4
Simulating the Wess-Zumino Supersymmetry Model in Optical Lattices Yue Yu 1 and Kun Yang 2 1 Institute of Theoretical Physics, Chinese Academy of Sciences, P.O. Box 2735, Beijing 100190, China 2 NHMFL and Department of Physics, Florida State University, Tallahassee, Florida 32306, USA (Received 25 May 2010; revised manuscript received 11 September 2010; published 8 October 2010) We study a cold atom-molecule mixture in two-dimensional optical lattices. We show that, by fine- tuning the atomic and molecular interactions, the Wess-Zumino supersymmetry (SUSY) model in 2 þ 1 dimensions emerges in the low-energy limit and can be simulated in such mixtures. At zero temperature, SUSY is not spontaneously broken, which implies identical relativistic dispersions of the atom and its superpartner, a bosonic diatom molecule. This defining signature of SUSY can be probed by single- particle spectroscopies. Thermal breaking of SUSY at a finite temperature is accompanied by a thermal Goldstone fermion, i.e., phonino excitation. This and other signatures of broken SUSY can also be probed experimentally. DOI: 10.1103/PhysRevLett.105.150605 PACS numbers: 05.50.+q, 11.30.Pb, 37.10.Jk, 67.85.Pq Introduction.—Wess and Zumino proposed the first space-time supersymmetry (SUSY) model (WZ-SUSY model) 36 years ago [1]. Since then, SUSY has become a fundamental ingredient of theories beyond the standard model in high-energy physics [2]. However, none of the superpartners of the known elementary particles have been found thus far; it remains to be seen if they can be detected in the energy range of the Large Hadron Collider. On a different front, nonrelativistic SUSY (a Bose- Fermi symmetry unrelated to space-time symmetry) has attracted considerable recent interest in the cold atom community, as it can be realized by using Bose-Fermi atom (molecule) mixtures which are loaded in optical lattices. Examples include attempts to simulate the non- relativistic limit of a superstring by trapping fermionic atoms in the core of vortices in a Bose-Einstein condensate [3], the study of the SUSY effect in an exactly solvable one-dimensional Bose-Fermi mixture with the Bethe an- satz [4], and SUSY models for nonrelativistic particles in various dimensions [57]. In Refs. [6,7], we studied per- haps the simplest cold atom SUSY model and discussed detecting the Goldstino mode by measuring the single- fermion spectral function and the SUSY response. Although these studies are interesting, SUSY in these non- relativistic systems is very different from the relativistic (or space-time) SUSY in high-energy physics. In this Letter, we propose a way to simulate the simplest relativistic SUSY model, the WZ-SUSY model [1]. We show that it can emerge in the low-energy limit of a cold atom-molecule mixture in properly chosen two- dimensional lattices. The first requirement is the existence of Dirac points in the Brillouin zone. In most proposed models [8], two Dirac points K and K 0 are related to each other by K 0 ¼K. This means that two fermionic atoms which form a usual BCS pair or a diatom molecule belong to two different Dirac points. This molecule cannot sever as a Klein-Gordon field which corresponds to a diatom molecule made by two Dirac fermions from the same Dirac point. Such molecules carry a 2K Þ 0 momentum and are energetically unfavorable as a result. In a recent work, Lee attempted to avoid this difficulty by introducing frustrated hopping for the molecules, such that the boson dispersion has minima at 2K instead of zero [9]. It is found that the massless WZ-SUSY model emerges at the boson’s superfluid-insulator critical point. In this work, we show that the WZ-SUSY model can emerge not only at the critical point. We use a lattice model studied recently by Liu et al. [10] instead. This is a square lattice model in which the Dirac points at K ¼ð0; 0Þ and K 0 ¼ð0;%Þ are their own negatives, as ð0; %Þð0;%Þ. This means a diatom molecule made of two atoms from the same Dirac points has zero momentum for 2K ¼ð0; 0Þ and 2K 0 ¼ð0; 2%Þð0; 0Þ. With this setup, we can simulate the WZ-SUSY model more straightforwardly, after appro- priate interactions are introduced and fine-tuned. The research interest in WZ-SUSY models has been re- newed recently [11]. No spontaneous breaking of the SUSY implies that there are equal poles in the single-particle spec- tral functions of both the Dirac field and the Klein-Gordon field. A further calculation showed that these single-particle spectral functions are not renormalized from their free par- ticle ones [12]. This is the identifier of the SUSY and may be detected by the established techniques of the single-particle spectroscopies [13]. It is known that a thermal bath always breaks the SUSY [14], and this thermal breaking of the SUSY is accompanied by a thermal Goldstone fermion, the phonino [12]; thus, studying this model at a finite tempera- ture sheds light on the physics of SUSY breaking. There are many studies of SUSY in space-time lattice models [15]. The significant difference between the present work and those lattice SUSY models is that, while the latter are supersymmetric on the lattices, we study the emergence of SUSY from a microscopic space lattice (but continuous time) model with no SUSY to begin with. PRL 105, 150605 (2010) PHYSICAL REVIEW LETTERS week ending 8 OCTOBER 2010 0031-9007= 10=105(15)=150605(4) 150605-1 Ó 2010 The American Physical Society

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Page 1: Simulating the Wess-Zumino Supersymmetry Model in Optical Lattices

Simulating the Wess-Zumino Supersymmetry Model in Optical Lattices

Yue Yu1 and Kun Yang2

1Institute of Theoretical Physics, Chinese Academy of Sciences, P.O. Box 2735, Beijing 100190, China2NHMFL and Department of Physics, Florida State University, Tallahassee, Florida 32306, USA

(Received 25 May 2010; revised manuscript received 11 September 2010; published 8 October 2010)

We study a cold atom-molecule mixture in two-dimensional optical lattices. We show that, by fine-

tuning the atomic and molecular interactions, the Wess-Zumino supersymmetry (SUSY) model in 2þ 1

dimensions emerges in the low-energy limit and can be simulated in such mixtures. At zero temperature,

SUSY is not spontaneously broken, which implies identical relativistic dispersions of the atom and its

superpartner, a bosonic diatom molecule. This defining signature of SUSY can be probed by single-

particle spectroscopies. Thermal breaking of SUSY at a finite temperature is accompanied by a thermal

Goldstone fermion, i.e., phonino excitation. This and other signatures of broken SUSY can also be probed

experimentally.

DOI: 10.1103/PhysRevLett.105.150605 PACS numbers: 05.50.+q, 11.30.Pb, 37.10.Jk, 67.85.Pq

Introduction.—Wess and Zumino proposed the firstspace-time supersymmetry (SUSY) model (WZ-SUSYmodel) 36 years ago [1]. Since then, SUSY has become afundamental ingredient of theories beyond the standardmodel in high-energy physics [2]. However, none of thesuperpartners of the known elementary particles have beenfound thus far; it remains to be seen if they can be detectedin the energy range of the Large Hadron Collider.

On a different front, nonrelativistic SUSY (a Bose-Fermi symmetry unrelated to space-time symmetry) hasattracted considerable recent interest in the cold atomcommunity, as it can be realized by using Bose-Fermiatom (molecule) mixtures which are loaded in opticallattices. Examples include attempts to simulate the non-relativistic limit of a superstring by trapping fermionicatoms in the core of vortices in a Bose-Einstein condensate[3], the study of the SUSY effect in an exactly solvableone-dimensional Bose-Fermi mixture with the Bethe an-satz [4], and SUSY models for nonrelativistic particles invarious dimensions [5–7]. In Refs. [6,7], we studied per-haps the simplest cold atom SUSY model and discusseddetecting the Goldstino mode by measuring the single-fermion spectral function and the SUSY response.Although these studies are interesting, SUSY in these non-relativistic systems is very different from the relativistic (orspace-time) SUSY in high-energy physics.

In this Letter, we propose a way to simulate the simplestrelativistic SUSY model, the WZ-SUSY model [1].We show that it can emerge in the low-energy limit of acold atom-molecule mixture in properly chosen two-dimensional lattices. The first requirement is the existenceof Dirac points in the Brillouin zone. In most proposedmodels [8], two Dirac points K and K0 are related to eachother by K0 ¼ �K. This means that two fermionic atomswhich form a usual BCS pair or a diatom molecule belongto two different Dirac points. This molecule cannot severas a Klein-Gordon field which corresponds to a diatom

molecule made by two Dirac fermions from the sameDiracpoint. Such molecules carry a 2K � 0 momentum and areenergetically unfavorable as a result. In a recent work, Leeattempted to avoid this difficulty by introducing frustratedhopping for the molecules, such that the boson dispersionhas minima at �2K instead of zero [9]. It is found thatthe massless WZ-SUSY model emerges at the boson’ssuperfluid-insulator critical point.In this work, we show that the WZ-SUSY model can

emerge not only at the critical point. We use a lattice modelstudied recently by Liu et al. [10] instead. This is a squarelattice model in which the Dirac points at K ¼ ð0; 0Þ andK0 ¼ ð0; �Þ are their own negatives, as ð0;��Þ � ð0; �Þ.This means a diatommolecule made of two atoms from thesame Dirac points has zero momentum for 2K ¼ ð0; 0Þ and2K0 ¼ ð0; 2�Þ � ð0; 0Þ. With this setup, we can simulatethe WZ-SUSY model more straightforwardly, after appro-priate interactions are introduced and fine-tuned.The research interest in WZ-SUSY models has been re-

newed recently [11]. No spontaneous breaking of the SUSYimplies that there are equal poles in the single-particle spec-tral functions of both the Dirac field and the Klein-Gordonfield. A further calculation showed that these single-particlespectral functions are not renormalized from their free par-ticle ones [12]. This is the identifier of the SUSYand may bedetected by the established techniques of the single-particlespectroscopies [13]. It is known that a thermal bath alwaysbreaks the SUSY [14], and this thermal breaking of theSUSY is accompanied by a thermal Goldstone fermion, thephonino [12]; thus, studying this model at a finite tempera-ture sheds light on the physics of SUSY breaking.There are many studies of SUSY in space-time lattice

models [15]. The significant difference between the presentwork and those lattice SUSYmodels is that, while the latterare supersymmetric on the lattices, we study the emergenceof SUSY from a microscopic space lattice (but continuoustime) model with no SUSY to begin with.

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Free fermion lattice model and continuum limit.—Webriefly recall the lattice model proposed in Ref. [10].Consider a single-component fermionic atom gas loadedin a square lattice. The potential minimum in the sublatticeA is higher than that in the sublattice B. Two states with theenergy difference 2M, the s orbital at the A sites and the porbital at the B sites, form a pseudospin-1=2 subspace. Thesublattices are anisotropic with 1, 2, 3, and 4, the nextnearest neighbor sites [Fig. 1(b)]. The hoppings betweenthe nearest and next nearest sites are taken into account.The corresponding hopping amplitudes are tA;Aþ�xðyÞ ¼�tA;A��xðyÞ ¼ tAB, tA1 ¼ tA3, tA2 ¼ tA4, tB1 ¼ tB3, and

tB2 ¼ tB4 with �x (�y) being the unit vector in the x (y)

direction. In addition, a periodic gauge field generated bytwo opposite-traveling standing wave laser beams couplingwith atoms [16] is introduced. This gives rise to a tunablestaggered Peierls phase ��0 along the vertical links andvanishing in the horizontal and 1, 2, 3, 4 links. With thesethe single-fermion Hamiltonian is given by

HðkÞ ¼ pxðkÞ�x þ pyðkÞ�y þ hzðkÞ�z; (1)

where px ¼ 2tAB sin�0 sinðkyaÞ, py ¼ 2tAB½sinðkxaÞ þ cos

�0 sinðkyaÞ�, and hz ¼ �M� t0 cosðkxaÞ cosðkyaÞ � 2~t

sinðkxaÞ sinðkyaÞ with t0 ¼ tA1 � tB1 þ tA2 � tB2 and ~t ¼ðtA1 � tB1 þ tB2 � tA2Þ=2. When M ¼ �t0 � 0, there is aunique gapless Dirac point: either K ¼ ð0; 0Þ or K0 ¼ð0; �Þ. We choose �0 ¼ �=2 and define the ‘‘speed oflight’’ vs ¼ 2tABa. In the continuum limit and near theDirac points, pxðK þ �kÞ � 2tABa�ky � vsqx and pxðK0

þ�kÞ � �2tABa�ky ¼ �vsqx; pyðK þ �kÞ � 2tABa�kx� vsqy and pyðK0 þ �kÞ � 2tABa�kx � vsqy; and hzðK þ�kÞ ¼ �M� t0 ¼ m0 and hzðK0 þ �kÞ ¼ �Mþ t0 ¼m�. Thus, for the Dirac fields �ðxÞ near K and �ðxÞ nearK0, the effective Hamiltonian reads

Hð0Þc ¼ vs

Zd2x�yð�i�aþ@a þm0�zÞ�

þ vs

Zd2x�yð�i�a�@a þm��zÞ�; (2)

where �1� ¼ ��x and �2� ¼ �y; the two-componentDirac field �ðrÞ is given by

�1

�2

� �¼ 1ffiffiffi

2p

Z �

0d2qeiq:x �1q

�q1

� �þ �y

2;�q

�q�1

� �� �;

with �q ¼ qxþiqyjqj ¼ ���q and similarly for � . The momen-

tum cutoff � corresponds to that when the lattice fermiondispersion deviates severely from the linear one. The massterms here can be fine-tuned. WhenM ¼ �t0, which is notzero in this lattice setup [10], one of the Dirac field ismassless and another is massive. The latter can be inte-grated out in the low-energy limit. We note that the zeromatter density (necessary for Lorentz invariance) in therelativistic quantum field theory corresponds to fermionicatoms being at half filling in this lattice realization. Afteran external source is introduced, the fermion number(including those forming molecules) will fluctuate butaverage at half filling. To facilitate pairing or moleculeformation, we introduce attraction between fermionicatoms, which is modeled in a two-channel fashion below.For such spinless fermions, the two-atom attraction and p-wave-type bound state have already been achievedexperimentally [17].Two-channel model.—We take m0 ¼ 0 and m� � 0 and

integrate out � in the low-energy limit where only the stateswith their energy lower than minfm�; E�g are relevant. Wenow extend our Hamiltonian to a two-channel model, i.e.,the lowest two hyperfine atom states with two-atom scat-tering states in an open channel and the two-atom boundstate (Feshbachmolecule) in a closed channel.We denote as

�ðoÞðxÞ the Dirac fermions in the open channel and �ðcÞðxÞthe Dirac fermion in the closed channel. Analogous to themany-body theory of the atom-molecule coherence inRef. [18], the effective Lagrangian describing this two-channel Dirac fermion model is given by

L ¼ ��ðoÞy��@��ðoÞ � �ðcÞy��@��

ðcÞ

þUðcÞ�ðcÞy2 �ðcÞy

1 �ðcÞ1 �ðcÞ

2 þUðcoÞ�ðcÞy2 �ðcÞy

1 �ðoÞ1 �ðoÞ

2

þ H:c:;

where�� ¼ ðI; �x; �yÞ and @� ¼ ð@t; vsrÞ.UðcÞ andUðcoÞ

are the interaction between closed channel fermions and theinterchannel interaction, respectively. We have neglectedthe background interaction in the open channel. By intro-

ducing the pairing field �ðr; tÞ for �ðcÞ via a Hubbard-

Stratonovich transformation and integrating out �ðcÞ, theresulting Lagrangian is given by

L ð�ðoÞ;�Þ ¼ � 1

2�ðoÞy�y��@��

ðoÞ � j�j2UðcÞ þ Tr lnGðcÞ�1:

(3)

The inverse of the propagator GðcÞ of �ðcÞ is given by

2 1

3 4

A B(a) (b)

x

y

FIG. 1 (color online). (a) Josephson tunneling between theatom-molecule mixture (lower lattice plane) and the dimoleculeBose-Einstein condensate nearby (upper plane). The orange dotsare molecules in the mixture, and red dots are dimolecules.Fermionic atoms are in the lattice sites. (b) The square latticewhere 1, 2, 3, and 4 denote the next nearest neighbor sites.

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Page 3: Simulating the Wess-Zumino Supersymmetry Model in Optical Lattices

GðcÞ�1 ¼ 0 i��@��i��@� 0

� �� � 0

0 �y� �

;

where � ¼ �þUðcoÞ�ðoÞ1 �ðoÞ

2 . Expanding the Lagrangian

in powers of � and its gradients yields

L ½’� ¼ � 1

2@�’

y@�’� 1

2"mj’j2 �

8j’j4 þOðj’j6Þ;

(4)

where ’ / �=UðcÞ is the Feshbach molecular field with

the detuning energy "m and the interacting strength /ðUðcÞÞ2. We have vb ¼ vs in the weak coupling limit (i.e.,

Uðc;coÞ much smaller than all other energy scales in thesystem including m� and E�) due to (emergent) Lorentzinvariance. Lattice effects (which break Lorentz invari-ance) give rise to nonuniversal corrections to vs and vb;thus, tuning of one parameter (e.g., molecule dispersionthrough an additional lattice potential seen by the moleculeonly) is needed to ensure vb ¼ vs to maintain Lorentzinvariance in the low-energy limit. Also included in (3) is

the Yukawa coupling between ’ and �ðoÞ, i.e., L’� ¼� g

2 ð’�ðoÞy2 �ðoÞy

1 þ ’y�ðoÞ1 �ðoÞ

2 Þ with g / �2UðcoÞ.WZ-SUSY model: Massless.—For simplicity, we drop

the superscript of �ðoÞ hereafter. By combining (3) and(4) and the Yukawa coupling together, the effectiveLagrangian after neglecting Oðj’j6Þ is given by

L ð�; ’Þ ¼ � 1

2@�’

y@�’� 1

2"mj’j2 � i�y��@��

8j’j4 � g

2ð’�y

2�y1 þ ’y�1�2Þ: (5)

By tuning "m ¼ 0 by varying UðcÞ, and further tuning pair-pair (or molecule-molecule) interaction by varyingUðcoÞ sothat the coupling constant ¼ g2, the effective LagrangianLð�;’Þ is exactly the massless WZ-SUSY model with theSUSY under the SUSY transformations �’ ¼ y�y� and�� ¼ ���y@�’

y � g2’

y2, where is a constant two-

component spinor parameter.WZ-SUSY model: Massive.—To have a massive WZ-

SUSY model, we need to introduce an external source.This can be realized by putting a Bose-Einstein condensateof dimolecules nearby, which is made of pairs of molecules(or 4-atom molecules) [see Fig. 1(a)]. Through Josephsontunneling with an amplitude �, the dimolecule condensateexchanges pairs of molecules with the mixture. The effec-tive Lagrangian reads

Lð�;’;�Þ ¼ � 1

2@�’

y@�’� i�y��@��� g2

8j’j4

� g

2ð’�y

2�y1 þ ’y�1�2Þ

þ �ð�y’2 þ�’y2Þ; (6)

where� is the external dimolecular field. There is a globalUð1Þ symmetry (called R symmetry) under � ! ei��, ’ !

e2i�’, and � ! e4i�� [11]. If � slowly varies in space-time, it is also SUSY invariant under �’ ¼ y�y� and

�� ¼ ���y@�’y � g

2’y2þ 4��y

g . By taking � to be

its condensed order parameter h�i ¼ h�yi ¼ m2=8�, theR symmetry is broken and reduced to a discrete Z2 sym-metry with � ! i� and ’ ! �’, and the on-shell WZLagrangian appears (up to an additive constant):

Lð�; ’;mÞ ¼ � 1

2@�’

y@�’� i�y��@��

� g2

8

�’y2 �m2

g2

��’2 �m2

g2

� g

2ð’�y

2�y1 þ ’y�1�2Þ: (7)

The SUSY is exact by replacing�y with h�yi in the SUSYtransformations. The Z2 symmetry is always spontane-ously broken in one of the degenerate ground states with’ ¼ ��m=g. The SUSY Lagrangian with spontaneousbreaking of Z2 becomes

L ¼ � 1

2@��

y@��� i�y��@��� 1

2mð�y

2�y1 þ �1�2Þ

� g2

8j�j4 � 1

2m2j�j2 � gm

4j�j2ð�þ�yÞ � g

2

� ð��y2�

y1 þ�y�1�2Þ: (8)

This is the (2þ 1)-dimensional reduction of the originalWZ-SUSY model in 3þ 1 dimensions [1,2].Supercurrent and supercharge.—SUSY leads to a con-

served supercurrent, whose conserved supercharges aregenerators of SUSY. The supercurrent is defined by�Rdtd2xL ¼ R

dtd2xy�y@�J�s . The supercharges are

then given by Q ¼ Rd2xJ0s ðxÞ and Qy. The SUSY trans-

formation generated by Q for a field O reads �O ¼�iy�y½Q;O��. We focus on the on-shell model withthe Z2 symmetry spontaneously broken, where the on-shell supercurrent [19] is given by J�s ¼ i��� �@ �þi g2 ð�2 � 2m�=gÞ�y���. The SUSY spontaneous break-

ing is signaled by hfQ;Ogi � 0 for a fermionic operatorO.However, for this simplest SUSY model, the SUSY is notspontaneously broken at zero temperature [2].Nonrenormalization.—In this simplest WZ-SUSY

model, single-particle Green’s functions are not renormal-ized. For example, the renormalization to the Klein-Gordon field’s propagator in a one-loop self-energycalculation is given by q2 �m2 ! q2 �m2

�ðqÞ with [12]

m�ðqÞ ¼ mþ gRhAi0 þOðg2RhAi20Þ, where A ¼ Re�. For

2þ 1 dimensions, due to the nonzero anomalous criticalexponents [20], the coupling constant may be renormalizedto gR. However, hAi0 / hfQ; �gi0 ¼ 0 because the SUSY isnot spontaneously broken. The mass of the Dirac field isalso not renormalized as required by SUSY. Therefore, theGreen’s functions, both of the Dirac and Klein-Gordonfields, are not renormalized from their free version.The spectral functions of the Green’s functions can be

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measured by the single-particle spectroscopic techniquewhich has been developed recently [13]. The nonrenorm-alization of the Green’s functions implies sharp peaks intheir spectral functions, with identical relativistic disper-sions for the atoms and molecules. Experimentally, thiswould be the hallmark of achieving SUSY.

Thermal breaking of SUSY.—By replacing t by i�,the imaginary time, the Euclidean version of Lagrangian(8) describes the WZ-SUSY model in finite temperatureT. When T � 0, SUSY is always broken becausehfQ;Qy�ygiT ¼ h��P�iT � 0 with P� being the energy-

momentum operator [14], due to the nonvanishing thermalenergy. This SUSY thermal breaking is accompanied by athermal Goldstone fermion (phonino) but not necessarilyby a phonon because the Lorentz symmetry is also brokenby hP0iT � 0 [12]. The phonino dispersion is given by [12]q0 ¼ �vssjqj, where the SUSY sound velocity vss ¼vs=3 for T � m and vss ¼ Tvs=m for T m.

To detect the phonino mode, one can consider the re-sponse to an external ‘‘fermionic’’ field coupled to thesupercurrent. The phonino is a pole of the supercurrent-supercurrent correlation function. This external fermionicfield can be a combination of an external photon withanother hyperfine state of the fermionic atom which isdecoupled to the mixture. We have studied this kind ofSUSY response theory for a nonrelativistic SUSY mixture[7]. However, in the present case, the supercurrent is notsimple, and thus the coupling between the external fermi-onic field and the supercurrent is not that easy to beexperimentally handled.

By replacing hAi0 by hAiT , the masses are thermallyrenormalized. The masses of A, B (� ¼ Aþ iB), and thespinor � have been calculated in low temperature and hightemperature limits [12]. Namely, in 2þ 1 dimensions up toone loop, for T m, one hasmB ¼ m,m2

A �m2B / g2m�,

and m� �mA / g2m�, where � ¼ 2T�m e

�m=T ; for T � m,

mB ¼ m, m2A ¼ m2 � 2g2T, and m2

� ¼ m2 � g2T. These

unequal masses of these fields signal SUSY breaking andcan be probed quantitatively. We expect spectroscopymeasurements to show double peaks in the molecule spec-tral function due to the unequal masses, while the atomspectral function has a single peak with a mass of the Diracfield equal to neither mA nor mB.

Experimental challenges.—Optical lattices that trapcold atoms can be routinely set up in the laboratory. Thestaggered Peierls phase originates from production of theartificial magnetic field [16]. As discussed earlier, oneneeds to tune three parameters to achieve SUSY: atom-atom interaction, molecule-molecule interaction, andmolecule velocity. The former two may be done by adjust-ing the real magnetic field in a Feshbach resonance, whilethe latter may be related to the interaction between thelaser field and the Feshbach molecule. These are all ac-hievable within existing experimental capabilities. Perhapsthe biggest challenge is finding the right fermionic atom,which needs to have a highly tunable interaction through a

p-wave Feshbach resonance. It also needs to support a suf-ficiently stable dimolecule state, whose condensate pro-vides the source term in Eq. (6), which gives rise to equalparticle masses. Experimentally, one needs to overcomethe atom loss due to the heating of the atom gas caused bythree- and four-body collisions. Without the last ingre-dient, however, one can still realize the massless versionof the WZ-SUSY model, Eq. (5), which already containsvery rich SUSY physics. Despite these and other chal-lenges, we believe simulating the WZ-SUSY model byusing cold atom-molecule mixtures is a worthwhile en-deavor, as the present model may be generalized to (3þ 1)dimensions, which provides new opportunities to explorethe real space-time SUSY physics.Y.Y. thanks Q. J. Chen, C. Liu, andM.X. Luo for helpful

discussions. This work was supported by NNSF of China,the national program for basic research of MOSTof China,and the Key Lab of Frontiers in Theoretical Physics of CAS(Y.Y.) and by National Science Foundation GrantsNo. DMR-0704133 and No. DMR-1004545 (K.Y.).

[1] J. Wess and B. Zumino, Nucl. Phys. B70, 39 (1974).[2] See, e.g., S. Weinberg, The Quantum Theory of Fields, III

(Cambridge University Press, Cambridge, England, 2000).[3] M. Snoek,M.Haque, S. Vandoren, andH. T. C. Stoof, Phys.

Rev. Lett. 95, 250401 (2005); M. Snoek, S. Vandoren, andH. T. C. Stoof, Phys. Rev. A 74, 033607 (2006).

[4] A. Imambekov and E. Demler, Phys. Rev. A 73, 021602(R) (2006); Ann. Phys. (N.Y.) 321, 2390 (2006).

[5] G. S. Lozano et al., Phys. Rev. A 75, 023608 (2007).[6] Y. Yu and K. Yang, Phys. Rev. Lett. 100, 090404 (2008).[7] T. Shi, Y. Yu, and C. P. Sun, Phys. Rev. A 81, 011604(R)

(2010).[8] S. L. Zhu, B. Wang, and L.M. Duan, Phys. Rev. Lett. 98,

260402 (2007); E. Zhao and A. Paramekanti, ibid. 97,230404 (2006); L. B. Shao et al., ibid. 101, 246810 (2008).

[9] S. S. Lee, Phys. Rev. B 76, 075103 (2007).[10] X. J. Liu, X. Liu, C. Wu, and J. Sinova, Phys. Rev. A 81,

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[11] See, e.g., Z. Komargodski and D. Shih, J. High EnergyPhys. 04 (2009) 93, and references therein.

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[13] T. L. Dao et al., Phys. Rev. Lett. 98, 240402 (2007); J. T.Stewart, J. P. Gaebler, and D. S. Jin, Nature (London) 454,744 (2008).

[14] D. Buchholz and I. Ojima, Nucl. Phys. B498, 228 (1997).[15] See, e.g., M. Beccaria, M. Campostrini, and A. Feo,

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[16] Y. J. Lin et al., Phys. Rev. Lett. 102, 130401 (2009).[17] J. P. Gaebler et al., Phys. Rev. Lett. 98, 200403 (2007).[18] See, e.g., R. A. Duine and H. T. C. Stoof, Phys. Rep. 396,

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PRL 105, 150605 (2010) P HY S I CA L R EV I EW LE T T E R Sweek ending

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