<?xml version='1.0'?>
<!DOCTYPE art SYSTEM 'http://www.biomedcentral.com/xml/article.dtd'>
<art>
   <ui>1754-0410-3-6</ui>
   <ji>1754-0410</ji>
   <fm>
      <dochead>Letter</dochead>
      <bibl>
         <title>
            <p>First evidence of new physics in <it>b </it>&#8596; <it>s </it>transitions</p>
         </title>
         <aug>
            <au id="A1">
               <snm>Bona</snm>
               <fnm>Marcella</fnm>
               <insr iid="I1"/>
               <email>Marcella.Bona@cern.ch</email>
            </au>
            <au id="A2">
               <snm>Ciuchini</snm>
               <fnm>Marco</fnm>
               <insr iid="I2"/>
               <email>ciuchini@roma3.infn.it</email>
            </au>
            <au id="A3">
               <snm>Franco</snm>
               <fnm>Enrico</fnm>
               <insr iid="I3"/>
               <email>Enrico.Franco@roma1.infn.it</email>
            </au>
            <au id="A4">
               <snm>Lubicz</snm>
               <fnm>Vittorio</fnm>
               <insr iid="I4"/>
               <insr iid="I2"/>
               <email>lubicz@fis.uniroma3.it</email>
            </au>
            <au id="A5">
               <snm>Martinelli</snm>
               <fnm>Guido</fnm>
               <insr iid="I5"/>
               <insr iid="I3"/>
               <email>Guido.Martinelli@roma1.infn.it</email>
            </au>
            <au id="A6">
               <snm>Parodi</snm>
               <fnm>Fabrizio</fnm>
               <insr iid="I6"/>
               <email>fabrizio.parodi@ge.infn.it</email>
            </au>
            <au id="A7">
               <snm>Pierini</snm>
               <fnm>Maurizio</fnm>
               <insr iid="I1"/>
               <email>Maurizio.Pierini@cern.ch</email>
            </au>
            <au id="A8">
               <snm>Schiavi</snm>
               <fnm>Carlo</fnm>
               <insr iid="I6"/>
               <email>Carlo.Schiavi@cern.ch</email>
            </au>
            <au ca="yes" id="A9">
               <snm>Silvestrini</snm>
               <fnm>Luca</fnm>
               <insr iid="I3"/>
               <email>Luca.Silvestrini@roma1.infn.it</email>
            </au>
            <au id="A10">
               <snm>Sordini</snm>
               <fnm>Viola</fnm>
               <insr iid="I7"/>
               <email>Viola.Sordini@roma1.infn.it</email>
            </au>
            <au id="A11">
               <snm>Stocchi</snm>
               <fnm>Achille</fnm>
               <insr iid="I8"/>
               <email>stocchi@lal.in2p3.fr</email>
            </au>
            <au id="A12">
               <snm>Vagnoni</snm>
               <fnm>Vincenzo</fnm>
               <insr iid="I9"/>
               <email>Vincenzo.Vagnoni@bo.infn.it</email>
            </au>
         </aug>
         <insg>
            <ins id="I1">
               <p>CERN, CH-1211 Geneva 23, Switzerland</p>
            </ins>
            <ins id="I2">
               <p>INFN, Sezione di Roma Tre, I-00146 Roma, Italy</p>
            </ins>
            <ins id="I3">
               <p>INFN, Sezione di Roma, I-00185 Roma, Italy</p>
            </ins>
            <ins id="I4">
               <p>Dipartimento di Fisica, Universit&#224; di Roma Tre, I-00146 Roma, Italy</p>
            </ins>
            <ins id="I5">
               <p>Dipartimento di Fisica, Universit&#224; di Roma "La Sapienza", I-00185 Roma, Italy</p>
            </ins>
            <ins id="I6">
               <p>Dipartimento di Fisica, Universit&#224; di Genova and INFN, I-16146 Genova, Italy</p>
            </ins>
            <ins id="I7">
               <p>ETH Zurich, HG Raemistrasse 101, 8092 Zurich, Switzerland</p>
            </ins>
            <ins id="I8">
               <p>Laboratoire de l'Acc&#233;l&#233;rateur Lin&#233;aire, IN2P3-CNRS et Universit&#233; de Paris-Sud, BP 34, F-91898 Orsay Cedex, France</p>
            </ins>
            <ins id="I9">
               <p>INFN, Sezione di Bologna, I-40126 Bologna, Italy</p>
            </ins>
         </insg>
         <source>PMC Physics A</source>
         <issn>1754-0410</issn>
         <pubdate>2009</pubdate>
         <volume>3</volume>
         <issue>1</issue>
         <fpage>6</fpage>
         <url>http://www.physmathcentral.com/1754-0410/3/6</url>
         <xrefbib>
            <pubid idtype="doi">10.1186/1754-0410-3-6</pubid>
         </xrefbib>
      </bibl>
      <history>
         <rec>
            <date>
               <day>7</day>
               <month>9</month>
               <year>2009</year>
            </date>
         </rec>
         <acc>
            <date>
               <day>18</day>
               <month>12</month>
               <year>2009</year>
            </date>
         </acc>
         <pub>
            <date>
               <day>18</day>
               <month>12</month>
               <year>2009</year>
            </date>
         </pub>
      </history>
      <cpyrt>
         <year>2009</year>
         <collab>Silvestrini et al</collab>
         <note>This is an Open Access article distributed under the terms of the Creative Commons Attribution License (<url>http://creativecommons.org/licenses/by/2.0</url>), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.</note>
      </cpyrt>
      <abs>
         <sec>
            <st>
               <p>Abstract</p>
            </st>
            <p>We combine all the available experimental information on <it>B</it><sub><it>s </it></sub>mixing, including the very recent tagged analyses of <it>B</it><sub><it>s </it></sub>&#8594; <it>J</it>/&#936;<it>&#981; </it>by the CDF and D&#216; collaborations. We find that the phase of the <it>B</it><sub><it>s </it></sub>mixing amplitude deviates more than 3<it>&#963; </it>from the Standard Model prediction. While no single measurement has a 3<it>&#963; </it>significance yet, all the constraints show a remarkable agreement with the combined result. This is a first evidence of physics beyond the Standard Model. This result disfavours New Physics models with Minimal Flavour Violation with the same significance.</p>
            <p><b>PACS Codes</b>: 12.15.Ff, 12.15.Hh, 14.40.Nb</p>
         </sec>
      </abs>
   </fm>
   <bdy>
      <sec>
         <st>
            <p>1. Letter</p>
         </st>
         <p>In the Standard Model (SM), all flavour and CP violating phenomena in weak decays are described in terms of quark masses and the four independent parameters in the Cabibbo-Kobayashi-Maskawa (CKM) matrix <abbrgrp><abbr bid="B1">1</abbr><abbr bid="B2">2</abbr></abbrgrp>. In particular, there is only one source of CP violation, which is connected to the area of the Unitarity Triangle (UT). A peculiar prediction of the SM, due to the hierarchy among CKM matrix elements, is that CP violation in <it>B</it><sub><it>s </it></sub>mixing should be tiny. This property is also valid in models of Minimal Flavour Violation (MFV) <abbrgrp><abbr bid="B3">3</abbr><abbr bid="B4">4</abbr><abbr bid="B5">5</abbr><abbr bid="B6">6</abbr><abbr bid="B7">7</abbr><abbr bid="B8">8</abbr></abbrgrp>, where flavour and CP violation are still governed by the CKM matrix. Therefore, the experimental observation of sizable CP violation in <it>B</it><sub><it>s </it></sub>mixing is a clear (and clean) signal of New Physics (NP) and a violation of the MFV paradigm. In the past decade, <it>B </it>factories have collected an impressive amount of data on <it>B</it><sub><it>d </it></sub>flavour- and CP-violating processes. The CKM paradigm has passed unscathed all the tests performed at the <it>B </it>factories down to an accuracy just below 10% <abbrgrp><abbr bid="B9">9</abbr><abbr bid="B10">10</abbr><abbr bid="B11">11</abbr></abbrgrp>. This has been often considered as an indication pointing to the MFV hypothesis, which has received considerable attention in recent years. The only possible hint of non-MFV NP is found in the penguin-dominated <it>b </it>&#8594; <it>s </it>non-leptonic decays. Indeed, in the SM, the <inline-formula><graphic file="1754-0410-3-6-i1.gif"/></inline-formula> coefficient of the time-dependent CP asymmetry in these channels is equal to the <inline-formula><graphic file="1754-0410-3-6-i2.gif"/></inline-formula> measured with <it>b </it>&#8594; <inline-formula><graphic file="1754-0410-3-6-i3.gif"/></inline-formula> decays, up to hadronic uncertainties related to subleading terms in the decay amplitudes. Present data show a systematic, although not statistically significant, downward shift of <inline-formula><graphic file="1754-0410-3-6-i1.gif"/></inline-formula> with respect to <inline-formula><graphic file="1754-0410-3-6-i2.gif"/></inline-formula><abbrgrp><abbr bid="B12">12</abbr><abbr bid="B13">13</abbr><abbr bid="B14">14</abbr><abbr bid="B15">15</abbr><abbr bid="B16">16</abbr><abbr bid="B17">17</abbr><abbr bid="B18">18</abbr><abbr bid="B19">19</abbr><abbr bid="B20">20</abbr><abbr bid="B21">21</abbr></abbrgrp>, while hadronic models predict a shift in the opposite direction in many cases <abbrgrp><abbr bid="B22">22</abbr><abbr bid="B23">23</abbr><abbr bid="B24">24</abbr><abbr bid="B25">25</abbr><abbr bid="B26">26</abbr><abbr bid="B27">27</abbr><abbr bid="B28">28</abbr><abbr bid="B29">29</abbr></abbrgrp>.</p>
         <p>From the theoretical point of view, the hierarchical structure of quark masses and mixing angles of the SM calls for an explanation in terms of flavour symmetries or of other dynamical mechanisms, such as, for example, fermion localization in models with extra dimensions. All such explanations depart from the MFV paradigm, and generically cause deviations from the SM in flavour violating processes. Models with localized fermions <abbrgrp><abbr bid="B30">30</abbr><abbr bid="B31">31</abbr><abbr bid="B32">32</abbr></abbrgrp>, and more generally models of Next-to-Minimal Flavour Violation <abbrgrp><abbr bid="B33">33</abbr></abbrgrp>, tend to produce too large effects in <it>&#949;</it><sub><it>K </it></sub><abbrgrp><abbr bid="B34">34</abbr><abbr bid="B35">35</abbr></abbrgrp>. On the contrary, flavour models based on nonabelian flavour symmetries, such as <it>U</it>(2) or <it>SU</it>(3), typically suppress NP contributions to <it>s </it>&#8596; <it>d </it>and possibly also to <it>b </it>&#8596; <it>d </it>transitions, but easily produce large NP contributions to <it>b </it>&#8596; <it>s </it>processes. This is due to the large flavour symmetry breaking caused by the top quark Yukawa coupling. Thus, if (nonabelian) flavour symmetry models are relevant for the solution of the SM flavour problem, one expects on general grounds NP contributions to <it>b </it>&#8596; <it>s </it>transitions. On the other hand, in the context of Grand Unified Theories (GUTs), there is a connection between leptonic and hadronic flavour violation. In particular, in a broad class of GUTs, the large mixing angle observed in neutrino oscillations corresponds to large NP contributions to <it>b </it>&#8596; <it>s </it>transitions <abbrgrp><abbr bid="B36">36</abbr><abbr bid="B37">37</abbr><abbr bid="B38">38</abbr><abbr bid="B39">39</abbr></abbrgrp>.</p>
         <p>In this Letter, we show that present data give evidence of a <it>B</it><sub><it>s </it></sub>mixing phase much larger than expected in the SM, with a significance of more than 3<it>&#963;</it>. This result is obtained by combining all available experimental information with the method used by our collaboration for UT analyses and described in Ref. <abbrgrp><abbr bid="B40">40</abbr></abbrgrp>.</p>
         <p>We perform a model-independent analysis of NP contributions to <it>B</it><sub><it>s </it></sub>mixing using the following parametrization <abbrgrp><abbr bid="B41">41</abbr><abbr bid="B42">42</abbr><abbr bid="B43">43</abbr><abbr bid="B44">44</abbr><abbr bid="B45">45</abbr><abbr bid="B46">46</abbr></abbrgrp>:</p>
         <p>
            <display-formula id="M1">
               <graphic file="1754-0410-3-6-i4.gif"/>
            </display-formula>
         </p>
         <p>where <inline-formula><graphic file="1754-0410-3-6-i5.gif"/></inline-formula> is the effective Hamiltonian generated by both SM and NP, while <inline-formula><graphic file="1754-0410-3-6-i6.gif"/></inline-formula> only contains SM contributions. The angle <it>&#946;</it><sub><it>s </it></sub>is defined as <inline-formula><graphic file="1754-0410-3-6-i7.gif"/></inline-formula> and it equals 0.018 &#177; 0.001 in the SM (we are using the usual CKM phase convention in which <inline-formula><graphic file="1754-0410-3-6-i8.gif"/></inline-formula> is real to a very good approximation).</p>
         <p>We use the following experimental input: the CDF measurement of &#916;<it>m</it><sub><it>s </it></sub><abbrgrp><abbr bid="B47">47</abbr></abbrgrp>, the semileptonic asymmetry in <it>B</it><sub><it>s </it></sub>decays <inline-formula><graphic file="1754-0410-3-6-i9.gif"/></inline-formula><abbrgrp><abbr bid="B48">48</abbr></abbrgrp>, the dimuon charge asymmetry <inline-formula><graphic file="1754-0410-3-6-i10.gif"/></inline-formula> from D&#216; <abbrgrp><abbr bid="B49">49</abbr></abbrgrp> and CDF <abbrgrp><abbr bid="B50">50</abbr></abbrgrp>, the measurement of the <it>B</it><sub><it>s </it></sub>lifetime from flavour-specific final states <abbrgrp><abbr bid="B51">51</abbr><abbr bid="B52">52</abbr><abbr bid="B53">53</abbr><abbr bid="B54">54</abbr><abbr bid="B55">55</abbr><abbr bid="B56">56</abbr><abbr bid="B57">57</abbr><abbr bid="B58">58</abbr><abbr bid="B59">59</abbr></abbrgrp>, the two-dimensional likelihood ratio for &#916;&#915;<sub><it>s </it></sub>and &#981;<sub><it>s </it></sub>= 2(<it>&#946;</it><sub><it>s </it></sub>- <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula>) from the time-dependent tagged angular analysis of <it>B</it><sub><it>s </it></sub>&#8594; <it>J</it>/<it>&#968;&#981; </it>decays by CDF <abbrgrp><abbr bid="B60">60</abbr></abbrgrp> and the correlated constraints on &#915;<sub><it>s</it></sub>, &#916;&#915;<sub><it>s </it></sub>and <it>&#981;</it><sub><it>s </it></sub>from the same analysis performed by D&#216; <abbrgrp><abbr bid="B61">61</abbr></abbrgrp>. For the latter, since the complete likelihood is not available yet, we start from the results of the 7-variable fit in the free-<it>&#981;</it><sub><it>s </it></sub>case from Table one of ref. <abbrgrp><abbr bid="B61">61</abbr></abbrgrp>. We implement the 7 &#215; 7 correlation matrix and integrate over the strong phases and decay amplitudes to obtain the reduced 3 &#215; 3 correlation matrix used in our analysis. In the D&#216; analysis, the twofold ambiguity inherent in the measurement (&#981;<sub><it>s </it></sub>&#8594; <it>&#960; </it>- <it>&#981;</it><sub><it>s</it></sub>, &#916;&#915;<sub><it>s </it></sub>&#8594; - &#916;&#915;<sub><it>s</it></sub>, cos <it>&#948;</it><sub>1,2 </sub>&#8594; - cos <it>&#948;</it><sub>1,2</sub>) for arbitrary strong phases was removed using a value for cos <it>&#948;</it><sub>1,2 </sub>derived from the BaBar analysis of <it>B</it><sub><it>d </it></sub>&#8594; <it>J</it>/&#936;<it>K</it>* using SU(3). However, the strong phases in <it>B</it><sub><it>d </it></sub>&#8594; <it>J</it>/&#936;<it>K</it>* and <it>B</it><sub><it>s </it></sub>&#8594; <it>J</it>/&#936;<it>&#981; </it>cannot be exactly related in the SU(3) limit due to the singlet component of <it>&#981;</it>. Although the sign of cos <it>&#948;</it><sub>1,2 </sub>obtained using SU(3) is consistent with the factorization estimate, to be conservative we reintroduce the ambiguity in the D&#216; measurement. To this end, we take the errors quoted by D&#216; as Gaussian and duplicate the likelihood at the point obtained by applying the discrete ambiguity. Indeed, looking at Fig. 2 of ref. <abbrgrp><abbr bid="B61">61</abbr></abbrgrp>, this seems a reasonable procedure. Hopefully D&#216; will present results without assumptions on the strong phases in the future, allowing for a more straightforward combination. Finally, for the CKM parameters we perform the UT analysis in the presence of arbitrary NP as described in ref. <abbrgrp><abbr bid="B34">34</abbr></abbrgrp>, obtaining <inline-formula><graphic file="1754-0410-3-6-i12.gif"/></inline-formula> = 0.140 &#177; 0.046, <inline-formula><graphic file="1754-0410-3-6-i13.gif"/></inline-formula> = 0.384 &#177; 0.035 and sin 2<it>&#946;</it><sub><it>s </it></sub>= 0.0409 &#177; 0.0038. The new input parameters used in our analysis are summarized in Table <tblr tid="T1">1</tblr>, all the others are given in Ref. <abbrgrp><abbr bid="B34">34</abbr></abbrgrp>. The relevant NLO formulae for &#916;&#915;<sub><it>s </it></sub>and for the semileptonic asymmetries in the presence of NP have been already discussed in refs. <abbrgrp><abbr bid="B34">34</abbr><abbr bid="B62">62</abbr><abbr bid="B63">63</abbr></abbrgrp>.</p>
         <tbl id="T1">
            <title>
               <p>Table 1</p>
            </title>
            <caption>
               <p>Input parameters used in the analysis.</p>
            </caption>
            <tblbdy cols="3">
               <r>
                  <c ca="center">
                     <p>&#916;<it>m</it><sub><it>s </it></sub>[ps<sup>-1</sup>]</p>
                  </c>
                  <c ca="center">
                     <p>17.77 &#177; 0.12</p>
                  </c>
                  <c ca="center">
                     <p>
                        <abbrgrp>
                           <abbr bid="B47">47</abbr>
                        </abbrgrp>
                     </p>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p><inline-formula><graphic file="1754-0410-3-6-i9.gif"/></inline-formula> &#215; 10<sup>2</sup></p>
                  </c>
                  <c ca="center">
                     <p>2.45 &#177; 1.96</p>
                  </c>
                  <c ca="center">
                     <p>
                        <abbrgrp>
                           <abbr bid="B48">48</abbr>
                        </abbrgrp>
                     </p>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p><inline-formula><graphic file="1754-0410-3-6-i10.gif"/></inline-formula> &#215; 10<sup>3</sup></p>
                  </c>
                  <c ca="center">
                     <p>-4.3 &#177; 3.0</p>
                  </c>
                  <c ca="center">
                     <p>
                        <abbrgrp>
                           <abbr bid="B49">49</abbr>
                           <abbr bid="B50">50</abbr>
                        </abbrgrp>
                     </p>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p><inline-formula><graphic file="1754-0410-3-6-i14.gif"/></inline-formula> [ps]</p>
                  </c>
                  <c ca="center">
                     <p>1.461 &#177; 0.032</p>
                  </c>
                  <c ca="center">
                     <p>
                        <abbrgrp>
                           <abbr bid="B51">51</abbr>
                           <abbr bid="B52">52</abbr>
                           <abbr bid="B53">53</abbr>
                           <abbr bid="B54">54</abbr>
                           <abbr bid="B55">55</abbr>
                           <abbr bid="B56">56</abbr>
                           <abbr bid="B57">57</abbr>
                           <abbr bid="B58">58</abbr>
                           <abbr bid="B59">59</abbr>
                        </abbrgrp>
                     </p>
                  </c>
               </r>
               <r>
                  <c cspan="3">
                     <hr/>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p>
                        <it>&#981;</it>
                        <sub>
                           <it>s</it>
                        </sub>
                     </p>
                  </c>
                  <c ca="center">
                     <p>see ref. <abbrgrp><abbr bid="B60">60</abbr></abbrgrp></p>
                  </c>
                  <c ca="center">
                     <p>
                        <abbrgrp>
                           <abbr bid="B60">60</abbr>
                        </abbrgrp>
                     </p>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p>&#916;&#915;<sub><it>s</it></sub></p>
                  </c>
                  <c ca="center">
                     <p>see ref. <abbrgrp><abbr bid="B60">60</abbr></abbrgrp></p>
                  </c>
                  <c ca="center">
                     <p>
                        <abbrgrp>
                           <abbr bid="B60">60</abbr>
                        </abbrgrp>
                     </p>
                  </c>
               </r>
               <r>
                  <c cspan="3">
                     <hr/>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p><it>&#981;</it><sub><it>s </it></sub>[rad]</p>
                  </c>
                  <c ca="center">
                     <p>0.60 &#177; 0.27</p>
                  </c>
                  <c ca="center">
                     <p>
                        <abbrgrp>
                           <abbr bid="B61">61</abbr>
                        </abbrgrp>
                     </p>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p>&#916;&#915;<sub><it>s </it></sub>[ps<sup>-1</sup>]</p>
                  </c>
                  <c ca="center">
                     <p>0.19 &#177; 0.07</p>
                  </c>
                  <c ca="center">
                     <p>
                        <abbrgrp>
                           <abbr bid="B61">61</abbr>
                        </abbrgrp>
                     </p>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p><inline-formula><graphic file="1754-0410-3-6-i15.gif"/></inline-formula>[ps]</p>
                  </c>
                  <c ca="center">
                     <p>1.52 &#177; 0.06</p>
                  </c>
                  <c ca="center">
                     <p>
                        <abbrgrp>
                           <abbr bid="B61">61</abbr>
                        </abbrgrp>
                     </p>
                  </c>
               </r>
               <r>
                  <c cspan="3" ca="center">
                     <p><inline-formula><graphic file="1754-0410-3-6-i16.gif"/></inline-formula> = -0.042 <inline-formula><graphic file="1754-0410-3-6-i17.gif"/></inline-formula> = -0.571 <inline-formula><graphic file="1754-0410-3-6-i18.gif"/></inline-formula> = 0.23</p>
                  </c>
               </r>
            </tblbdy>
            <tblfn>
               <p>We also show the correlation coefficients <it>C</it>s of the measurements of <it>&#981;</it><sub><it>s</it></sub>, &#916;&#915;<sub><it>s </it></sub>and <inline-formula><graphic file="1754-0410-3-6-i15.gif"/></inline-formula> from ref. <abbrgrp><abbr bid="B61">61</abbr></abbrgrp>.</p>
            </tblfn>
         </tbl>
         <p>The results of our analysis are summarized in Table <tblr tid="T2">2</tblr>. We see that the phase <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula> deviates from zero at 3.7<it>&#963;</it>. We comment below on the stability of this significance. In Fig. <figr fid="F1">1</figr> we present the two-dimensional 68% and 95% probability regions for the NP parameters <inline-formula><graphic file="1754-0410-3-6-i19.gif"/></inline-formula> and <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula>, the corresponding regions for the parameters <inline-formula><graphic file="1754-0410-3-6-i20.gif"/></inline-formula> and <inline-formula><graphic file="1754-0410-3-6-i21.gif"/></inline-formula>, and the one-dimensional distributions for NP parameters. Notice that the ambiguity of the tagged analysis of <it>B</it><sub><it>s </it></sub>&#8594; <it>J</it>/&#936;<it>&#981; </it>is slightly broken by the presence of the CKM-subleading terms in the expression of &#915;<sub>12</sub>/<it>M</it><sub>12 </sub>(see for example eq. (5) of ref. <abbrgrp><abbr bid="B63">63</abbr></abbrgrp>). The solution around <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula> ~ -20&#176; corresponds to <inline-formula><graphic file="1754-0410-3-6-i21.gif"/></inline-formula> ~ -50&#176; and <inline-formula><graphic file="1754-0410-3-6-i20.gif"/></inline-formula> ~ 75%. The second solution is much more distant from the SM and it requires a dominant NP contribution (<inline-formula><graphic file="1754-0410-3-6-i20.gif"/></inline-formula> ~ 190%). In this case the NP phase is thus very well determined. The strong phase ambiguity affects the sign of cos <it>&#981;</it><sub><it>s </it></sub>and thus Re <inline-formula><graphic file="1754-0410-3-6-i20.gif"/></inline-formula>, while Im <inline-formula><graphic file="1754-0410-3-6-i20.gif"/></inline-formula> ~ - 0.74 in any case.</p>
         <fig id="F1">
            <title>
               <p>Figure 1</p>
            </title>
            <caption>
               <p>From left to right and from top to bottom, 68% (dark) and 95% (light) probability regions in the <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula> - <inline-formula><graphic file="1754-0410-3-6-i9.gif"/></inline-formula>, <inline-formula><graphic file="1754-0410-3-6-i20.gif"/></inline-formula> - <inline-formula><graphic file="1754-0410-3-6-i21.gif"/></inline-formula> planes and p.d.f for <inline-formula><graphic file="1754-0410-3-6-i19.gif"/></inline-formula>, <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula>, <inline-formula><graphic file="1754-0410-3-6-i20.gif"/></inline-formula>, <inline-formula><graphic file="1754-0410-3-6-i21.gif"/></inline-formula>, Re <inline-formula><graphic file="1754-0410-3-6-i20.gif"/></inline-formula>, Im <inline-formula><graphic file="1754-0410-3-6-i20.gif"/></inline-formula></p>
            </caption>
            <text>
               <p><b>From left to right and from top to bottom, 68% (dark) and 95% (light) probability regions in the <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula> - <inline-formula><graphic file="1754-0410-3-6-i9.gif"/></inline-formula>, <inline-formula><graphic file="1754-0410-3-6-i20.gif"/></inline-formula> - <inline-formula><graphic file="1754-0410-3-6-i21.gif"/></inline-formula> planes and p.d.f for <inline-formula><graphic file="1754-0410-3-6-i19.gif"/></inline-formula>, <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula>, <inline-formula><graphic file="1754-0410-3-6-i20.gif"/></inline-formula>, <inline-formula><graphic file="1754-0410-3-6-i21.gif"/></inline-formula>, Re <inline-formula><graphic file="1754-0410-3-6-i20.gif"/></inline-formula>, Im <inline-formula><graphic file="1754-0410-3-6-i20.gif"/></inline-formula></b>.</p>
            </text>
            <graphic file="1754-0410-3-6-1"/>
         </fig>
         <tbl id="T2">
            <title>
               <p>Table 2</p>
            </title>
            <caption>
               <p>Fit results for NP parameters, semileptonic asymmetries and width differences.</p>
            </caption>
            <tblbdy cols="3">
               <r>
                  <c ca="center">
                     <p>
                        <b>Observable</b>
                     </p>
                  </c>
                  <c ca="center">
                     <p>
                        <b>68% Prob.</b>
                     </p>
                  </c>
                  <c ca="center">
                     <p>
                        <b>95% Prob.</b>
                     </p>
                  </c>
               </r>
               <r>
                  <c cspan="3">
                     <hr/>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p><inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula>[&#176;]</p>
                  </c>
                  <c ca="center">
                     <p>-19.9 &#177; 5.6</p>
                  </c>
                  <c ca="center">
                     <p>[-30.45,-9.29]</p>
                  </c>
               </r>
               <r>
                  <c>
                     <p/>
                  </c>
                  <c ca="center">
                     <p>-68.2 &#177; 4.9</p>
                  </c>
                  <c ca="center">
                     <p>[-78.45,-58.2]</p>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p>
                        <inline-formula>
                           <graphic file="1754-0410-3-6-i19.gif"/>
                        </inline-formula>
                     </p>
                  </c>
                  <c ca="center">
                     <p>1.07 &#177; 0.29</p>
                  </c>
                  <c ca="center">
                     <p>[0.62,1.93]</p>
                  </c>
               </r>
               <r>
                  <c cspan="3">
                     <hr/>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p><inline-formula><graphic file="1754-0410-3-6-i21.gif"/></inline-formula>[&#176;]</p>
                  </c>
                  <c ca="center">
                     <p>-51 &#177; 11</p>
                  </c>
                  <c ca="center">
                     <p>[-69,-27]</p>
                  </c>
               </r>
               <r>
                  <c>
                     <p/>
                  </c>
                  <c ca="center">
                     <p>-79 &#177; 3</p>
                  </c>
                  <c ca="center">
                     <p>[-84,-71]</p>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p>
                        <inline-formula>
                           <graphic file="1754-0410-3-6-i20.gif"/>
                        </inline-formula>
                     </p>
                  </c>
                  <c ca="center">
                     <p>0.73 &#177; 0.35</p>
                  </c>
                  <c ca="center">
                     <p>[0.24,1.38]</p>
                  </c>
               </r>
               <r>
                  <c>
                     <p/>
                  </c>
                  <c ca="center">
                     <p>1.87 &#177; 0.06</p>
                  </c>
                  <c ca="center">
                     <p>[1.50,2.47]</p>
                  </c>
               </r>
               <r>
                  <c cspan="3">
                     <hr/>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p>Im <inline-formula><graphic file="1754-0410-3-6-i20.gif"/></inline-formula></p>
                  </c>
                  <c ca="center">
                     <p>-0.74 &#177; 0.26</p>
                  </c>
                  <c ca="center">
                     <p>[-1.54,-0.30]</p>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p>Re <inline-formula><graphic file="1754-0410-3-6-i20.gif"/></inline-formula></p>
                  </c>
                  <c ca="center">
                     <p>-0.13 &#177; 0.31</p>
                  </c>
                  <c ca="center">
                     <p>[-0.61,0.78]</p>
                  </c>
               </r>
               <r>
                  <c>
                     <p/>
                  </c>
                  <c ca="center">
                     <p>-1.82 &#177; 0.28</p>
                  </c>
                  <c ca="center">
                     <p>[-2.68,-1.36]</p>
                  </c>
               </r>
               <r>
                  <c cspan="3">
                     <hr/>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p><inline-formula><graphic file="1754-0410-3-6-i9.gif"/></inline-formula> &#215; 10<sup>2</sup></p>
                  </c>
                  <c ca="center">
                     <p>-0.34 &#177; 0.21</p>
                  </c>
                  <c ca="center">
                     <p>[-0.75,0.03]</p>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p><inline-formula><graphic file="1754-0410-3-6-i10.gif"/></inline-formula> &#215; 10<sup>3</sup></p>
                  </c>
                  <c ca="center">
                     <p>-2.1 &#177; 1.0</p>
                  </c>
                  <c ca="center">
                     <p>[-4.7,-0.3]</p>
                  </c>
               </r>
               <r>
                  <c ca="center">
                     <p>&#916;&#915;<sub><it>s</it></sub>/&#915;<sub><it>s</it></sub></p>
                  </c>
                  <c ca="center">
                     <p>0.105 &#177; 0.049</p>
                  </c>
                  <c ca="center">
                     <p>[0.02,0.20]</p>
                  </c>
               </r>
               <r>
                  <c>
                     <p/>
                  </c>
                  <c ca="center">
                     <p>-0.098 &#177; 0.044</p>
                  </c>
                  <c ca="center">
                     <p>[-0.19,-0.02]</p>
                  </c>
               </r>
            </tblbdy>
            <tblfn>
               <p>Whenever present, we list the two solutions due to the ambiguity of the measurements. The first line corresponds to the one closer to the SM.</p>
            </tblfn>
         </tbl>
         <p>Before concluding, we comment on our treatment of the D&#216; result for the tagged analysis and on the stability of the NP fit. Clearly, the procedure to reintroduce the strong phase ambiguity in the D&#216; result and to combine it with CDF is not unique given the available information. In particular, the Gaussian assumption can be questioned, given the likelihood profiles shown in Ref. <abbrgrp><abbr bid="B61">61</abbr></abbrgrp>. Thus, we have tested the significance of the NP signal against different modeling of the probability density function (p.d.f.). First, we have used the 90% C.L. range for <it>&#981;</it><sub><it>s </it></sub>= [-0.06, 1.20]&#176; given by D&#216; to estimate the standard deviation, obtaining <it>&#981;</it><sub><it>s </it></sub>= (0.57 &#177; 0.38)&#176; as input for our Gaussian analysis. This is conservative since the likelihood has a visibly larger half-width on the side opposite to the SM expectation (see Fig. 2 of Ref. <abbrgrp><abbr bid="B61">61</abbr></abbrgrp>). Second, we have implemented the likelihood profiles for <it>&#981;</it><sub><it>s </it></sub>and &#916;&#915;<sub><it>s </it></sub>given by D&#216;, discarding the correlations but restoring the strong phase ambiguity. The likelihood profiles include the second minimum corresponding to <it>&#981;</it><sub><it>s </it></sub>&#8594; <it>&#981;</it><sub><it>s</it></sub>+<it>&#960;</it>, &#916;&#915; &#8594; -&#916;&#915;, which is disfavoured by the oscillating terms present in the tagged analysis and is discarded in our Gaussian analysis. Also this approach is conservative since each one-dimensional profile likelihood is minimized with respect to the other variables relevant for our analysis. It is remarkable that both methods give a deviation of <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula> from zero of 3 <it>&#963; </it>(the 3 <it>&#963; </it>ranges for <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula> are [-88, -48]&#176; &#8746; [-41, 0]&#176; and [-88, 0]&#176; for the two methods respectively). We conclude that the combined analysis gives a stable evidence for NP, although the precise number of standard deviations depends on the procedure followed to combine presently available data.</p>
         <p>To illustrate the impact of the experimental constraints, we show in Fig. <figr fid="F2">2</figr> the p.d.f. for <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula> obtained without the tagged analysis of <it>B</it><sub><it>s </it></sub>&#8594; <it>J</it>/&#936;<it>&#981; </it>or including only CDF or D&#216; results. Including only the CDF tagged analysis, we obtain <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula> &lt; 0 at 97.7% probability (2.3<it>&#963;</it>). For D&#216;, we show results obtained with the Gaussian and likelihood profile treatment of the errors. In the Gaussian case, the D&#216; tagged analysis gives <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula> &lt; 0 at 98.0% probability (2.3<it>&#963;</it>), while using the likelihood profiles <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula> &lt; 0 at 92.8% probability (1.8<it>&#963;</it>). Finally, it is remarkable that the different constraints in Fig. <figr fid="F2">2</figr> are all consistent among themselves and with the combined result. We notice, however, that the top-left plot is dominated by the measurement of <inline-formula><graphic file="1754-0410-3-6-i10.gif"/></inline-formula> while <inline-formula><graphic file="1754-0410-3-6-i9.gif"/></inline-formula> favours positive <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula>, although with a very low significance. For completeness, in Table <tblr tid="T2">2</tblr> we also quote the fit results for <inline-formula><graphic file="1754-0410-3-6-i9.gif"/></inline-formula>, <inline-formula><graphic file="1754-0410-3-6-i10.gif"/></inline-formula> and for &#916;&#915;<sub><it>s</it></sub>/&#915;<sub><it>s</it></sub>.</p>
         <fig id="F2">
            <title>
               <p>Figure 2</p>
            </title>
            <caption>
               <p>From left to right: P.d.f. for <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula> without the tagged analysis of <it>B</it><sub><it>s </it></sub>&#8594; <it>J</it>/&#936;<it>&#981;</it>, including only the CDF analysis, including only the D&#216; Gaussian analysis, including only the D&#216; likelihood profiles. We show 68% (dark) and 95% (light) probability regions</p>
            </caption>
            <text>
               <p><b>From left to right: P.d.f. for <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula> without the tagged analysis of <it>B</it><sub><it>s </it></sub>&#8594; <it>J</it>/&#936;<it>&#981;</it>, including only the CDF analysis, including only the D&#216; Gaussian analysis, including only the D&#216; likelihood profiles. We show 68% (dark) and 95% (light) probability regions</b>.</p>
            </text>
            <graphic file="1754-0410-3-6-2"/>
         </fig>
         <p>In this Letter we have presented the combination of all available constraints on the <it>B</it><sub><it>s </it></sub>mixing amplitude leading to a first evidence of NP contributions to the CP-violating phase. With the procedure we followed to combine the available data, we obtain an evidence for NP at more than 3<it>&#963;</it>. To put this conclusion on firmer grounds, it would be advisable to combine the likelihoods of the tagged <it>B</it><sub><it>s </it></sub>&#8594; <it>J</it>/&#936;<it>&#981; </it>angular analyses obtained without theoretical assumptions. This should be feasible in the near future. We are eager to see updated measurements using larger data sets from both the Tevatron experiments in order to strengthen the present evidence, waiting for the advent of LHCb for a high-precision measurement of the NP phase.</p>
         <p>It is remarkable that to explain the result obtained for <it>&#981;</it><sub><it>s</it></sub>, new sources of CP violation beyond the CKM phase are required, strongly disfavouring the MFV hypothesis. These new phases will in general produce correlated effects in &#916;<it>B </it>= 2 processes and in <it>b </it>&#8594; <it>s </it>decays. These correlations cannot be studied in a model-independent way, but it will be interesting to analyse them in specific extensions of the SM. In this respect, improving the results on CP violation in <it>b </it>&#8594; <it>s </it>penguins at present and future experimental facilities is of the utmost importance.</p>
      </sec>
      <sec>
         <st>
            <p>2. Note added</p>
         </st>
         <p>During the review procedure of this Letter, results based on new data were presented by the Tevatron experiments, as well as a combination of Tevatron results on the tagged angular analysis of <it>B</it><sub><it>s </it></sub>&#8594; <it>J</it>/&#968;<it>&#981;</it>. However these updates are all unpublished. Furthermore, the likelihoods required by our analysis are not publicly available except for the new D&#216; analysis with no assumption on strong phases <abbrgrp><abbr bid="B64">64</abbr></abbrgrp>. For the sake of completeness, we quote <inline-formula><graphic file="1754-0410-3-6-i11.gif"/></inline-formula> = (-19 &#177; 8)&#176; &#8746; (-69 &#177; 7)&#176; ([-36, -5]&#176; &#8746; [-83, -54]&#176; at 95% probability), obtained using this new likelihood for the D&#216; tagged angular analysis of <it>B</it><sub><it>s </it></sub>&#8594; <it>J</it>/&#968;<it>&#981;</it>. Clearly, we no longer need to manipulate the D&#216; likelihood to remove the strong phase assumption and to account for the non-Gaussian shape as described above. Remarkably, this updated result is well compatible with the results of this Letter, confirming a deviation from the SM at the level of ~3<it>&#963; </it>(99.6% probability). More recent experimental results seem to confirm the effect discussed in this Letter. We will include them in future analyses as soon as they become available.</p>
         <p>We are much indebted to M. Rescigno for triggering this analysis and for improving it with several valuable suggestions. We also thank G. Giurgiu, G. Punzi and D. Zieminska for their assistance with the Tevatron experimental results. We acknowledge partial support from RTN European contracts MRTN-CT-2006-035482 "FLAVIAnet" and MRTN-CT-2006-035505 "Heptools". M.C. is associated to the Dipartimento di Fisica, Universit&#224; di Roma Tre. E.F. and L.S. are associated to the Dipartimento di Fisica, Universit&#224; di Roma "La Sapienza".</p>
      </sec>
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