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A new approach for studying large numbers of fermions in the unitary regime 1 1 0 2 n MichaelG. Endres∗ a PhysicsDepartment,ColumbiaUniversity,NewYork,NY10027,USAand J TheoreticalPhysicsLaboratory,RIKEN,Wako,Saitama351-0198,Japan 5 E-mail: [email protected] ] t DavidB.Kaplan a l InstituteforNuclearTheory,UniversityofWashington,Seattle,WA98195-1550,USA - p E-mail: [email protected] e h Jong-WanLee [ InstituteforNuclearTheory,UniversityofWashington,Seattle,WA98195-1550,USA 2 E-mail: [email protected] v 9 Amy N.Nicholson 8 0 InstituteforNuclearTheory,UniversityofWashington,Seattle,WA98195-1550,USA 3 E-mail: [email protected] . 1 1 Anovellatticeapproachispresentedforstudyingsystemscomprisingalargenumberofinteract- 0 1 ing nonrelativisticfermions. The constructionis ideally suited fornumericalstudy of fermions : v near unitarity–a strongly coupled regime corresponding to the two-particle s-wave scattering Xi phase shift d 0 =p /2. Such systems may be achieved experimentally with trapped atoms, and r providea starting point for an effective field theorydescription of nuclear physics. We discuss a theconstructionofourlatticetheory,whichallowsustostudysystemsofupto(butbynomeans limited to) 38 fermions with high accuracy and modest computational resources, and offer an overviewofseveralapplicationsofthetechnique.Amoredetaileddiscussionofapplicationsand simulationresultswillbedescribedincompanionproceedingsbyA.N.N.andJ-W.L. TheXXVIIIInternationalSymposiumonLatticeFieldTheory,Lattice2010 June14-19,2010 Villasimius,Italy Speaker. ∗ (cid:13)c Copyrightownedbytheauthor(s)underthetermsoftheCreativeCommonsAttribution-NonCommercial-ShareAlikeLicence. http://pos.sissa.it/ Anewapproachforstudyinglargenumbersoffermionsintheunitaryregime MichaelG.Endres 1. Introduction Simulatingtheoriesatfinitefermiondensityhasbeenalong-standing challengeinlatticefield theory. One of the main issues faced in Monte Carlo studies of such theories is the fermion sign problem: when a chemical potential is introduced, the action often becomes complex. A conse- quenceofthisisthattheexponentialoftheactioncannotbeinterpretedasaprobabilitymeasureas required by standard Monte Carlo algorithms. In the case of lattice QCD at finite baryon number density, thesignproblemhasseverelylimitedtheexplorable regionsoftheQCDphasediagramin thetemperature-chemical potential (T-m )planetotheregimewhere m /T .1. B B Alternatively, at zero temperature, finite densities can be achieved in a canonical ensemble setting by considering multi-fermion correlation functions ina finite box. In this case, however, a closelyrelatedproblememerges: correlatorsinvolvingfermionstypicallyhaveasignal/noisewhich decays exponentially with the time separation of the source and sink. This makes identification of effective mass plateaus difficult–if not impossible–for large numbers of fermions. In QCD, standard Lepagearguments[1]suggestthatthesignal/noise formulti-baryon correlation functions decay with a time constant tB−1 ∼B(mp−3/2mp ), where B is the baryon number, mp the proton massandmp thepionmass. In an effort to better understand the sign and signal/noise problems as well as their interrela- tionship, we choose to study multi-fermion systems in a much simpler setting than QCD. One of thesimplestnontrivialandinterestingtheoriesdescribesadilutetwo-componentsystemofnonrel- ativisticfermionsintheunitaryregime. Thisregimecorrespondstoatwoparticles-wavescattering phaseshiftneard =p /2,andwhenthislimitisachieved, thebounds 4p /p2 onthes-wave 0 l=0 ≤ scattering cross-section becomes saturated. Although these systems are dilute, they are strongly interacting and therefore require a nonperturbative treatment for reliable study. Unitary fermions areinterestingnotonlybecausetheycanbestudiedexperimentallyusingtrappedultra-coldatoms, but also because they serve as a starting point for a lattice effective field theory (EFT) descrip- tion of nuclear physics. The latter is due to the fact that the 1S and 3S scattering lengths for 0 1 nucleon-nucleon scattering areunnaturally largecomparedtotherangeofinteraction. Inthiswork,wefocusonanewcanonicalensembleapproachforsimulatinglargenumbersof nonrelativistic fermions in the unitary regime and at zero temperature. Using this new approach, we consider two systems in particular: unitary fermions in a finite box and unitary fermions in a harmonic trap. From numerical simulations of these systems, one may extract experimentally measurable non-perturbative quantities such as the Bertsch parameter (i.e., the ratio of the energy to that of the free gas energy in the thermodynamic limit) and pairing gap. Furthermore, moving away from unitarity one may test a set of universal relations involving a quantity known as the “integrated contactdensity”, firstdiscoveredbyTan[2,3,4]. These proceedings focus primarily on the details of our lattice construction, as well as the simulation and parameter tuning methods used in our studies of unitary fermions. Many past numerical simulations at zero temperature have been variational in nature, offering only an upper bound on the Bertsch parameter and possessing unknown systematic errors on other quantities [5, 6, 7]. Our approach is nonvariational and is therefore in principle free from such systematic errors. However, as is common among all simulations of this type, obtaining reliable results for thespectrum and matrixelements requires agoodchoice ofinterpolating operators whichpossess 2 Anewapproachforstudyinglargenumbersoffermionsintheunitaryregime MichaelG.Endres large overlap with the states of interest. Details ofhow weconstruct optimal sources and sinks as well as consideration of systematic errors due to finite volume and lattice spacing effects are the focus of our companion proceedings [8, 9]. In those proceedings we also present results of our initial exploratory studies ofupto20trapped and 38untrapped fermions, andpresent preliminary valuesfortheBertchparameterandpairinggap. 2. Lattice construction Thestartingpointforourconstructionisahighlyimprovedvariantofthenonrelativisticlattice actionfirstproposed in[10],givenby: S=(cid:229) n (cid:20)y¯n(¶ t y )n−21My¯n((cid:209) 2y )n+f ny¯n(√Cy )n−e0(cid:21) . (2.1) Thisaction describes twospecies ofinteracting fermions y =(y ,y )defined onaT L3 lattice ↑ ↓ × withopenboundary conditionsinthetimedirectionandperiodicboundaryconditions inthespace directions. Thederivative¶ t representsaforwarddifference operatorintimeand(cid:209) 2 isanon-local lattice gradient operator which we define so-as to give a “perfect” continuum-like single particle dispersionrelationforfreefermions. Afour-fermioncontactinteractionisachievedviaaGaussian orZ auxiliaryfieldf associated withthetime-likelinksofthelattice. TheoperatorC actsonlyin 2 space, andinprinciple mayinclude derivativeinteractions toanarbitrary evenorderinmomenta. We may express Eq. 2.1 succinctly as S=y¯Ky , where the time components of the fermion matrixK aregiveninblock-matrix formby: D X(0) 0 0 ... 0 0 D X(1) 0 ... 0   0 0 D X(2) ... 0 K =  , (2.2)  0 0 0 D ... 0   ... ... ... ... ... X(T 1)  −   0 0 0 0 ... D      with (cid:209) 2 D=1 , X(t )=1 f (t )√C . (2.3) −2M − NotethattheL3 L3matricesD,X andCactonlyinspaceandthatf (t )isadiagonalmatrixwith × independent random elements. In momentum space the specific expressions we use for D andC are: ep2/(2M)d p <L hp|D|p′i= ¥ p,p′ |p| L , hp|C|p′i=C(p)d p,p′ (2.4) ( | |≥ where L = p is a hard momentum cutoff imposed on the fermions and C(p) is some analytic function of p2 which may be determined order by order in momenta from scattering data (see Sec.5fordetails). 3 Anewapproachforstudyinglargenumbersoffermionsintheunitaryregime MichaelG.Endres Fermion propagators from timeslice zero to timeslices t maybe expressed asasequence of applications ofDandX operators: K 1(t ;0)=D 1X(t 1)D 1...D 1X(0)D 1 , (2.5) − − − − − − whichprovidesasimplerecursiveapproachforcomputation. Inversionofthenon-localDoperator andapplication ofX(t )maybeperformedefficientlywithfastFouriertransforms(FFTs);itisthis feature that allows us to use a perfect dispersion relation and momentum dependent interactions. Inthefree-fieldlimit,onemayexplicitly verifythatourdefinitionforDprovided inEq.2.4yields aperfectdispersion relation forfermions. Inmomentumspacethefermionpropagator reducesto: p2 p K 1(t ;0)p =e E(p)t d , E(p)= , (2.6) − ′ − p,p h | | i ′ 2M formomentalessthanthecut-offL . 3. Simulationmethod andcost SinceK isanupper tri-diagonal block matrix, thefermiondeterminant obtained by“integrat- ingout”thefermionsisgivenbydetK=detDT. Weseethatthedeterminantisindependent ofthe auxiliary field, and therefore the full numerical simulation of Eq. 2.1 is equivalent to a quenched simulation. Byconstruction, our simulations are therefore free of the sign problem. Furthermore, the decomposition offermion propagators as aproduct of random matrices in Eq.2.5 provides an unusual interpretation for our approach: in essence we perform Euclidean time-evolution of sin- gle particle wavefunctions over random background noise (either Z orGaussian). Multi-particle 2 sources and sinks may be constructed from a direct product of single particle wavefunctions, and in the case of sinks, more elaborate constructions may be considered as well which incorporate pairing correlations [8,9]. NumericalsimulationofEq.2.1consistsoffoursteps: 1)latticegeneration,2)propagatorgen- eration, 3) projection of time-evolved states onto sinks and 4) computation of Slater determinants (i.e., anti-symmetrization of initial and final states). The relative computational cost of each of thesestepsonanL=32latticeisshowninFig.1asafunctionofthenumberofidenticalfermions. To give meaning to the vertical axis, note that the O(N0) curve indicates the numerical cost of generating O(L3) random numbers (i.e., lattice generation). The steps 1)-3) scale like T L3 or × T L3logL3, whereas step 4) is independent of the spatial volume. Although step 4) scales like × O(N4),1thecomputationalcostofthisstepisnegligibleevenforasmanyasN 50 100identical ∼ − fermionsonthetypicalvolumesweconsider, whichrangefromL 12 64. ∼ − 4. Transfer matrices Wemaytranslate our lattice action Eq.2.1into Hamiltonian language withasuitable reinter- pretation ofthe expression formulti-fermion correlation functions. Suchcorrelation functions are 1ThecostofcomputingdeterminantsscaleslikeN3,however, wecomputedeterminantsofallN sub-matricesas well,givingrisetoanadditionalpowerofN. 4 Anewapproachforstudyinglargenumbersoffermionsintheunitaryregime MichaelG.Endres 150 1012 L=32 100 1010 N1 50 Cost110068 N2 Latticegen. N0 HLSΗ 0 -50 Propagatorgen. 104 N´N3 Sinkproj. Slaterdet. -100 100 1 2 5 10 20 50 100 200 -150 -4 -2 0 2 4 6 8 10 Nidenticalfermions Η Figure 1: Cost ofnumericalsimulationsas a func- Figure2:Aplotofthethree-dimensionalz function tionofthenumberoffermionsN. S(h )givenbyEq.5.2 obtainedfromanensembleaverageofdirectproductsofpropagators. Sincethepropagatordefined inEq.2.5isitselfaproductofuncorrelated randommatrices(theauxiliaryfieldisaction-less), the multi-fermioncorrelationfunctionwillfactorizeintoamatrixproductofensembleaverages. Ifwe define: T =D1/2(1 V)D1/2 , (4.1) − where D =D 1/2 ... D 1/2 , (1 V )= X(t ) ... X(t ) (4.2) − − ⊗ ⊗ − h ⊗ ⊗ i N N areVN dimensional m|atrices, th{ezntheN-}fermioncorrelator|maybew{zrittenas:} K 1(t ;0) ... K 1(t ,0) =D 1/2T t D 1/2 , (4.3) − − − − h ⊗ ⊗ i N and we may identify T| as the trans{fzer matrix and}H = logT as the Hamiltonian of the N- − fermionsystem. Inthecaseoftwofermions(oneupandonedown),thetransfermatrixevaluatedinmomentum spaceisgivenby:2 pq T pq = d p,p′d q,q′+ C(p′) C(q′)d p+q,p′+q′ , C(p)= 4p (cid:229) C O (p), (4.4) h ′ ′| | i e−(pp2+p′2+q2p+q′2)/(4M) M n 2n 2n wherewehaveexpandedC(p)intheoperator basis: n O (p)=Mn 1 e p2/M p2n , for p <<1. (4.5) 2n − − ≈ | | (cid:16) (cid:17) Thistransfer matrixcanbediagonalized exactly, withthezerocenterofmomentum energy eigen- values(e E)givenbysolutions totheintegralequation: − (cid:229) 1 (cid:229) O2n(q) C I (p)=1, I (p)= , (4.6) 2n 2n 2n V e( p2+q2)/M 1 n q BZ − ∈ − 2WehaverecentlyimplementedanewHermitian,Galileaninvariantandanalyticversionofthisinteractionwhich corresponds to replacing: C(p) C(q) C(p p); results using this improved interaction will be presented in ′ ′ → − ′ detailinafuturepublication. p p 5 Anewapproachforstudyinglargenumbersoffermionsintheunitaryregime MichaelG.Endres where p=√ME andqaremomentawithinthefirstBrillouinzone(BZ). 5. Lattice parameter tuning andthe continuum limit Inthecontinuum,Luscher’sformulaallowsustorelatethetwoparticlescatteringphaseshifts at infinite volume to the discrete energies of the same system at finite volume [11, 12]. Having solved the twobody problem exactly on the lattice atfinite volume, wemay now relate the lattice couplings ofourtheorytocontinuum scattering data. Startingfromtheeffectiverangeexpansion 1 1 pcotd = + r p2+... (5.1) 0 0 −a 2 one can relate the scattering length (a), effective range (r ) and higher order shape parameters to 0 the s-wave scattering phase shift. Given an expression for pcotd one may then determine the 0 continuum energy eigenvalues inafiniteboxfromthesolutions to[13]: pcotd = 1 S(h ), S(h )= lim (cid:229) 1 4p L , (5.2) 0 p L L ¥ n2 h − → "n<L − # | | with h = (pL/2p )2. Finally one may tune the lattice couplings C (for n = 1,...,k) defined 2n in Eq. 4.5 by matching the lattice eigenvalues predicted by Eq. 4.6 to the lowest k continuum energies predicted by Luscher’s formula. In this way, we may absorb all temporal and spatial latticediscretization errorsintoourdefinitionofthecouplings. Thecontinuum limitforourlatticetheorycorresponds tothelimitofinfinitescattering length as measured inunits ofthe lattice spacing. In order tomaintain afinitephysical scattering length, onemusttakethislimitwhilekeeping otherphysical quantities measuredinunitsofthescattering length held fixed. In the case of unitary fermions, however, we need not concern ourselves with such complications and simply take pcotd =0. We therefore tune the couplings C so that the 0 2n latticeeigenvalues matchthelowestkrootsofS(h )showninFig.2. In Fig. 3 we plot the percent deviation between the roots of S(h ) and the lattice eigenvalues predicted byEq.4.6foruptoseventunedC-valuesforunitaryfermions. Foreigenvalues lessthan the k-th, the deviation is exactly zero by construction. For eigenvalues beyond the k-th, we find thatthepercentdeviation remainsquitesmallevenforeigenvalues ashighas27,corresponding to three filled shells. Given a tuned set ofC-values, we may also take the eigenvalues predicted by Eq.4.6and insert them back into Luscher’s formula, giving alattice prediction for pcotd . Fig. 4 0 shows a plot of the predicted pcotd for up to seven tuned C-values. We find pcotd 1 for a 0 0 ≪ widerangeofmomenta,extending wellbeyondthatofthek-theigenvalue wetunedto. 6. Conclusion Wehave developed anew approach for simulating alarge number ofnonrelativistic fermions in the unitary regime. In these proceedings we have described some of the details of our lattice construction, an efficient numerical implementation of the theory and a method for tuning the lattice couplings to scattering data. Application of these ideas to unitary fermions in a finite box 6 Anewapproachforstudyinglargenumbersoffermionsintheunitaryregime MichaelG.Endres 5 0.00006 LΗ HS 0.1 4 0.00004 of 0.00002 Out[76]= omroots0.001 No321.Cs pcot∆23 0 5 10 15 20 25-00.00002 No321.Cs v.fr10-5 54 1 54 de 6 6 % 7 7 10-7 0 0 5 10 15 20 25 0 50 100 150 200 250 Eigenvalueno. Η Figure3: Percentdeviationinh betweenexactlat- Figure 4: Implied pcotd obtainedfrom exactlat- 0 ticeeigenvalues(usingM=5andL=32)andcon- tice eigenvalues (using M = 5 and L = 32) and tinuumLuschereigenvalues. Luscher’sformula. [8]andinaharmonictrap3 [9]arediscussedingreaterdetailinourcompanionproceedings. There the issue of finding optimal sinks/sources as well as finite volume and cutoff effects are explored, andpreliminary resultsfortheBertschparameter andpairinggapreported. 7. Acknowledgments Thisworkwassupported byU.S.DepartmentofEnergygrantsDE-FG02-92ER40699(toM. G.E.)andDE-FG02-00ER41132(toD.B.K.,J-W.L.andA.N.N.). M.G.Eissupported bythe ForeignPostdoctoral Researcherprogram atRIKEN. References [1] G.P.Lepage, InvitedlecturesgivenatTASI’89SummerSchool,Boulder,CO,Jun4-30,1989. [2] S.Tan, AnnalsofPhysics323,2952(2008),cond-mat/0505200. [3] S.Tan, AnnalsofPhysics323,2971(2008),cond-mat/0508320. [4] S.Tan, AnnalsofPhysics323,2987(2008),arXiv:0803.0841. [5] S.Y.Chang,V.R.Pandharipande,J.Carlson,andK.E.Schmidt, Phys.Rev.A70,043602(2004), physics/0404115. [6] S.Y.ChangandG.F.Bertsch, Phys.Rev.A76,021603(2007),physics/0703190. [7] D.BlumeandK.M.Daily, (2010),arXiv:1008.3191. [8] J.-W.Lee,M.G.Endres,D.B.Kaplan,andA.N.Nicholson, (2010),arXiv:1011.3026. [9] A.N.Nicholson,M.G.Endres,D.B.Kaplan,andJ.-W.Lee, (2010),arXiv:1011.2804. [10] J.-W.ChenandD.B.Kaplan, Phys.Rev.Lett.92,257002(2004),hep-lat/0308016. [11] M.Luscher, Commun.Math.Phys.105,153(1986). [12] M.Luscher, Nucl.Phys.B354,531(1991). [13] S.R.Beane,P.F.Bedaque,A.Parreno,andM.J.Savage, Phys.Lett.B585,106(2004), hep-lat/0312004. 3Detailsregardingtheintroductionofexternalpotentialswillbepresentedin[9]. 7

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