD and the bounds on ij described above would also aect the restrictions on the mass and couplings of the doubly charged scalar, h ++. Indeed, dening 0 ij h ij =m h ++, if the singly charged scalars are lighter than the doubly charged ones then 0 ij < ij and therefore any upper bound of ij would be also an upper bound of 0 ij. The direct bounds on 0 ij (without assuming the inequality m h + < m h ++) are obtained from the experimental results on (g ; ), Bhabha scattering, muonium-antimuonium (M M) transitions and the decay ;! e ; e + e ;. They are summarized in the left half of table 8.. The fact that the h ; exchange diagram modies the quantity A is due to the helicity structure in the lagrangian of eq. (.54). Acharged Higgs belonging to a doublet would, instead, contribute to C (see ref. [11]).

174 Chapter 8. Higgs triplet eects in purely leptonic processes 90% C.L. bound Process 90% C.L. bound Process (general) (assuming m h + <m h ++) jeej 0 < :8 10 ;3 GeV ;1 Bhabha jeej 0 < :5 10 ;3 GeV ;1 e e j 0 j < 4:3 e 10;3 GeV ;1 (g ; ) j 0 j < 9:9 e 10;4 GeV ;1 e e jj 0 < 4:3 10 ;3 GeV ;1 (g ; ) jj 0 < 4:1 10 ;3 GeV ;1 (g ; ) jee 0 j 0 < 8:6 10 ;6 GeV ; MM jee 0 j 0 < 6:5 10 ;7 GeV ; osc. j 0 ee 0 j < :3 e 10;11 GeV ;! 3e j 0 ee 0 j < :3 e 10;11 GeV ;! 3e Table 8.: Best bounds on 0 ij. The (g ; ) bound is obtained by applying eq. (8.7) to the h ++ contribution to a i given by [59], a i = ; m i 6 X j=e The resulting inequalities are 0 ij : (8.14) 0 j 0 eej j 0 ej < 0:19 GeV ;1 (90% C.L.) 0 e 0 < 4:3 10 ;3 GeV ;1 (90% C.L.) : The remaining bounds are discussed in ref. [6] 3. If m h + <m h ++, the bounds of table 8.1 became also bounds on ij 0. We show them in the right half of table 8.. In the case of 0, the slight improvement of the bound is obtained by adding the h + and h ++ contributions to a i, given by eqs. (8.6) and (8.14) respectively, and using the inequality 0 ij < ij. We have then 3m i 16 X j=e 0 ij < a (h+ ) i +a (h++ ) i with the r.h.s. satisfying the bounds of eq. (8.7). 3 The MM bound has been updated according to the new experimental limit given in ref. [188]. The Bhabha scattering and! 3e bounds were also discussed in ref. [59]. Notice that our h ee, h and h e are respectively the g ee, g and g e= of ref. [6].

8.3 Analytical eect of Left-Right Models on R LCD 175 8.3 Analytical eect of Left-Right Models on R LCD We now turn to the ratio R LCD dened in eq. (8.1). Introducing the quantities ; = 1 (1 ; x W ) 0 ; = 1 (;1 ; x W ) + = 0 + = ;x W the tree level SM value can be written as RLCD 0 ; + 1 = 3 + + + 3 1 ; + 0 ; + 1 =0:14 : (8.15) 3 0 + This value is modied by the presence of non SM physics (in our case, the h ; interactions) as well as by SM radiative corrections. The dominant h ; contributions to the cross sections appearing in eq. (8.1) are given by the two diagrams of g. 8.1d and the rst one involving the electron neutrino. The eect of these h ; exchange contributions is taken into account by simply replacing in eq. (8.15) the quantities and 0 by ~ and ~ 0 respectively, where e ~ + = + ~ ; = ; + 1 p GF ee ~ 0 + = 0 + ~ 0 ; = 0 ; + 1 p : GF Thus, we have ~ ; + 1 R LCD = 3 ~ + ~ + + 3 1~ ; +~ 0 ; + 1 3 ~0 + where R R:C: LCD ref. [1]. The result is +R R:C: LCD is the eect of the SM radiative corrections which have been computed in R R:C: LCD =0:036 R 0 LCD =5:1 10 ;3 : 8.4 Numerical Analysis of Left-Right Models eects on R LCD and discussion In g. 8.b we plot the contour lines of R LCD =R SM LCD, where R SM LCD R 0 LCD +R R:C: LCD =0:147

(g ) µ δ µµ (GeV 1 ) 0.01 0.005 0 ν osc. (a) ν e e 0 0.001 0.00 0.003 δ ee (GeV 1 ) 0.001 ν µ e/ν µ e 1.5 1. δ eµ (GeV 1 ) 0.0005 1.01 1.0 1.05 1.1 ν e e 0 0 0.001 0.00 0.003 δ ee (GeV 1 ) (b) Figure 8.: Allowed regions (white zones) in the j ee j-j j plane (a) and j ee j- j e j plane (b). R LCD =R SM LCD In the latter we also show the contour lines for the ratio as predicted by the Higgs triplet model. 176

8.4 Numerical Analysis of Left-Right Models eects on R LCD and discussion 177 is the SM prediction (including radiative corrections). We observe that in a large part of the allowed region in the j ee j-j e j plane the deviations of the ratio R LCD from the SM prediction are larger than % and therefore detectable. For some (allowed) values of ee and e these deviations can be even larger than 50% (in the top right corner of the allowed region of g. 8.b the value of R LCD would double the SM one). On the other hand, if no deviations from the SM were observed the region above the 1.0 curve would be ruled out. The! 3e bound on jee 0 ej 0 appearing in the last line of table 8. is, by far, the most restrictive one and implies that either m h ++ is very large or h ee h e is very small. If the couplings h ij are not small compared to, say, the SU() L gauge coupling g, then h ++ must be very massive. In fact, if h ee h e g the h ++ mass would be extremely large ( 100 TeV). The same applies to m h + and m h 0, for if the three masses were very dierent there would be unacceptable contributions to the electroweak parameter [59]. As a result, the quantities ij and ij 0 would be very small and Higgs triplet eects at the tree levelwould be hard to detect. Nevertheless, there could still be sizable one-loop eects through (oblique) contributions to the parameter. If, instead, h ee h e is very small, one can consider two situations. One possibility is that both couplings are very small as it happens with the Yukawa couplings of the SM Higgs to the rst two fermion generations, which are several orders of magnitude smaller than the gauge couplings, a fact that is considered an unnatural feature of the SM. Another theoretically more appealing possibility isthat h e = 0 (i.e.i.e., that the Higgs triplet interactions are diagonal in lepton avour) and h ee h g. Indeed, one can have this type of scenario compatible with all the bounds of tables 8.1 and 8.. For instance, if m < h + m h ++ 500 GeV, one could have h ee h g =5 while fullling the parameter constraint. Thus, extended Higgs sectors as the one considered here are specially attractive since they can be \natural", entailing a potentially rich phenomenology beyond the SM.

178 Chapter 8. Higgs triplet eects in purely leptonic processes 8.5 Conclusions Though we have updated the dierent bounds on the couplings and masses of the single and double charged members of a Left-Right modelwe still nd that in a large part of the allowed region the deviations from the SM prediction are detectable with the proposed measurement of the ratio R LCD = ( e)=[( e)+( e e)]. Deviations from the SM as large as 50% are still allowed and such an experiment would put tied limits on the bounds on the couplings and masses of the single and double charged members of a Left-Right model.