Literature DB >> 28260971

Universal Unitarity Triangle 2016 and the tension between [Formula: see text] and [Formula: see text] in CMFV models.

Monika Blanke1, Andrzej J Buras2.   

Abstract

Motivated by the recently improved results from the Fermilab Lattice and MILC Collaborations on the hadronic matrix elements entering [Formula: see text] in [Formula: see text]-[Formula: see text] mixing, we determine the universal unitarity triangle (UUT) in models with constrained minimal flavour violation (CMFV). Of particular importance are the very precise determinations of the ratio [Formula: see text] and of the angle [Formula: see text]. They follow in this framework from the experimental values of [Formula: see text] and of the CP-asymmetry [Formula: see text]. As in CMFV models the new contributions to meson mixings can be described by a single flavour-universal variable S(v), we next determine the CKM matrix elements [Formula: see text], [Formula: see text], [Formula: see text] and [Formula: see text] as functions of S(v) using the experimental value of [Formula: see text] as input. The lower bound on S(v) in these models, derived by us in 2006, implies then upper bounds on these four CKM elements and on the CP-violating parameter [Formula: see text], which turns out to be significantly below its experimental value. This strategy avoids the use of tree-level determinations of [Formula: see text] and [Formula: see text], which are presently subject to considerable uncertainties. On the other hand, if [Formula: see text] is used instead of [Formula: see text] as input, [Formula: see text] are found to be significantly above the data. In this manner we point out that the new lattice data have significantly sharpened the tension between [Formula: see text] and [Formula: see text] within the CMFV framework. This implies the presence of new physics contributions beyond this framework that are responsible for the breakdown of the flavour universality of the function S(v). We also present the implications of these results for [Formula: see text], [Formula: see text] and [Formula: see text] within the Standard Model.

Entities:  

Year:  2016        PMID: 28260971      PMCID: PMC5312165          DOI: 10.1140/epjc/s10052-016-4044-6

Source DB:  PubMed          Journal:  Eur Phys J C Part Fields        ISSN: 1434-6044            Impact factor:   4.590


Introduction

Already for decades the transitions in the down-quark sector, that is – and – mixings, have been vital in constraining the Standard Model (SM) and in the search for new physics (NP) [1, 2]. However, theoretical uncertainties related to the hadronic matrix elements entering these transitions and their large sensitivity to the CKM parameters so far precluded clear cut conclusions about the presence of new physics (NP). The five observables of interest arewith being the mass differences in – mixings and and the corresponding mixing induced CP-asymmetries. describes the size of the indirect CP-violation in – mixing. and are already known with impressive precision. The asymmetries and are less precisely measured but have the advantage of being subject to only very small hadronic uncertainties. We do not include in (1) as it is subject to much larger theoretical uncertainties than the five observables in question. The hadronic uncertainties in and within the SM and CMFV models reside within a good approximation in the parametersFortunately, during the last years these uncertainties decreased significantly. In particular, concerning and , an impressive progress has recently been made by the Fermilab Lattice and MILC Collaborations (Fermilab-MILC) that find [3]with uncertainties of 3 % and 4 %, respectively. An even higher precision is achieved for the ratioThis value is significantly lower than the central value 1.27 in the previous lattice estimates [4] and its reduced uncertainty by a factor of three plays an important role in our analysis. The ETM Collaboration has also presented results for matrix elements of all five operators entering – mixing [5]. This work, however, only employs two flavours of sea quarks and does not estimate the uncertainty from quenching the strange quark. The ETM and Fermilab-MILC results for matrix elements differ by  %, or , which could arise from the omitted strange sea. We think it is safer to avoid this issue and use only the Fermilab-MILC results with . However, we note that the result for obtained by the ETM Collaboration supports a rather low value of from the Universal Unitarity Triangle (UUT). An extensive list of references to other lattice determinations of these parameters can be found in [3]. Lattice QCD also made impressive progress in the determination of the parameter , which enters the evaluation of [6-11]. The most recent preliminary world average from FLAG reads [12], very close to its large N value [13, 14]. Moreover, the analyses in [15, 16] show that cannot be larger than 0.75 but must be close to it. Taking the present results and precision of lattice QCD into account it is then a good approximation to set . In the evaluation of we also take into account long distance contributions parametrised by [17]. Note that at present the theoretical uncertainty in is dominated by the parameter [18] summarising NLO and NNLO QCD corrections to the charm quark contribution. We take these uncertainties into account. With determined already very precisely, the main uncertainties in the CKM parameters reside inwith being one of the angles of the unitarity triangle (UT). These three parameters can be determined from tree-level decays that are subject to only very small NP contributions. However, the tensions between inclusive and exclusive determinations of and to a lesser extent of do not yet allow for clear cut conclusions on their values. Moreover, the current world average of direct measurements of is not precise [19]This is consistent with from the U-spin analysis of and decays () [20]. The U-spin analysis by LHCb [21], on the other hand, finds a lower value in good agreement with the result from the UUT analysis in (25). The present uncertainties in and from tree-level decays preclude then a precise determination of the so-called reference unitarity triangle (RUT) [22] which is expected to be practically independent of the presence of NP. In addition the uncertainty in prevents precise predictions for and in the SM. However, in the SM and more generally models with constrained minimal flavour violation (CMFV) [23-25] it is possible to construct the so-called Universal Unitarity Triangle (UUT) [23] for which the knowledge of and is not required. The UUT can be constructed fromand this in turn allows one to determine and . The important virtue of this determination is its universality within CMFV models. In the case of transitions in the down-quark sector various CMFV models can only be distinguished by the value of a single flavour-universal real one-loop function, the box diagram function S(v), with v collectively denoting the parameters of a given CMFV model. This function enters universally , and and cancels out in the ratio in (7). Therefore the resulting UUT is the same in all CMFV models. Moreover, it can be shown that in these models S(v) is bounded from below by its SM value [26]with given in (11). The recent results in (3) and (4) have a profound impact on the determination of the UUT. The UUT can be determined very precisely from the measured values of and . This in turn implies a precise knowledge of the ratio and the angle , both to be compared with their tree-level determinations. Also the side of the UUT can be determined precisely in view of the result for in (4). In order to complete the determination of the full CKM matrix without the use of any tree-level determinations, except for , we will use two strategies:Both strategies use the determination of the UUT by means of (7) and allows to determine the whole CKM matrix, in particular , , and as functions of S(v). Yet their outcome is very different, which signals the tension between and in this framework. As we will demonstrate below, this tension, known already from previous studies [27, 28], has been sharpened significantly through the results in (3) and (4). Using these two strategies separately allows one to exhibit this tension transparently. Indeed we have the following:It has been known since 2008 that the SM experiences some tension in the correlation between and [29-33]. It should be emphasised that in CMFV models only the version of this tension in [30], i. e. NP in , is possible as in these models there are no new CP-violating phases. Therefore has to be used to determine the sole phase in these models, the angle in the UT, or equivalently the CKM phase, through the unitarity of the CKM matrix. The resulting low value of can be naturally raised in CMFV models by enhancing the value of S(v) and/or increasing the value of . However, as pointed out in [27, 28], this spoils the agreement of the SM with the data on , signalling the tension between and in CMFV models. The 2013 analysis of this tension in [34] found that the situation of CMFV with respect to transitions would improve if more precise results for and turned out to be lower than the values known in the spring of 2013. The recent results from [3] in (3) show the opposite. Both and increased. Moreover the more precise and significantly smaller value of enlarges the tension in question. : strategy in which the experimental value of is used to determine as a function of S(v), and is then a derived quantity. : strategy in which the experimental value of is used, while is then a derived quantity and follows from the determined UUT. The lower bound in (8) implies in upper bounds on , , and which are saturated in the SM, and in turn it allows to derive an upper bound on in CMFV models that is saturated in the SM but turns out to be significantly below the data. The lower bound in (8) implies in also upper bounds on , , and which are saturated in the SM. However the S(v) dependence of these elements determined in this manner differs from the one obtained in , which in turn allows to derive lower bounds on in CMFV models that are reached in the SM but turn out to be significantly above the data. In view of the new lattice results, in this paper we take another look at CMFV models. Having more precise values for , and than in 2013, our strategy outlined above differs from the one in [34]. In particular we take to be a derived quantity and not an input as done in the latter paper. Moreover, we will be able to reach much firmer conclusions than it was possible in 2013. In particular, in contrast to [34] and also to [3] at no place in our paper tree-level determinations of , and are used. However, we compare our results with them. It should be mentioned that Fermilab-MILC identified a significant tension between their results for the mass differences and the tree-level determination of the CKM matrix within the SM. Complementary to their findings, we identify a significant tension within processes, that is between and in the whole class of CMFV models. Moreover, we determine very precisely the UUT, in particular the angle in this triangle and the ratio , both valid also in the SM. Our paper is organised as follows. In Sect. 2 we determine first the UUT as outlined above, that in 2016 is significantly better known than in 2006 [25] and in particular in 2000, when the UUT was first suggested [23]. Subsequently we execute the strategies and defined above. The values of , , and , resulting from these two strategies, differ significantly from each other which is the consequence of the tension between and in question. In Sect. 3 we present the implications of these results for , and within the SM, obtaining again rather different results in and . In Sect. 4 we briefly discuss how the models match the new lattice data and comment briefly on other models. We conclude in Sect. 5.

Deriving the UUT and the CKM

Determination of the UUT

We begin with the determination of the UUT. For the mass differences in the systems we have the very accurate expressions The value 2.322 in the normalisation of S(v) is its SM value for obtained fromand is the perturbative QCD correction [35]. Our input parameters, equal to the ones used in [3], are collected in Table 1.
Table 1

Values of the experimental and theoretical quantities used as input parameters. For future updates see PDG [36] and HFAG [37]

\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$m_{B_s} = 5366.8 (2)\, \mathrm{MeV}$$\end{document}mBs=5366.8(2)MeV [36] \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$m_{B_d}=5279.58 (17)\, \mathrm{MeV}$$\end{document}mBd=5279.58(17)MeV [36]
\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\Delta M_s = 17.757 (21) \,\text {ps}^{-1}$$\end{document}ΔMs=17.757(21)ps-1 [37] \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\Delta M_d = 0.5055 (20) \,\text {ps}^{-1}$$\end{document}ΔMd=0.5055(20)ps-1 [37]
\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$S_{\psi K_S}= 0.691 (17)$$\end{document}SψKS=0.691(17) [37] \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$S_{\psi \phi }= 0.015 (35)$$\end{document}Sψϕ=0.015(35) [37]
\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$|V_{us}|=0.2253 (8)$$\end{document}|Vus|=0.2253(8) [36] \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$|\varepsilon _K|= 2.228 (11)\cdot 10^{-3}$$\end{document}|εK|=2.228(11)·10-3 [36]
\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$F_{B_s}$$\end{document}FBs = \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$226.0 (22)\, \mathrm{MeV}$$\end{document}226.0(22)MeV [38] \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$F_{B_d}$$\end{document}FBd = \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$188 (4)\, \mathrm{MeV}$$\end{document}188(4)MeV [39]
\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$m_t(m_t)=163.53 (85)\, \mathrm{GeV}$$\end{document}mt(mt)=163.53(85)GeV \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$S_0(x_t)=2.322 (18)$$\end{document}S0(xt)=2.322(18)
\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\eta _{cc}=1.87 (76)$$\end{document}ηcc=1.87(76) [18] \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\eta _{ct}= 0.496 (47)$$\end{document}ηct=0.496(47) [40]
\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\eta _{tt}=0.5765 (65)$$\end{document}ηtt=0.5765(65) [35] \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\eta _B=0.55 (1)$$\end{document}ηB=0.55(1) [35, 41]
\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\tau _{B_s}= 1.510 (5)\,\text {ps}$$\end{document}τBs=1.510(5)ps [37] \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\Delta \Gamma _s/\Gamma _s=0.124 (9)$$\end{document}ΔΓs/Γs=0.124(9) [37]
\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\tau _{B_d}= 1.520 (4)\,\text {ps}$$\end{document}τBd=1.520(4)ps [37] \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\kappa _\varepsilon = 0.94 (2)$$\end{document}κε=0.94(2) [17]
Values of the experimental and theoretical quantities used as input parameters. For future updates see PDG [36] and HFAG [37] From (9) and (10) we find using (4)which perfectly agrees with [3]. The tree-level determination of this ratio, quoted in the latter paper and obtained from CKMfitter [42], readsIt is significantly higher than the value in (12). It should be emphasised that the values of and to a very good approximation do not enter this ratio. Therefore this discrepancy is not a consequence of the tree-level determinations of and . As we will demonstrate below it is the consequence of the value of the angle , which due to the small value of found in [3] turns out to be significantly smaller than its tree-level value in (6). Now,with being one of the sides of the unitarity triangle (see Fig. 1) andwhere we have usedobtained from
Fig. 1

Universal Unitarity Triangle 2016. The green square at the apex of the UUT shows that the uncertainties in this triangle are impressively small

Universal Unitarity Triangle 2016. The green square at the apex of the UUT shows that the uncertainties in this triangle are impressively small versus in CMFV (green) compared with the tree-level exclusive (yellow) and inclusive (violet) determinations. The squares are our results in (red) and (blue) Thus using (12) and (14) we determine very preciselyHaving determined and we can construct the UUT shown in Fig. 1, from which we findWe observe that the UUT in Fig. 1 differs significantly from the UT obtained in global fits [42, 43], with the latter exhibiting smaller and larger values. Subsequently, using the relationallows for a very precise determination of the ratioThis implies, as shown in Fig. 2, a strict correlation between and , which can be compared with the tree-level determinations of both CKM elements, also shown in this plot. The exclusive determinations [3, 44–46] giveand the inclusive ones [47]We note that after the recent Belle data on [46], the exclusive and inclusive values of do not differ by much, while in the case of there is a significant difference. Moreover, the recent result on from LHCb with [48] favours its lower value in (22).
Fig. 2

versus in CMFV (green) compared with the tree-level exclusive (yellow) and inclusive (violet) determinations. The squares are our results in (red) and (blue)

Upper bounds on CKM elements in units of and of in units of obtained using strategies and as explained in the text. We set We observe that within the CMFV framework only special combinations of these two CKM elements are allowed. The red and blue squares represent the ranges obtained in the strategies and , respectively, as explained below and summarised in Table 2. We observe significant tensions both between the results in and and also between them and the inclusive tree-level determination of . On the other hand, the exclusive determination of accompanied by the inclusive one for gives , very close to the result in (21). However, the separate values of and in (22) and (23) used to obtain this result are not compatible with our findings in , implying problems with as we will see below.
Table 2

Upper bounds on CKM elements in units of and of in units of obtained using strategies and as explained in the text. We set

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Returning to the issue of the origin of the difference between (12) and (13), the new lattice results [3] have important implications on the angle in the UUT that can be determined by means ofWith the very precise value of and consequently we can precisely determine the angle independently of the values of S(v), and . In Fig. 3 we show as a function of from which we extractbelow its central value from tree-level decays in (6), and with an uncertainty that is by a factor of three smaller. We will use this value in what follows. We note that the uncertainty due to is very small. In order to appreciate this result one can read off the plot in Fig. 3 that the old range of corresponds to .
Fig. 3

versus for . The violet range corresponds to the new lattice determination of in (4), and the yellow range displays the tree-level determination of (6)

versus for . The violet range corresponds to the new lattice determination of in (4), and the yellow range displays the tree-level determination of (6) Finally, from (16) and (25) we determine the angle in the unitarity triangleIt should be emphasised that the results in (16), (18), (21), (25) and (26) are independent of S(v) and therefore valid for all CMFV models.

: upper bounds on , , , and

Returning to (9) and (10), we note that the overall factors on the r.h.s. equal the central experimental values of and , respectively. We can therefore read off from these formulae the central values of and corresponding to the lattice results in (3). Including the uncertainties in the latter formula and taking into account the inequality (8) we find the maximal values of and in the CMFV models that are consistent with the data on and It should be noted thatwhere we suppressed the errors given in (27). Thus the bounds in (27) are saturated in the SM. The results within the SM are in excellent agreement with those obtained in [3]. Yet, here we also stress that these are upper bounds in CMFV models. Therefore, the tension between the values of these CKM elements extracted from and their tree-level determinations found in [3] within the SM is larger in any other CMFV model. Interestingly the values of and extracted from the rare semileptonic decays and agree with the ones in (28) and (12), respectively [49]:For , the values are found to be even smaller than in (28). However, this determination of CKM parameters still suffers from large uncertainties. We refer to [3] for a more detailed comparison of rare semileptonic B-decays with mixing results and the relevant references. With the knowledge of , , and we can determine and as functions of S(v) so that they can directly be compared with their determinations from semileptonic decays summarised in (22) and (23). We findThis dependence is represented by the red band in Fig. 4 with defined byFor illustrative purposes we also show the tree-level values in (22) and (23). Evidently the exclusive determinations of are favoured in . Furthermore with increasing , quickly drops significantly below the value in (22).
Fig. 4

versus the flavour-universal NP contribution obtained in (red) and (blue). The horizontal bands correspond to the tree-level measurements in (22) (yellow) and (23) (violet)

versus the flavour-universal NP contribution obtained in (red) and (blue). The horizontal bands correspond to the tree-level measurements in (22) (yellow) and (23) (violet) Having the full CKM matrix as a function of S(v), we can calculate the CP-violating parameter . We use the usual formulae, which can be found in [34]. It should be noted that depends directly onwith . Consequently, the value of is not needed for this evaluation. Now, the dominant contribution to is proportional towhere we have used (28). Thus with and determined through , the parameter decreases with increasing S(v), in contrast to the analysis in which the CKM parameters are taken from tree-level decays. In that case increases with increasing S(v). Consequently using we find the upper bound on in CMFV models to beWe conclude that the imposition of the constraints within CMFV models implies an upper bound on , saturated in the SM, which is significantly below its experimental value given in Table 1. Therefore a non-CMFV contributionis required, implying a discrepancy of the SM and CMFV value of with the data by . Once more we stress that this shift cannot be obtained within CMFV models without violating the constraints from . In Table 2 we collect the values of the most relevant CKM parameters as well as the real and imaginary parts of . In particular the value of is important for the ratio . Its value found in is lower than what has been used in the recent papers [50-53], thereby further decreasing the value of in the SM.

: lower bounds on

The strategy uses the construction of the UUT as outlined above, but then instead of using for the complete extraction of the CKM elements, the experimental value of is used as input. Taking the lower bound in (8) into account, this strategy again implies upper bounds on , , and . However, this time their S(v) dependence differs from the one in (28), as seen in the case of in Fig. 4, where is represented by the blue band. The weaker S(v) dependence in , together with the higher values, is another proof that the tension between and cannot be removed within the CMFV framework and is in fact smallest in the SM limit. In order to understand this weaker dependence of on S(v) we use the formula for extracted from , which has been derived in [34]. We recall it here for convenience1 where for the central values of the QCD corrections and in Table 1 one findsValues of and in the full range of and can be found in Table 3 of [34]. Inserting (36) into (14) we findand consequently from (9) and (10)Therefore, with (8), we find lower bounds on and that are significantly larger than the data,Consequently, our results for and in the SM differ from their experimental values by and , respectively. This difference increases for other CMFV models. On the other hand, as seen in Fig. 4, the value of in is fully compatible with its tree-level determination from inclusive decays, but for small larger than its exclusive determination. The ratio of the central values of obtained by usperfectly agrees with the data, as this ratio is used in and as experimental input in our analysis. The error on this ratio calculated directly from (40) is spurious as we impose this ratio from experiment and the true error is negligible. Only when one individually calculates and with extracted from , the errors in (40) are found. However, they are correlated and cancel in the ratio. On the other hand, using the tree-level determination of the CKM matrix, the authors of [3] find in the SMandCompared with (41), this shows the inconsistency between the tree-level determination of the CKM matrix and processes in CMFV models. In Table 2 we compare the results for the CKM elements obtained in with the ones found using . In both cases we use the SM value for S(v), as it allows to obtain values of in and of in closest to the data. But as we can see, the values of the CKM elements obtained in differ by much from the corresponding ones in , and in particular favour the inclusive determination of . Also the value of is larger, however, it differs only by a few percent from the one used in recent calculations of [50-53]. and obtained from the strategies and for , at which the upper bound on in and lower bound on in are obtained. The arrows show how the red and blue regions move with increasing S(v). The black dot represents the experimental values CMFV predictions for various quantities as functions of S(v) and . The four elements of the CKM matrix are in units of , and in MeV and in units of . From [34] We conclude therefore, as already indicated by the analysis in [34], that it is impossible within CMFV models to obtain a simultaneous agreement of and with the data. The improved lattice results in (3) and (4) allow one to exhibit this difficulty stronger. In the context of the strategies and , the tension between and is summarised by the plots of vs. in Fig. 5. Note that these plots differ from the known plots of vs. in CMFV models (see e.g. Fig. 5 in [2]). In the latter plot the CKM parameters were taken from tree-level decays, and varying S(v) increased both and in a correlated manner. Even if the physics in those plots and in the plots in Fig. 5 is the same, presently the accuracy of the outcome of strategies and shown in Fig. 5 is higher.
Fig. 5

and obtained from the strategies and for , at which the upper bound on in and lower bound on in are obtained. The arrows show how the red and blue regions move with increasing S(v). The black dot represents the experimental values

The problems with CMFV models encountered here could be anticipated on the basis of the first three rows of Table 2 from [34], which we recall in Table 3. In that paper a different strategy has been used and various quantities have been predicted in CMFV models as functions of S(v) and . As the first three columns correspond to and , very close to the values of these quantities found in the present paper, there is a clear message from Table 3. The predicted values of and are significantly below their recent values from [3] in (3). Moreover, with increasing S(v) there is a clear disagreement between the values of these parameters favoured by CMFV and the values in (3). We also refer to the plots in Fig. 4 of [34], where the correlations between and and between and implied by CMFV have been shown. Already in 2013 there was some tension between the grey regions in that figure representing the 2013 lattice values and the CMFV predictions. With the 2016 lattice values in (3), the grey areas shrunk and moved away from the values favoured by CMFV. Other problems of CMFV seen from the point of view of the strategy in [34] are listed in Sect. 3 of that paper.
Table 3

CMFV predictions for various quantities as functions of S(v) and . The four elements of the CKM matrix are in units of , and in MeV and in units of . From [34]

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Implications for rare K and B decays in the SM

In the previous section we have determined the full CKM matrix using in turn the strategies and . It is interesting to determine the impact of these new determinations on the branching ratios of the rare decays , and within the SM. To this end we use for and the parametric formulae derived in [54] which we recall here for completeness: For we use the formula from [55], slightly modified in [2] SM predictions for rare decay branching ratios using the strategies and , as explained in the text whereThe “bar” in (46) indicates that effects [56-58] have been taken into account throughFor one finds [55]whereIn Table 4 we collect the results for the four branching ratios in the SM obtained using the strategies and for the determination of the CKM parameters and other updated parameters collected in Table 1. We observe significant differences in these two determinations, which gives another support for the tension between and in the SM, holding more generally in CMFV models.
Table 4

SM predictions for rare decay branching ratios using the strategies and , as explained in the text

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Our results for should be compared with the results of the combined analysis of CMS and LHCb data [59]We observe that in the SM prediction for is rather close to the data, while in the case of it is visibly larger. Finally, in view of the improved lattice determinations of the parameters and [3]it is tempting to calculate the branching ratios by normalizing them to [60]. This eliminates not only the dependence on the CKM parameters and weak decay constants, but also reduces the dependence on . Neglecting the tiny uncertainties in , and we find the very accurate expressions These expressions apply only to the SM and , where the experimental values of are used to determine the CKM matrix. We then findThese results agree perfectly with the ones in Table 4. This is not surprising because in the constraint from has been imposed and the authors of [3] extracted the values of from their results in (3) and in Table 1. The outcome of this exercise will be more illuminating once independent and more precise lattice determinations of the parameters become available. In addition, the derived formulae (53) and (54) are much simpler than the ones in (46) and (49), respectively. They allow in no time to calculate the branching ratios in question in terms of , , and .

Beyond CMFV

Our analysis of CMFV models signals the violation of flavour universality in the function S(v), signalling the presence of new sources of flavour and CP-violation and/or new operators contributing to transitions beyond the SM ones.2 For simplicity we will here restrict ourselves to solutions in which only SM operators are present. A fully general and very convenient solution in this case is just to consider instead of the flavour-universal function S(v) three functionsIt is evident that with two free parameters in each meson system it is possible to obtain agreement with the data on observables. The simplest models of this type are models with tree-level and Z exchanges analysed in detail in [62]. The flavour violating couplings in these models are complex numbers (two free parameters) and can be chosen in such a manner that any problems of CMFV models in processes are removed by properly choosing these couplings. Effectively the observables in (1) are simply used to find these parameters or equivalently . The test of these scenarios is only offered through the correlations with processes, that is rare K or decays, which in these simple models involve the same couplings. The analysis in [62] then shows that when constraints from processes are taken into account it is easier to obtain agreement with the data for processes in the case of models than models with tree-level Z exchanges. Here we would like to discuss only the models with a minimally broken flavour symmetry [63, 64] which are more constrained. In these models, as discussed in detail in [65], in addition to the unitary CKM matrix one hasandwith being a real parameter which could be larger or smaller than unity. The important difference from the CMFV scenario is that it cannot be tested without invoking tree-level determinations of at least some elements of the CKM matrix. The main features of this scenario are:However, due to the equality there are two important implications that can be tested. No correlation between the K and systems, so that the tension between and is absent in these models. However, as , finding one day in the SM to be larger than the data would exclude this scenario. Presently such a situation seems rather unlikely. are complex functions and can be larger or smaller than unity. Consequently, through interference with the SM contributions, can be suppressed or enhanced as needed. With the new phase and not bounded from below there is more freedom than in the CMFV scenario. The first one is the CMFV relation [65]from which one can obtain the ratio as done already in Sect. 2, see (12), which can be compared with its tree-level determination. As stated before, the tree-level determination of this ratio, quoted in (13), is significantly larger, and consequently M models have the same difficulty here as CMFV models. Yet, a firm conclusion will only be reached after the result in (13) will be superseded by a more precise tree-level determination of the angle . The second one is the correlation between the two CP-asymmetries that results from the equality of NP phases inAs is very small in the SM, a precise measurement of determines . From the measured value of we then obtain . The latter value can be compared with the one obtained from the tree-level determination of and either or the tree-level determination of . However, is strongly correlated with , with very weak dependence on and . Therefore eventually (60) implies a triple correlation between [65]which provides another important test of the M scenario once the three observables will be known precisely. In summary, M models match the new lattice data better than CMFV, but similar to the latter models they have difficulties with the value of and of the ratio being significantly below their tree-level determinations. Concerning more complicated models like the Littlest Higgs model with T-parity [66, 67] or 331 models [68], it is clear that the new lattice data have an impact on the allowed ranges of new parameters. However, such a study is beyond the scope of our paper.

Conclusions

In this paper we have determined the Universal Unitarity Triangle (UUT) of constrained minimal flavour violation (CMFV) models. We then derived the full CKM matrix, using either the experimental value of or of as input. The recently improved values of the hadronic matrix elements in (3) and (4) [3] have been crucial for this study. In contrast to many analyses in the literature, we avoided tree-level determinations of and . The main messages from this analysis are as follows:Our analysis of CMFV models shows that they fail to properly describe the existing data on observables simultaneously and implies thereby the presence of either new sources of flavour violation and/or new operators. Several models analysed in the literature like models, 331 models, or the Littlest Higgs model with T-parity could help in bringing the theory to agree with the data. Firm conclusions would, however, require a dedicated study. The extracted angle in the UUT is already known precisely and is significantly smaller than its tree-level determination. This is a direct consequence of the small value of in (4). In turn the ratio also turns out to be smaller than its tree-level determination, as already pointed out in [3]. The precise relation between and obtained by us in (21) provides another test of CMFV. See Fig. 2. Requiring CMFV to reproduce the data for (strategy ), we find that low values of and are favoured, in agreement with their exclusive determinations. More importantly we derived an upper bound on that is significantly below the data. Requiring CMFV to reproduce the data for (strategy ), we find a higher value of , still consistent with exclusive determinations, but significantly higher than in and in agreement with its inclusive determination. The derived lower bounds on are then significantly above the data. The tension between and in CMFV models with either being too small or being too large cannot be removed by varying S(v). This would only be possible, as stressed in [34], if the values in (3) turned out to be significantly smaller and larger than in (4). With the present values of these parameters, the SM performs best among all CMFV models, even if, as seen in Fig. 5, it falls short in properly describing the data. The inconsistency of and in the SM and CMFV is also signalled by rather different predictions for rare decay branching ratios obtained using strategies and . See Sect. 3 and Table 4. As the correlation between and is broken in models with flavour symmetry, these models perform better than CMFV models. Still the correlation between and , that is of CMFV type, predicted by these models is in conflict with the tree-level determinations already pointed out in [3] within the SM. See (12) and (13). Certainly, further improvements on the hadronic matrix elements from lattice QCD and on the tree-level determinations of , and will sharpen the prediction for the size of required NP contributions to observables, thereby selecting models which could bring the theory to agree with experimental data. In particular finding the value of from tree-level determinations in the ballpark of would imply the violation of the CMFV relation (59). On the other hand, resolving the discrepancy between exclusive and inclusive tree-level determinations of in favour of the latter, would indicate the presence of new CP-violating phases affecting . Moreover, the correlations of transitions with rare K and decays and could eventually give us a deeper insight into the NP at short distance scales that is responsible for the anomalies indicated by the new lattice data, as reviewed in [2] and recently stressed in [53].
  11 in total

1.  Model-independent analysis of B-B-bar mixing and CP violation in B decays.

Authors: 
Journal:  Phys Rev D Part Fields       Date:  1996-06

2.  Next-to-next-to-leading-order charm-quark contribution to the CP violation parameter ϵ(K) and ΔM(K).

Authors:  Joachim Brod; Martin Gorbahn
Journal:  Phys Rev Lett       Date:  2012-03-19       Impact factor: 9.161

3.  Standard Model Prediction for Direct CP Violation in K→ππ Decay.

Authors:  Z Bai; T Blum; P A Boyle; N H Christ; J Frison; N Garron; T Izubuchi; C Jung; C Kelly; C Lehner; R D Mawhinney; C T Sachrajda; A Soni; D Zhang
Journal:  Phys Rev Lett       Date:  2015-11-17       Impact factor: 9.161

4.  B-meson decay constants from improved lattice nonrelativistic QCD with physical u, d, s, and c quarks.

Authors:  R J Dowdall; C T H Davies; R R Horgan; C J Monahan; J Shigemitsu
Journal:  Phys Rev Lett       Date:  2013-05-31       Impact factor: 9.161

5.  Observation of the rare B(s)(0) →µ+µ− decay from the combined analysis of CMS and LHCb data.

Authors: 
Journal:  Nature       Date:  2015-06-04       Impact factor: 49.962

6.  Precision determination of the Cabibbo-Kobayashi-Maskawa element V(cb).

Authors:  Andrea Alberti; Paolo Gambino; Kristopher J Healey; Soumitra Nandi
Journal:  Phys Rev Lett       Date:  2015-02-11       Impact factor: 9.161

7.  Probing new physics via the B(s)0→μ(+)μ- effective lifetime.

Authors:  Kristof De Bruyn; Robert Fleischer; Robert Knegjens; Patrick Koppenburg; Marcel Merk; Antonio Pellegrino; Niels Tuning
Journal:  Phys Rev Lett       Date:  2012-07-25       Impact factor: 9.161

8.  Towards the identification of new physics through quark flavour violating processes.

Authors:  Andrzej J Buras; Jennifer Girrbach
Journal:  Rep Prog Phys       Date:  2014-08-06

9.  B(s,d)→ℓ(+)ℓ(-) in the standard model with reduced theoretical uncertainty.

Authors:  Christoph Bobeth; Martin Gorbahn; Thomas Hermann; Mikołaj Misiak; Emmanuel Stamou; Matthias Steinhauser
Journal:  Phys Rev Lett       Date:  2014-03-11       Impact factor: 9.161

Review 10.  Review of lattice results concerning low-energy particle physics.

Authors:  S Aoki; Y Aoki; C Bernard; T Blum; G Colangelo; M Della Morte; S Dürr; A X El-Khadra; H Fukaya; R Horsley; A Jüttner; T Kaneko; J Laiho; L Lellouch; H Leutwyler; V Lubicz; E Lunghi; S Necco; T Onogi; C Pena; C T Sachrajda; S R Sharpe; S Simula; R Sommer; R S Van de Water; A Vladikas; U Wenger; H Wittig
Journal:  Eur Phys J C Part Fields       Date:  2014-09-17       Impact factor: 4.590

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