ebook img

Nonperturbative HQET at Order $1/m$ PDF

0.24 MB·
Save to my drive
Quick download
Download
Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.

Preview Nonperturbative HQET at Order $1/m$

February 1, 2011 2:12 WSPC/INSTRUCTION FILE mendes˙iwara09˙final International JournalofModernPhysicsD (cid:13)c WorldScientificPublishingCompany 1 1 0 2 Nonperturbative HQET at Order 1/m n a J BenoˆıtBlossier 0 LaboratoiredePhysiqueTh´eorique,Bˆatiment210,Universit´eParisXI, 3 F-91405OrsayCedex,France GeorgvonHippel ] Institutfu¨rKernphysik,UniversityofMainz,D-55099Mainz,Germany t a NicolasGarron l - SchoolofPhysicsandAstronomy,UniversityofEdinburgh,EdinburghEH93JZ,UK p TerezaMendes∗ e IFSC,UniversityofS˜aoPaulo,C.P.369,CEP13560-970, S˜aoCarlosSP,Brazil h [ ReceivedDayMonthYear 1 RevisedDayMonthYear v CommunicatedbyManagingEditor 0 0 We summarize first results for masses and decay constants of bottom-strange (pseudo- 8 scalar and vector) mesons from nonperturbatively renormalized heavy-quark effective 5 theory(HQET),usinglattice-QCDsimulationsinthequenched approximation. . 1 0 Keywords: Bphysics;latticeQCD;heavy-quarkeffective theory. 1 1 : 1. Introduction v i ThestudyofBphysicsisessentialtodeterminetheflavorstructureoftheStandard X Model, through knowledge of the Cabibbo-Kobayashi-Maskawa(CKM) matrix de- r a scribing quark mixing and CP violation, which may be associated with the lack of symmetry between matter and anti-matter in the Universe. In fact, since the amount of baryons in the Universe predicted using the CKM mechanism is sev- eral orders of magnitude smaller than what is observed by astronomers,extensions of the Standard Model propose additional sources of CP violation, which must be tested against Standard-Model predictions. B mesons provide the ideal environ- 1 ment for such tests. In particular,high-precisiontheoretical inputs are needed for hadronic matrix elements, which may be computed starting from the gauge theory itself using numericalsimulations of lattice QCD. At present,however,it is not yet feasible to perform simulations on lattices that can simultaneously represent the tworelevantscalesofBphysics:thelowenergyscaleΛ ,requiringlargephysical QCD lattice size, and the high energy scale of the b-quark mass m , requiringvery small b lattice spacing a. An approximate framework is therefore needed, but one should ∗Speaker. 1 February 1, 2011 2:12 WSPC/INSTRUCTION FILE mendes˙iwara09˙final 2 B. Blossier etal. [Alpha Collaboration] strive to achieve sufficiently precise results, otherwise the task of overconstraining the parameters of the Standard Model is compromised. Apromisingsuchframeworkistoconsider(lattice)heavy-quarkeffectivetheory (HQET), which allows for an elegant theoretical treatment, with the possibility of fully nonperturbative renormalization.2,3 The approach is briefly described as follows. HQET provides a valid low-momentum description for systems with one heavy quark, with manifest heavy-quark symmetry in the limit m . The b → ∞ heavy-quarkflavorandspinsymmetriesarebrokenatfinitevaluesofm respectively b by kinetic and spin terms, with first-order corrections to the static Lagrangian parametrized by ω and ω kin spin HQET = ψ (x)D ψ (x) ω ω , (1) L h 0 h − kinOkin − spinOspin where = ψ (x)D2ψ (x), = ψ (x)σ Bψ (x). (2) Okin h h Ospin h · h TheseO(1/m )correctionsareincorporatedbyanexpansionofthestatisticalweight b in 1/m such that , are treated as insertions into static correlation func- b kin spin O O tions. This guarantees the existence of a continuum limit, with results that are independent of the regularization, provided that the renormalization be done non- perturbatively. As a consequence, expansions for masses and decay constants are given respec- tively by m = m + Estat + ω Ekin + ω Espin (3) B bare kin spin and m f B = ZHQETpstat(1 + cHQETpδA + ω pkin + ω pspin), (4) Br 2 A A kin spin where the parameters m and ZHQET are written as sums of a static and an bare A O(1/m ) term (denoted respectively with the superscripts “stat” and “1/m ” be- b b low), and cHQET is of order 1/m . Bare energies (Estat, etc.) and matrix elements A b (pstat, etc.) are computed in the numerical simulation. The divergences (with inverse powers of a) in the above parameters are can- celled through the nonperturbative renormalization, which is based on a matching of HQET parameters to QCD on lattices of small physical volume — where fine lattice spacings can be considered — and extrapolation to a large volume by the step-scalingmethod.Suchananalysishasbeenrecentlycompletedforthequenched 4 case. In particular, there are nonperturbative (quenched) determinations of the static coefficients mstat and Zstat for HYP1 and HYP2 static-quark actions5 at bare A the physical b-quark mass, and similarly for the O(1/m ) parameters ω , ω , b kin spin m1/mb, Z1/mb and cHQET. bare A A The newly determined HQET parameters are very precise (with errors of a couple of a percent in the static case) and show the expected behavior with a. February 1, 2011 2:12 WSPC/INSTRUCTION FILE mendes˙iwara09˙final Nonperturbative HQETat Order 1/m 3 They are used in our calculations reported here, to perform the nonperturbative renormalization of the (bare) observables computed in the simulation. Of course, in order to keep a high precision, also these bare quantities have to be accurately determined. This is accomplished by an efficient use of the generalized eigenvalue problem(GEVP)forextractingenergylevelsE andmatrixelements,asdescribed n below. Asignificantsourceofsystematic errorsinthe determinationofenergylevels in lattice simulations is the contamination from excited states in the time correlators ∞ C(t) = O(t)O(0) = n Oˆ 0 2 e−Ent (5) h i |h | | i| nX=1 of fields O(t) with the quantum numbers of a given bound state. Insteadofstarting fromsimple localfields O and getting the (ground-state)en- ergyfromaneffective-massplateauinC(t)asdefinedabove,itisthenadvantageous 6 to consider all-to-all propagators and to solve, instead, the GEVP C(t)v (t,t ) = λ (t,t )C(t )v (t,t ), (6) n 0 n 0 0 n 0 where t>t and C(t) is now a matrix of correlators,given by 0 ∞ C (t) = O (t)O (0) = e−EntΨ Ψ , i,j =1,...,N. (7) ij i j ni nj h i nX=1 The chosen interpolators O are taken (hopefully) linearly independent, e.g. they i may be built from the smeared quark fields using N different smearing levels. The matrix elements Ψ are defined by ni Ψ (Ψ ) = nOˆ 0 , mn = δ . (8) ni n i i mn ≡ h | | i h | i One thus computes C for the interpolator basis O from the numerical simu- ij i lation, then gets effective energy levels Eeff and estimates for the matrix elements n Ψ from the solution λ (t,t ) of the GEVP at large t. For the energies ni n 0 1 λ (t,t ) Eeff(t,t ) log n 0 (9) n 0 ≡ a λ (t+a,t ) n 0 it is shown7 that Eeff(t,t ) convergesexponentially as t (and fixed t ) to the n 0 →∞ 0 true energy E . However, since the exponential falloff of higher contributions may n be slow, it is also essential to study the convergence as a function of t in order 0 8 to achieve the requiredefficiency for the method. This has been recently done, by explicit application of (ordinary) perturbation theory to a hypothetical truncated problemwhereonlyN levelscontribute.Thesolutioninthiscaseisexactlygivenby thetrueenergies,andcorrectionsduetothehigherstatesaretreatedperturbatively. We get Eeff(t,t ) = E + ε (t,t ) (10) n 0 n n 0 February 1, 2011 2:12 WSPC/INSTRUCTION FILE mendes˙iwara09˙final 4 B. Blossier etal. [Alpha Collaboration] for the energies and ∞ e−Hˆt(Qˆenff(t,t0))†|0i = |ni + πnn′(t,t0)|n′i (11) nX′=1 for the eigenstates of the Hamiltonian, which may be estimated through ˆeff(t,t )= R (Oˆ, v (t,t )), (12) Qn 0 n n 0 t/2 λ (t +a,t ) R = (v (t,t ), C(t)v (t,t ))−1/2 n 0 0 . (13) n n 0 n 0 (cid:20)λ (t +2a,t )(cid:21) n 0 0 In our analysis we see that, due to cancellations of t-independent terms in the effective energy, the first-order corrections in ε (t,t ) are independent of t and n 0 0 very strongly suppressed at large t. We identify two regimes: 1) for t < t/2, the 0 2nd-order corrections dominate and their exponential suppression is given by the smallestenergygap E E ∆E betweenlevelnanditsneighboringlevels m n m,n | − |≡ m; and 2) for t t/2, the 1st-order corrections dominate and the suppression 0 ≥ is given by the large gap ∆EN+1,n. Amplitudes πnn′(t,t0) get main contributions from the first-order corrections. For fixed t t these are also suppressed with 0 − ∆E . Clearly, the appearance of large energy gaps in the second regime im- N+1,n proves convergence significantly. We therefore work with t, t combinations in this 0 regime. A very important step of our approach is to realize that the same perturba- tive analysis may be applied to get the 1/m corrections in the HQET correlation b functions mentioned previously C (t) = Cstat(t) + ωC1/mb(t) + O(ω2), (14) ij ij ij where the combined O(1/m ) corrections are symbolized by the expansion param- b eter ω.Following the same procedure as above,we get similar exponentialsuppres- sions (with the static energy gaps) for static and O(1/m ) terms in the effective b theory. We arrive at Eneff(t,t0) = Eneff,stat(t,t0)+ωEneff,1/mb(t,t0)+O(ω2) (15) with Eneff,stat(t,t0)= Enstat + βnstate−∆ENsta+t1,nt+... , (16) Eneff,1/mb(t,t0)= En1/mb + [βn1/mb − βnstatt∆EN1/+m1b,n]e−∆ENsta+t1,nt+... . (17) and similarly for matrix elements. Preliminary results of our application of the 9 methods described in this section were presented recently and are summarized in 10 thenextsection.Amoredetailedversionofthisstudywillbepresentedelsewhere. February 1, 2011 2:12 WSPC/INSTRUCTION FILE mendes˙iwara09˙final Nonperturbative HQETat Order 1/m 5 2. Results We carried out a study of static-light B -mesons in quenched HQET with the non- s perturbative parameters described in the previous section, employing the HYP1 and HYP2 lattice actions for the static quark and anO(a)-improvedWilson action for the strange quark in the simulations. The lattices considered were of the form L3 2Lwithperiodicboundaryconditions.WetookL 1.5fmandlatticespacings × ≈ 0.1 fm, 0.07 fm and 0.05 fm, corresponding respectively to β =6.0219, 6.2885 and 6.4956.We usedall-to-allstrange-quarkpropagatorsconstructedfromapproximate lowmodes,with100configurations.Gaugelinksininterpolatingfieldsweresmeared with 3 iterations of (spatial) APE smearing, whereas Gaussian smearing (8 levels) was used for the strange-quark field. A simple γ γ structure in Dirac space was 0 5 taken for all 8 interpolating fields. Also, the local field (no smearing) was included in order to compute the decay constant. Theresulting(8 8)correlationmatrixmaybeconvenientlytruncatedtoanN × × N oneandtheGEVPsolvedforeachN,sothatresultscanbestudiedasafunction ofN.Wethenpickabasisfromunprojectedinterpolators,bysamplingthedifferent smearing levels (from 1 to 7) as 1,7 , 1,4,7 ,etc. We perform fits of the various { }{ } energy levels and values of N to the behavior in Eq. (16) and extract our results from the predicted plateaus. Next, we take the continuum limit, extrapolating our resultstoa 0.Weseethatthecorrectiontotheground-stateenergyduetoterms → of order 1/m , which is positive for finite a, is quite small (consistent with zero) b in the continuum limit. Our results for the pseudoscalar meson decay constant, both in the static limit and including O(1/m ) corrections, are shown in terms b of the combination ΦHQET FPS√mPS/CPS, where CPS(M/ΛQCD) is a known ≡ matching function and ΦRGI denotes the renormalization-group-invariant matrix 11 elementofthestaticaxialcurrent. Thesetwocontinuumextrapolationsareshown 11 in comparison with fully relativistic heavy-light (around charm-strange) data in Fig. 1 below. Note that, up to perturbative corrections of order α3 in C , HQET PS predicts a behaviorconst.+O(1/r m ) inthis graph.Surprisinglyno 1/(r m )2 0 PS 0 PS terms are visible, even with our rather small errors. 3. Conclusions The combined use of nonperturbatively determined HQET parameters (in action and currents) and efficient GEVP allows us to reach precisions of a few percent in matrix elements and of a few MeV in energy levels, even with only a moder- ate number of configurations. The method is robust with respect to the choice of interpolator basis. All parameters have been determined nonperturbatively and in particular power divergences are completely subtracted. We see that HQET plus O(1/m )correctionsatthe b-quarkmassagreeswellwithaninterpolationbetween b thestaticpointandthecharmregion,indicatingthatlinearityin1/mextendseven to the charm point. A corresponding study for N =2 is in progress. f February 1, 2011 2:12 WSPC/INSTRUCTION FILE mendes˙iwara09˙final 6 B. Blossier etal. [Alpha Collaboration] Fig.1. ComparisonofthecontinuumvaluesforthepseudoscalarmesondecayconstantfromFig. 4tofullyrelativisticdatainthecharmregion.Thesolidlineisalinearinterpolationbetweenthe staticlimitandthepointsaroundthecharm-quarkmass,whichcorrespondsto 1/r0mPS≈0.2. Acknowledgements.Thisworkis supportedby theDFG inthe SFB/TR09,and by the EU Contract No. MRTN-CT-2006-035482,“FLAVIAnet”. T.M. thanks the A.vonHumboldtFoundation;N.G.thankstheMICINNgrantFPA2006-05807,the Comunidad Aut´onoma de Madrid programme HEPHACOS P-ESP-00346 and the Consolider-Ingenio 2010 CPAN (CSD2007-00042). References 1. M. Antonelli et al., arXiv:0907.5386 [hep-ph]. 2. J. Heitger and R. Sommer [ALPHA Collaboration], JHEP 0402, 022 (2004) [arXiv:hep-lat/0310035]. 3. R.Sommer, arXiv:hep-lat/0611020. 4. B. Blossier, M. Della Morte, N. Garron and R. Sommer, arXiv:1001.4783 [hep-lat]. 5. M.DellaMorteetal.,Phys.Lett.B581,93(2004)[Erratum-ibid.B612,313(2005)] [arXiv:hep-lat/0307021]. 6. J. Foley et al., Comput. Phys.Commun. 172, 145 (2005) [arXiv:hep-lat/0505023]. 7. M. Lu¨scher and U.Wolff, Nucl. Phys. B 339, 222 (1990). 8. B. Blossier et al., JHEP 0904, 094 (2009) [arXiv:0902.1265 [hep-lat]]; PoS LAT- TICE2008, 135 (2008) [arXiv:0808.1017 [hep-lat]]. 9. B. Blossier, M. Della Morte, N. Garron, G. von Hippel, T. Mendes, H. Simma and R.Sommer, arXiv:0911.1568 [hep-lat]. 10. B. Blossier et al., arXiv:1004.2661 [hep-lat]. 11. M. Della Morte et al., JHEP 0802, 078 (2008) [arXiv:0710.2201 [hep-lat]].

See more

The list of books you might like

Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.