| OCR Text |
Show cc University of Utah Institutional Repository Author Manuscript 1 Static hybrid quarkonium potential with improved staggered quarks MILC Collaboration: C. Bernard a, T. Burch b, C.E. DeTar c, Ziwen Fu c *, Steven Gottlieb d, E. Gregory b, U.M. Heller e, J. Osborn c, R.L. Sugar f, and D. Toussaint b aDepartment of Physics, Washington University, St. Louis, MO 63130, USA bDepartment of Physics, University of Arizona, Tucson, AZ 85721 , USA CPhysics Department, University of Utah, Salt Lake City, UT 84112, USA dDepartment of Physics, Indiana University, Bloomington, IN 47405, USA and Fermilab, Batavia, IL 60510, USA eCSIT, Florida State University, Tallahassee, FL 32306-4120, USA fDepartment of Physics, University of California, Santa Barbara, CA 93106, USA We are studying the effects of light dynamical quarks on the excitation energies of a flux tube between a static quark and antiquark. We report preliminary results of an analysis of the ground state potential and the ~~+ and IIu potentials. We have measured these potentials on closely matched ensembles of gauge configurations, generated in the quenched approximation and with 2+1 flavors of Asqtad improved staggered quarks. 1. INTRODUCTION Simulations with dynamical quarks have found that light quarks modify the heavy quarkantiquark potential in a number of ways [1 ,2,3]. At large distances they decrease the string tension in units of the Sommer ro and rl parameters (defined by r2 F (r) = 1. 65 and 1. 00, respectively) and lead eventually to string-breaking. At shorter distances they modify the running of the coupling constant, deepening the Coulomb well and increasing the ratio ro/rl' In this work, we extend these studies to some of the potentials with excited flux tubes. Of particular interest to quarkonium spectroscopy are the IIu excitations leading to exotic QQg hybrids [4]. We report results of a study in which our sources and sinks are optimized to create and annihilate a flux-tube state. In the presence of dynamical quarks, string breaking is expected. It is known that in the conventional ~t channel, transitions to the open two-meson channel are exceedingly weak, qualitatively consistent with the small *Presented by Ziwen Fu widths of quarkonium states above the heavylight meson thresholds [5 ,3]. Since at present we do not include the open two-meson channel we do not expect to observe string breaking here. 2. MEASUREMENTS We have measured the heavy quark potential on an ensemble of 283 x 96 (a ~ 0.09 fm) gauge configurations generated in the presence of 2 + 1 flavors of Asqtad dynamical quarks of varying masses and a one-loop Symanzik gauge action[6]. The strange quark mass is set approximately to its physical value. Here we compare results from our 358-configuration quenched ensemble with our 495-configuration dynamical quark ensemble for which (m7rro)2 ~ 1.3. The configurations are first smoothed using a single hypercubic (HYP) blocking pass [7] , a technique that improves significantly the signal-tonoise ratio [8] . The blocking procedure involves replacing all gauge links (timelike as well as spacelike) with an SU(3)-projected average over paths confined to adjacent hypercubes. Thus distortions in the result are local and expected to be c C H ~ :> c rt :::J 0 H ~ ~ ~ c (fJ n .H.. ... ~ rt cc ,.--.... H ->---0 H University of Utah Institutional Repository Author Manuscript 2 4 2 0 -2 ~ -4 0 2.60 2.0 1.6 1.0 1.6 2.0 2.6 o quenched o dynamical 1 fm 1 2 3 r/ro 2fm 4 Figure 1. The ground state static quark potential for quenched (octagons) and 2+ 1 flavor ( diamonds) QCD, in units of ro. The solid lines are fits to the Coulomb plus constant plus linear form, fixing Vfit(rO) = O. The lattice spacing is matched using ro. The inset expands the area shown by the box. confined to distances smaller than about 2a [8]. After HYP blocking the spacelike links are further smoothed via five cycles of APE smearing with SU(3) projection. On the thus smoothed lattices we measure the expectation value of the standard R x T Wilson loop on axis and along three different off-axis directions. These measurements yield the conventional ground state ~t and excited state ~t' potentials. For the IIu excited state, we measured the expectation value of a bent loop formed by replacing the source and sink flux tubes of length R by a superposition of large "staples" of sides (2a, R, 2a). For example one such loop replaces each on-axis spacelike flux path (Rx) by paths of the form (2af) , Rx, -2af)) minus its reflection in the xz plane [9]. 5 o 1 2 3 4 5 r/ro Figure 2. The excited ~~ potential for quenched (octagons) and 2+1 flavor (diamonds) QCD, in units of roo The lattice spacing was matched us-ing roo For the standard Wilson loop we extracted the usual ~t potential VL:;g+ and its excited state Vfg+ by doing a blocked, correlated, doubleexponential fit to the Wilson loop data: W(R, T) CL:;g+(R)e- V"Eg+(R)T + C~g+(R)e - V~g+(R)T. (1) (2) For the IIu potential we did only a singleexponential fit. In all cases we use the same fit ranges for both quenched and dynamical lattices to reduce possible systematic errors. 3. RESULTS In Fig. 1 we compare the ground state potential on the quenched ensemble and the 2+ 1 flavor ensemble. Both the distance scale and the potential are plotted in units of ro, and a constant has been subtracted from the potential so that it is zero at ro . Since ro was determined from this potential, the fits are tangent at this point. Away from ro , the potentials have dif- C C H ~ :> c rt :::J 0 H ~ ~ ~ C (fJ n .H.. ... ~ rt cc University of Utah Institutional Repository Author Manuscript 8 II - u 6 "...... 4 t ~~I H "--" > H0 (J) t~to~to~¥Drl 2 o quenched 0 <> dynamical 1 fm 2fm -2 0 1 2 3 4 5 r/ro Figure 3. The II;- potential for quenched (octagons) and 2+ 1 flavor (diamonds) QCD, in units of ro. The potentials are plotted relative to the zero determined in the fit to the ground state potentials. ferent shapes, namely, the Coulomb attraction is slightly stronger in the light quark ensemble and the string tension is slightly weaker in units of ro, confirming earlier findings [1]. A softening of the Coulomb well is also evident. This is an expected consequence of HYP smoothing. Similarly in Fig. 2 we show light quark effects in the ~~ excitation potential. The potentials are plotted relative to the zero determined in the fit to the ground state potentials. From Fig. 2 we see that the excited state potential ~~ is slightly steeper than that of quenched QCD. In Fig. 3 we plot the II;- potential. This hybrid potential is weakly repulsive at short range, as would be expected from the Coulomb interaction in a color octet quark-antiquark system. This effect is softened by HYP smoothing. At the level of our statistical errors there are no apparent differences at long range, but better statistics would certainly be of interest. 3 4. CONCLUSIONS Our measurements at a = 0.09 fm confirm the shape changes in the ground-state potential, seen previously at a = 0.13 fm. In units of ro we find, further, that adding 2 + 1 flavors of dynamical quarks makes the ~t' excited state potential slightly steeper and the II;- slightly more repulsive at short range. We find no clear evidence for a flattening of the potentials that would signal string breaking. Computations were performed at LANL, NERSC, NCSA, ORNL, PSC, SDSC, FNAL, and the CHPC (Utah). This work is supported by the U.S. NSF and DOE. REFERENCES 1. C. Bernard et al., Phys. Rev. D 62 (2000) 034503 and D. Toussaint, this conference (2002). 2. G. S. Bali et al. [TXL Collaboration]' Phys. Rev. D 62 (2000) 054503. C. Allton [UKQCD Collaboration], Nucl. Phys. Proc. Suppl. 109 (2002) 3. 3. B. Bolder et al., Phys. Rev. D 63 (2001) 074504. 4. K. J. Juge, J. Kuti and C. J. Morningstar, Phys. Rev. Lett. 82 (1999) 4400. and Nucl. Phys. Proc. Suppl. 83 (2000) 304. 5. C. Bernard et al., Phys. Rev. D 64 (2001) 074509.1. T. Drummond and R. R. Horgan, Phys. Lett. B 447 (1999) 298. 6. K. Orginos and D. Toussaint, Phys. Rev. D 59 (1999) 014501; K. Orginos, D. Toussaint and R. L. Sugar, Phys. Rev. D 60 (1999) 054503; G. P. Lepage, Phys. Rev. D 59 (1999) 074502. 7. A. Hasenfratz and F. Knechtli, Phys. Rev. D 64 (2001) 034504. 8. A. Hasenfratz, R. Hoffmann and F. Knechtli, Nucl. Phys. Proc. Suppl. 106 (2002) 418. 9. L. A. Griffiths, C. Michael and P. E. Rakow, Phys. Lett. B 129 (1983) 351. |