The 1D spin-12 AF-Heisenberg model in a staggered field
英语作文,大学里令我印象最深刻的课程

英语作文,大学里令我印象最深刻的课程全文共3篇示例,供读者参考篇1The Best Class Ever!Hi there! My name is Timmy and I'm 8 years old. Today I want to tell you about the most awesome, super cool, and just plain amazing class I took when I was in university a few years back. Yeah, that's right - university! I know I'm just a kid but I'm really smart. I even skipped a few grades because regular school was just too easy for me.Anyway, let me tell you about this crazy great class. It was called "Intro to Coding and Computer Programming" and it was taught by the funniest, nicest professor ever - Professor Jackie Codemaster. I'll never forget the first day I walked into that giant lecture hall. There must have been like a million students in there! Okay, maybe not a million, but definitely a few hundred at least.Professor Codemaster came bounding into the room full of energy. She had these really wild pink and blue streaks in her hair and was wearing ripped jeans with cool patterns all over them. I could tell right away this wasn't going to be a boring, lame class.The professor started cracking jokes from the very beginning to get everyone loosened up and laughing.Then she mind-blew all of us by writing some computer code up on the overhead projector. It looked like a total jumble of numbers, letters, and symbols to me at first. But Professor Codemaster explained it all in a way that actually made sense! She broke it down step-by-step and before I knew it, I was understanding the basic logic behind coding and programming. It was like learning a brand new language, but one that gave instructions to computers instead of humans. So cool!Over the next few months, we learned all sorts of programming languages like Python, Java, C++, and more. At first it was really hard and frustrating. I'll admit there were times I got mad and wanted to give up because I just couldn't get the hang of it. Professor Codemaster must have sensed my struggles because she went out of her way to meet with me one-on-one during office hours. She was super patient, encouraging, and didn't make me feel dumb at all for asking tons of questions. Gradually, it started to click and I was writing basic programs and making my computer do all kinds of neat tricks!The hands-on coding assignments and projects were my favorite part of the class. We made simple games, apps, and evenprogramming driving little robots to collect things and navigate mazes. Professor Codemaster turned it all into fun competitions and gave out prizes to the most creative and innovative projects. I'll never forget my proud smile when I won a Codemaster Medal for my "Mathinator 3000" program that could solve big math problems lickety-split.Towards the end of the semester, we had a huge interactive showcase day where we presented our final projects to the whole class, professors, tech company reps, and even our families. My little sister Susie couldn't believe her eyes when my program made the computer talk out loud with funny jokes and sound effects! Mom and Dad were bursting with pride, even though they didn't really understand any of the code stuff going on.I learned so much in that intro coding course, and it totally inspired me to keep studying computer science through school. In fact, I just accepted an internship this summer at a major tech company here in Silicon Valley! Pretty great for an 8-year-old, right?More than all the programming knowledge though, Professor Codemaster taught me valuable lessons about having a positive attitude, never giving up when things get hard, and using creativity to solve problems in fun new ways. Thanks to herawesomeness, I discovered my passion for tech and innovation. Who knows, maybe someday I'll be a professor myself, inspiring the next generation of kid coders and programmers! But for now, I've got to get back to working on my latest app idea - a fart sound board. Yo, coding is the best!篇2The Most Awesome Class Ever!You'll never guess what was the coolest, most fun, and straight up amazing class I took in college! It was Intro to Quantum Physics 201. I know, I know, you're probably thinking "Whoa, that sounds crazy hard and boring." But believe me, it was the total opposite of boring. It was mind-blowing!The very first day of class, Professor Everett came bouncing in with this giant smile on his face. He had crazy curly hair that stuck out in every direction, like he just rolled out of bed. Instead of just droning on about the syllabus like most professors, he started talking about how nothing is really solid - everything is made up of these tiny subatomic particles whizzing around. It's all just empty space and energy!Then he grabbed a baseball off his desk and yelled "Think fast!" and chucked it straight at my head! I flinched, but the balljust passed right through me. The whole class gasped. Turns out, it was just a hologram! Professor Everett cackled and said "You see? There's nothing really there! Your eyes were playing tricks on you."From that moment on, I was hooked. Every class was filled with demonstrations and experiments that scrambled your brain. Like the time we calculated that if you cooled a object to absolute zero, it would exist in every possible state at once! Or when we proved that a particle can somehow be in two places at the same time. Woah!My favorite was the double slit experiment. Professor Everett set up this big vacuum chamber with a laser shooting a beam of light particles at these tiny slits. You'd think the particles would just make two lines on the other side where the slits were. But the crazy thing is, they created this trippy interference pattern, like waves rippling on water!Professor Everett explained that's because the particles were behaving like waves, but also like particles at the same time. They were interfering with themselves, which is nuts! It totally shattered my assumptions about how the universe works on the smallest scales.After class, I went up to the professor and asked "But how can a particle act like a wave? And be in multiple places? It doesn't make any sense!" You know what he said? He smiled real big and said "Jeremy, if you think that's weird, you're not ready for what comes next!"No joke, this guy lived and breathed quantum physics. During exams, he'd walk around the room with a cat sealed in a box. He claimed that until somebody opened the box, the cat was both alive AND dead at the same time because of something called quantum superposition. My mind was blown every single class!It wasn't all fun and games though. The math and problem sets were no joke. Things like wave functions, Heisenberg's Uncertainty Principle, and Schrödinger's equation made my head spin. I spent long nights in the library with my study group, going over practice problems until 2am. Pulling all-nighters before tests was pretty common.The lowest grade on the midterm was a 12%. Seeing that soul-crushing number in red ink practically gave me a heart attack. I thought I was brilliant at first when I got a 63%, until Professor Everett handed them back wearing afdisappointed frown, saying "I expected better from you all."Despite being one of the hardest classes I've ever taken, it was also one of the most rewarding. Sure, I didn't understand half the crazy concepts we learned about like quantum entanglement, quantum tunneling, or the multiverse theory. But it opened my eyes to this strange, bizarre realm operating by rules that seem to defy logic and common sense.On the last day of class, Professor Everett brought in this gigantic mainframe computer that filled the entire lecture hall. He told us it could simulate incredibly complex quantum interactions using quantum bits or "qubits." As a demonstration, he showed us two particles that became "entangled" - whatever happened to one would instantly affect the other, even if they were billions of miles apart. My jaw hit the floor.Then the professor said something I'll never forget. He looked out at all of us and said in this peaceful, reassuring voice: "The universe is not only stranger than you imagine... it is stranger than you can imagine. Quantum physics is showing us that reality itself is vastly more wondrous and mystifying than our everyday experiences suggest."As I walked out of that last lecture, it felt like someone had re-adjusted how my brain perceived everything in existence. Solid objects, light, gravity, time...none of it was as real orconcrete as I thought. It was all fuzzy at the subatomic level, made up of weird quantum probabilities and uncertainties. Things I took for granted, like causality, suddenly seemed up for debate in the quantum realm.While it didn't give me any definite answers, Intro to Quantum Physics 201 exposed me to the deliciouslymind-bending mysteries buried in the deepest fabric of our universe. It shattered my assumptions about how reality works at the fundamental level. More importantly, it filled me with a sense of awe about the bizarre, unintuitive behavior of the quantum world that our human minds struggle to fully grasp.Since that class, I've had a constant feeling of amazement and curiosity about the true nature of our existence. Like there are Hidden realities and dimensions peeking through the cracks of our surface-level experience, bizarre quantum effects leaking into the macroscopic world. It awakened a burning inquisitiveness in me about all the secrets and strangeness lurking in the universe that we've barely begun to glimpse.So if I could say one thing to anyone considering taking Intro to Quantum Physics 201, it would be: get ready to have your mind completely blown away! Be prepared to question everything you think you know about reality. Because studyingquantum physics is like taking a journey through a psychedelic, logic-defying alternate dimension. It's batty, insane, and utterly captivating!篇3The Bestest Class Ever!Wow, you want to hear about the coolest class I took in college? It was seriously awesome sauce! I'll never forget that class for as long as I live.It was called "Unicorns and Rainbows 101" and it was taught by the most magical professor of all time, Professor Twinkleberry. She was this tiny little lady with bright purple hair and stars painted all over her face. I'm not even kidding!On the very first day, she came prancing into the room on her tippy-toes, wearing a rainbow tutu and giant fuzzy slippers shaped like unicorn heads. "Welcome, my little stardust buddies!" she bellowed in a super high-pitched voice. "Who's ready to go on a journey to the most whimsical place of all?"We were all like "Uhh...what?" because none of us nerdy college kids had any idea what this crazy lady was talking about. But then she told us that for the whole semester, we'd belearning all about the magic of unicorns, rainbows, and friendship! Yeah, for real.At first, I kind of thought the class would be a total snoozefest. I only signed up because I needed one more elective to graduate. But after that first bonkers day, I was hooked!Pretty much every class was insane in the most wonderful way. Sometimes Professor Twinkleberry would make us all put on paper bag puppet unicorn horns and act out stories from her favorite unicorn fable books. Other times, we'd have to dance around passing a rainbow ribbon and humming made-up unicorn songs.My personal favorite was when we all got to make unicorn frap smoothies! Professor Twinkleberry gave us all these crazy ingredients like edible glitter, gummy worms, and bottles of sprinkle magic dust. We got to blend up our own smoothies and add whatever wild toppings we wanted. I literally drank a sunshiny glittery smoothie through a crazy straw shaped like a unicorn horn's spiral. It was so sugary and silly, but absolutely delicious!The assignments were just as ridiculous and wonderful. One time, we had to write a short story from the perspective of a grumpy fairy who was sick of dodging pooped rainbows.Another paper needed to be a haiku poem about why best friends are more awesome than ice cream sundaes.Then there was the big group project, which pretty much every other class dreads. But leave it to Professor Twinkleberry to make it magically delightful! We had to break into teams and come up with a brand new unicorn fairy tale book to read to elementary schoolers. My team's book was called "Sir Sparklelips Poots a Party"...it was about a unicorn who couldn't stop farting rainbows and stink clouds. Everybody thought it was so dumb and hysterical!On the last day of class, Professor Twinkleberry told us the whole unicorn and rainbows thing was just her extraordinary way to teach bigger life lessons with whimsy. "You see, my stardust angels, unicorns represent purity, bravery, and individualism. Rainbows symbolize diversity, optimism, and finding the bright side to any storm clouds. And friendship...well, that's the rarest, most magical element of all!"As cheesy as it sounds, that class honestly did make me look at the world a little differently. I started to appreciate the simple pops of color and magic that are all around us, if you just take a second to scout them out. I tried to stop sweating the small stuff and be more positive, the way unicorns and rainbows are. And Imade some of the grooviest friends from my smoothie-making team!So yeah, Unicorns and Rainbows 101 was hands down, no contest, the most amazingly absurd yet wholeheartedly impactful class I'll never forget. If you ever get the chance to take it, do it! Your inner child's mind will get blown to rainbow dust. Thanks a million, Professor Twinkleberry, for helping this student see the magic in the day-to-day. I'll never look at a unicorn or double rainbow the same way again!。
Two Qubit Entanglement in $XYZ$ Magnetic Chain with DM Antisymmetric Anisotropic Exchange I

a r X i v :0705.679v 1 [q u a n t -p h ] 4 M a y 2007APS/123-QEDTwo Qubit Entanglement in XY Z Magnetic Chain with DM AntisymmetricAnisotropic Exchange InteractionZeynep Nilhan GURKAN ∗and Oktay K.PASHAEV †Department of Mathematics,Izmir Institute of Technology,Urla-Izmir,35430,Turkey(Dated:February 1,2008)In the present paper we study two qubit entanglement in the most general XY Z Heisenberg mag-netic chain with (non)homogeneous magnetic fields and the DM anisotropic antisymmetric exchange interaction,arising from the spin-orbit coupling .The model includes all known results as particular cases,for both antiferromagnetic and ferromagnetic XX,XY,XXX,XXZ,XY Z chains.The con-currence of two qubit thermal entanglement and its dependence on anisotropic parameters,external magnetic field and temperature are studied in details.We found that in all cases,inclusion of the DM interaction,which is responsible for weak ferromagnetism in mainly antiferromagnetic crystals and spin arrangement in low symmetry magnets,creates (when it does not exist)or strengthens (when it exists)entanglement in XY Z spin chain.This implies existence of a relation between ar-rangement of spins and entanglement,in which the DM coupling plays an essential role.It suggests also that anisotropic antisymmetric exchange interaction could be an efficient control parameter of entanglement in the general XY Z case.PACS numbers:Valid PACS appear hereI.INTRODUCTIONEntanglement property has been discussed at the early years of quantum mechanics as specifically quantum me-chanical nonlocal correlation [1]-[3]and it becomes re-cently a key point of quantum information theory [4].For entangled subsystems,the whole state vector cannot be separated into a product of the states of the subsys-tems,and the last ones are no longer independent even if they are far spatially separated.A measurement on one subsystem not only gives information about the other subsystem,but also provides possibilities of manipulat-ing it.Therefore in quantum computations the entangle-ment becomes main tool of information processing,such as quantum cryptography,teleportation and etc.For realizing quantum logic gates,several models have been proposed and demonstrated by experiments in cav-ity QED,ion trap,and NMR [5],[6].Due to intrinsic pairwise character of the entanglement,in all these cases important is to find entangled qubit pairs.Generic two qubit state is characterized by 6real degrees of freedom.While separable two qubit state has only four degrees of freedom.It is clear that single qubit gates are unable to generate entanglement in an N qubit system,because starting from separable state we will obtain another sep-arable state with transformed by gates separable qubits.Then to prepare an entangled state one needs inter qubit interactions which is a two qubit gate.The well known example of two qubit gate generating entanglement is Controlled Not (CNOT)gate [7].Moreover realization of two qubit controlled gates is a necessary requirement for implementation of the universal quantum computa-k ln 3.Important point is how to increase entanglement in sit-uation where it exists already or to create entangle-ment in situation when it does not exist.Certainly this can be expected from a generalization of bilinear spin-spin interaction form.Around 50years ago to ex-plain weak ferromagnetism of antiferromagnetic crystals (α−F e 2O 3,MnCO 3and CrF 3),which has been contro-versial problem for a decade,Dzialoshinski [14]from phe-nomenological arguments and Moriya [15]from micro-scopic grounds have introduced anisotropic antisymmet-ric exchange interaction,the Dzialoshinski-Moriya (DM)interaction,expressed byD·[ S 1× S 2].This interaction arises from extending the Anderson‘stheory of superexchange interaction by including the spin orbit coupling effect [15],and it is important not only for2 weak ferromagnetism but also for the spin arrangement inantiferromagnets of low symmetry.In the present paperwe show that the Dzialoshinski-Moriya interaction playsan essential role for entanglement of two qubits in mag-netic spin chain model of most general XY Z form.Wefind that in all cases,inclusion of the DM interaction cre-ates(when it does not exist)or strengthens(when it ex-ists)entanglement.In particular case of isotropic Heisen-berg XXX model discussed above,inclusion of this termincreases entanglement for antiferromagnetic case andeven in ferromagnetic case,for sufficiently strong cou-pling D>(kT sinh−1e|J|/kT−J2)1/2,it creates entan-glement.These results imply existence of an intimaterelation between weak ferromagnetism of mainly antifer-romagnetic crystals and the spin arrangement in antifer-romagnets of low symmetry,with entanglement of spins.Moreover it shows that the DM interaction could be anefficient control parameter of entanglement in the generalXY Z model.II.XY Z HEISENBERG MODELThe Hamiltonian of XY Z model for N qubits isH=N−1i=112=D2[J xσx1σx2+J yσy1σy2+J zσz1σz2+(B+b)σz1+(B−b)σz2+D(σx1σy2−σy1σx2)](2) and in the matrix formH=266666664J z2 0−J z2+iD0 0J x+J y2−b0J x−J y2−B377777775.To study thermal entanglementfirstly we need to obtain all the eigenvalues and eigenstates of the Hamiltonian(2): H|Ψi =E i|Ψi ,(i=1,2,3,4).The eigenvalues(energy levels)are:E1=J z2−νE2=J z2+νwhere J x−J y2≡J+,µ≡b2+J2++D2and corresponding wave functions are|Ψ1 =12(µ2+Bν)2664J−00−(B+µ)3775|Ψ2 =12(µ2−Bν)2664J−00−(B−µ)3775|Ψ3 =−i2(ν2+bν)26640J++iD−(b+ν)03775|Ψ4 =12(ν2−bν)26640J++iD−(b−ν)03775For B=0,b=0,D=0the wave functions reduce tothe Bell states|Ψ2 −→|B0 =12(|00 +|11 )(3)|Ψ4 −→|B1 =12(|01 +|10 )(4)|Ψ3 −→|B2 =12(|01 −|10 )(5)|Ψ1 −→|B3 =12(|00 −|11 )(6)The state of the system at thermal equilibrium is deter-mined by the density matrixρ(T)=e−H/kTZ,(7)where Z is the partition function,k is Boltzmann’s con-stant and T is the temperature.Then for Hamiltonian(2)wefinde−H/kT=I+…−H2!…−H n!…−H3whereA 11=−e −J zkT−BkT–A 14=−e−J zµsinh µ2kT»coshννsinh ν2kT J ++iDkT A 32=−eJ zνsinh ν2kT»cosh ννsinhν2kTJ −kT A 44=e−JzkT+BkT–(9)andZ =T r [e−H/kT]=2h e−J zkT +eJ zkTi .As ρ(T )represents a thermal state,the entanglement in this state is called the thermal entanglement .The concurrence C (the order parameter of entanglement)is defined as [16],[17]C =max {λ1−λ2−λ3−λ4,0}(10)where λi (i =1,2,3,4)are the ordered square roots of the eigenvalues of the operatorρ12=ρ(σy ⊗σy )ρ∗(σy ⊗σy )(11)and λ1>λ2>λ3>λ4>0.The concurrence is bounded function 0≤C ≤1.When the concurrence C =0,states are unentangled;when C =1,states are maximally entangled.In our case:λ1,2=e−J zZ˛˛˛˛˛˛s µ2sinh 2µµsinh µkT1+J 2++D 2kT∓qνsinhνB 2+J 2−,ν≡q2[J z σz 1σz 2+(B +b )σz 1+(B −b )σz 2+D (σx 1σy 2−σy 1σx2)]The eigenvalues areλ1,2=e −J zZ(13)λ3,4=eJ zZ˛˛˛˛˛rν2sinh 2ννsinhνb 2+D 2and Z =T r [e −H/kT]=2»e−J zkT+e J zb 2+D 2Z>λ3=λ4=e −J z /2kT2kTand the concurrence is C 12=max {−e J z /2kT2kT,0}=0(15)and there is no entanglement.2.Ferromagnetic Case (J z <0):The ordered eigenvalues areλ1=λ2e |J z |/2kTZ.(16)where Z =4cosh|J z |2cosh|J z |Z,λ3=λ4=e −J z /2kT kT+eJ z /2kTiand the concur-renceC 12=max {−e J z /2kTkT+e J z /kT ),0}=0(19)and there is no entanglement.C.Ising Model with Nonhomogeneous MagneticField (B =0,b =0,D =0)The concurrence is C 12=max {−e J z /2kTkT),0}=0(20)and there is no entanglement.As we can see in pure Ising model and including homoge-neous (B)and nonhomogeneous (b)magnetic fields no entan-glement occurs [19],[20],[21].4D.Ising Model with DM Coupling(B =0,b =0,D =0)The eigenvalues areλ1=e (J z +2D )/2kTZ(21)λ3=λ4=e −J z /2kTkT+e−J z /2kTi.1.Antiferromagnetic Case (J z >0):Ordering the eigenvalues λ1>λ2>λ3=λ4we have theconcurrenceC 12=max {sinh |D |cosh|D |kT≤e −J z /kT .When sinh|D |kT −e −J z /kT kT+e −J z /kT.(23)Moreover states become more entangled for low temper-atures:maximally entangled for any D and T =0so that (lim kT →0C 12=1)and for stronger DM cou-pling lim D →∞C 12=1.With T growing,D min =kT sinh −1e −J z /kT is growing so that we need to increase D to have entangled states.2.Ferromagnetic Case (J z <0):a)With weak DM coupling |D |<|J z |there is no entangle-ment Ordering the eigenvalues λ3=λ4>λ1>λ2we have the concurrenceC 12=max {−cosh|D |cosh|D |kT −e |J z |/2kTkT+e |J z |/2kT,0}(25)Then C 12=0(no entanglement)if sinh|D |kT>e |J z |/kT or |D |>|J z |+kT kT −e|J z |/kTkT+e |J z |/kT.(26)Moreover states become more entangled for low temper-atures lim kT →0C 12=1and for stronger DM coupling lim D →∞C 12=1.As we can see there is entanglement even in ferromagnetic case with sufficiently strong DM parison of (23)and (26)shows that in anti-ferromagnetic case,states can be more easily entangled then in the ferro-magnetic oneIV.XX HEISENBERG MODELFor J z =0,J x =J y ≡J ,the Hamiltonian isH =1Z (27)λ3,4=11+J 2+D 2kT∓√νsinhνJ 2+b 2+D 2andZ =T r [e −H/kT]=2»coshB kT–.A.Pure XX Heisenberg Model (B =0,b =0,D =0)The eigenvalues areλ1=e J/kTZ,λ4=e −J/kTkT −1kT+1,0}and for a)sinhJ kT −1kT+1so that lim T →0C 12=1(29)b)sinhJk [sinh −11]−1|}T C(30)2.Ferromagnetic Case J <0he eigenvalues are λ1=e −|J |/kTZ,λ4=e |J |/kTkT −1kT+1,0}(32)and a)sinh|J |kT −1kT+15b)sinh|J |k [sinh −11]−1|}T c(33)In both cases states are entangled at sufficiently small tem-perature T <T C =|J |Z,λ2=λ3=1Z .(34)whereZ =2»coshBkT –.(35)and the concurrence is C 12=max {sinhJcosh JkT,0}anda)sinh|J |kT −1kT+coshBkT≤1,C 12=0no entanglement forT >|J |{zZ,λ3=e −β/kTZ(37)where β>0,β=√kT).The ordered eigenvalues are λ4>λ3>λ1=λ2and the concur-rence isC 12=max {sinh νcoshνJ 2+D 2:a)sinh νkT −1kT+1b)sinhν2[J x σx 1σx 2+J y σy 1σy 2+(B +b )σz 1+(B −b )σz 2+D (σx 1σy 2−σy 1σx2)]The eigenvalues areλ1,2=11+J 2−kT∓J −kT ˛˛˛˛˛˛(39)λ3,4=11+J 2++D 2kT ∓qνsinhνB 2+J 2−,ν=q2andZ =T r [e−H/kT]=2hcoshµkTi.(40)A.Pure XY Heisenberg Model (B =0,b =0,D =0)The eigenvalues are λ1=e J −/kTZ ,λ3=e J +/kTZ,whereZ =2»coshJ −kT–.(41)For J x =J (1+γ)and J y =J (1−γ)so that J +=J,J −=Jγ,the eigenvalues are λ1=e Jγ/kTZ,λ3=e J/kTZ,(42)1.Anti-ferromagnetic Case J x >0and J y >0The ordered eigenvalues are λ3>λ1>λ2>λ4and the concurrenceC 12=max {sinhJ +kT kT+coshJ +kT>coshJ −kT −coshJ −coshJ −kT,(lim T →0C 12=1)b)sinhJ +kT⇒C 12=0there is no entanglement.In Fig.1,we plot the concurrence C 12in XY Heisenbergantiferromagnet as function of J+J+6FIG.1:Concurrence C 12in XY antiferromagnet as functionof J +J +2.Ferromagnetic Case J x <0and J y <0C 12=max {sinh|J −|kTkT+coshJ +kT>coshJ +kT−cosh|J −|cosh|J −|kT(45)lim T →0C 12=1(46)b)sinh|J −|kT⇒C 12=0there is no entanglement.In Fig.2,we plot the concurrence C 12in XY Heisenbergferromagnet as function of J+|J +|.FIG.2:Concurrence C 12in XY ferromagnet as function ofJ +J +|Thermal entanglement in XY chain was studied in [24],[26]and [25]in the presence of external magnetic field B and in [27]by introducing non-uniform magnetic field b .B.XY Heisenberg Model with DM Coupling(B =0,b =0,D =0)The eigenvalues areλ1=e J −/kT Z(47)λ3=eqZ,λ4=e−qZ(48)whereZ =224cosh|J −|J 2++D 2J 2++D 2kTJ 2++D 2kT,0}.(50)It shows that for any temperature T we can adjust sufficiently strong DM coupling D to have entanglement.a)sinhqkT>coshJ −J 2++D 2kTJ 2++D 2kT(51)b)sinhqkT≤coshJ −2[J (σx 1σx 2+σy 1σy 2+σz 1σz 2)+(B +b )σz 1(52)+(B −b )σz 2+D (σx 1σy 2−σy 1σx2)].The eigenvalues are λ1,2=e −J/2kTZ ˛˛˛˛˛r ν2sinh 2νJ 2+D 2kT ˛˛˛˛˛whereZ =2»e −J/2kt coshBJ 2+b 2+D 27A.Pure XXX Model (B =0,b =0,D =0)The eigenvalues are λ1,2=e −J/2kTZ,λ4=e 3J/2kTkT–(56)1.Antiferromagnetic case (J >0):The concurrence isC 12=max {e 2J/kT −3kT>e −J/kTC 12=sinh J e −J/2kT+coshJk ln 3entangle-ment occurs and lim T →0C 12=1b)sinh JkTkT+e |J |/kT,0}=0and no entanglement occurs.Thus,for ferromagnets,spins are always disentangled,while entanglement is observed for antiferromagnets [9],[13].B.XXX Heisenberg Model with Magnetic Field(B =0)The eigenvalues are λ1,2=e −J/2kTZ ,λ4=e 3J/2kTkT+e J/2kT coshJe 2J/kT +1+2coshBkT>e −J/kT,C 12=sinh Je −J/2kT coshB 2kTFor sufficiently small temperature T <2JkT<e −J/kT ⇒C 12=0there is no entanglement.2.Ferromagnetic case (J <0):C 12=max {−cosh|J |cosh |J |kT,0}=0and no en-tanglement occurs.Therefore inclusion of magnetic field does not change the result.Entanglement in XXX Heisenberg model with magnetic field has been studied in [9].C.XXX Heisenberg Model with DM Coupling(B =0,b =0,D =0)The eigenvalues areλ1,2=e −J/2kTJ 2+D 2)/2kTJ 2+D 2)/2kTJ 2+D 2J 2+D 2e −J/kT+cosh√kT,0}(65)a)sinh√kT>e −J/kT C 12=sinh√kT−e −J/kTJ 2+D 2kT sinh −1e −J/kT −J 2(67)there is entanglement.b)sinh √kT≤e −J/kT ⇒C 12=0there is no entangle-ment.2.Ferromagnetic Case (J <0):The concurrence isC 12=max {sinh√kT−e |J |/kTJ 2+D 2J 2+D 2J 2+D 2e |J |/kT +cosh√kT(69)8For a given temperature,whenD >p J 2+D 22[J (σx 1σx 2+σy 1σy 2+∆σz 1σz 2)+(B +b )σz1(71)+(B −b )σz 2+D (σx 1σy 2−σy 1σx2)].where ∆≡J z /J .The eigenvalues are λ1,2=e −J zZ(72)λ3,4=eJ zZ˛˛˛˛˛r ν2sinh 2νJ 2+D 2kT ˛˛˛˛˛where µ=B ,ν=√kT+e J z /2kT coshνZ,λ3=e (J z −2J )/2kTZ(73)where β=J and Z =2he −J z /2kT +e J z /2kT coshJkT −e −J z /kTkT+e −J z /kT,0}(74)a)sinhJkT −e −J z /kT kT+e −J z /kT(75)b)sinhJkTkT+e |J z |/kT,0}=0(76)and no entanglement.For ∆=1the anisotropic model reduces the isotropic XXX model,and the concurrence reduces toC 12=max {e 2J/kT −3k ln 3the thermal entanglement disap-pears.2.Ferromagnetic Case (J <0):For ∆<1The concurrence isC 12=max {sinh |J |cosh|J |kT>e |J z |/kTC 12=sinh |J |cosh JkT≤e |J z |/kT ⇒C 12=0For ∆≥1the concurrence isC 12=max {−cosh|J |cosh|J |Z,λ3=e(J z −2√Z(81)λ4=e(J z +2√Z(82)whereZ =2»e −J z /2kT +e J z /2kTcosh√kT–(83)91.Antiferromagnetic case (J >0):The concurrence isC 12=max {sinh√kT −e −J z /kTJ 2+D 2J 2+D 2J 2+D 2cosh√kT+e −J z /kT(85)b)sinh √kT<e −J z /kT ⇒C 12=0Comparison with (75)shows that with growth of D entanglement increases.2.Ferromagnetic Case (J <0):a)For small D <D c =√J 2+D 2cosh√kT+e |J z |/kT,0}(86)and entanglement increases with growing D .Entanglement for XXZ Heisenberg model was considered in [29]and effect of DM interaction on XXZ model in [28].VIII.XY Z HEISENBERG MODELA.Pure XYZ Model (B =0,b =0,D =0)The eigenvalues areλ1=e (−J z −2J −)/2kTZ(87)λ3=e (J z −2J +)/2kTZ(88)whereZ =2»e −J z /2kT coshJ −kT–(89)1.Antiferromagnetic Case :J z >J y >J x >0⇒J +>0,J =−|J −|<0.The biggest eigenvalue is λ4=e|J z |+2|J +|Zand the concurrence isC 12=max {sinhJ +kT e −J z /kTkT+coshJ −kT−coshJ −Zand the concurrence isC 12=max {sinh|J −|kT e −|J z |/kTkT+cosh|J +|kT−cosh|J +|10B.XY Z Model with Magnetic Field(B=0,b=0,D=0)The full anisotropic XY Z Heisenberg spin two-qubit sys-tem in which a magneticfield is applied along the z-axis,wasstudied by Zhou et al.The enhancement of the entanglementfor particularfixed magneticfield by increasing the z-compo-nent of the coupling coefficient between the neighboring spins,was their mainfinding.C.XY Z Model with DM Coupling(B=0,b=0,D=0)λ1=e(−J z+2J−)/2kTZ(92)λ3=e(J z+2ν)/2kTZ(93)whereν=qkT +e J z/2kT coshνkT−e−J z/kT cosh J−coshνkT,0}(95) and entanglement occurs whensinh q kT>e−J z/kT cosh J−kT−e|J z|/kT cosh J−coshνkT,0}(96) and entanglement occurs for sufficiently strong Dsinh q kT>e|J z|/kT cosh J−11IX.CONCLUSIONWe found in general ifλ1(the largest eigenvalue)is degen-erate withλ2then no entanglement occurs.From our con-sideration follows that in all cases decreasing of temperature increases entanglement,if it exists.So that at zero temper-ature T=0states are completely entangled C12=1.This fact links entanglement with the Mattis-Lieb[10]theorem on absence of phase transitions in one dimension at T=0.More-over,inclusion of the DM coupling always increases entangle-ment,this is why it could be an efficient control parameter of the entanglement.Our results show existence of intrinsic re-lation between weak ferromagnetism of mainly antiferromag-netic crystals and spin arrangement in(anti)ferromagnets of low symmetry with entanglement.Very recently thermal entanglement of a two-qubit isotropic Heisenberg chain in presence of the Dzyaloshinski-Moriya anisotropic antisymmetric interaction and entanglement tele-portation,when using two independent Heisenberg XXX chains as quantum channel,have been investigated[30].It was found that the DM interaction can excite the entangle-ment and teleportationfidelity.As was noticed DM inter-action could be significant in designing spin-based quantum computers[34].Moreover,studying the effect of a phase shift on amount transferable two-spin entanglement in a spin chain [35],it was shown that maximum attainable entanglement en-hanced by DM interaction.Therefore would be interesting to consider most general XY Z Heisenberg models with DM interaction as quantum channel for quantum teleportation which requires to know de-pendence of pairwise entanglement on the number of qubits in the spin chain.These questions now are under investigation.AcknowledgmentsOne of the authors(Z.N.G.)would like to thank Dr.Koji Maruyama for his helpful remarks.This work was supported partially by Izmir Institute of Technology,Turkey.[1]E.Schr¨o dinger,Proc.Camb.Phil.Soc.31,555,(1935).[2]A.Einstein,B.Podolsky,and N.Rosen,Phys.Rev.47,777,(1935).[3]J.S.Bell,Physics1,195,(1964).[4]C.H.Bennet and D.P.DiVincenzo,Nature,404,247,(2000).[5]S.-B.Zheng,G.-C.Guo,Phys.Rev.Lett.,85,(2000).[6]A.Imamoglu,D.D.Awschalom,G.Burkhard,D.P.Di-Vincenzo,D.Loss,M,Sherwin,and A.Small,Phys.Rev.Lett.,83,20,(1999).[7]G.,Benenti,G.,Casati,and G.,Strini,Principles ofQuantum Computation and Information Volume I,World Scientific,(2004).[8]V.G.Baryakhtar,P.E.Wigen,and N.A.Lesnik(Eds.),Frontiers in Magnetism of Reduced Dimension Systems, Kluwer Academic Press,(1998).[9]M.C.,Arnesen,S.Bose and V.,Vedral,Phys.Rew.Lett.,87,(2001).[10]E.H.Lieb,D.C.Mattis,Mathematical Physics in OneDimension:Exactly Solubable Models of Interacting Par-ticles,Academic Press,(1966).[11]R.J.Baxter,Exactly Solved Models in Statistical Me-chanics,Academic Press,(1982).[12]T.Osborne and N.Linden,Phys.Rev.A,052315,(2004).[13]M.A.Nielsen,Ph.D.Thesis,University of Mexico,e-print quant-ph/0011036,(1998).[14]I.Dzialoshinski,J.Phys.Chem.Solids4,241,(1958).[15]T.Moriya,Phys.Rev.Lett.4,228,(1960).[16]W.K.,Wooters,Phys.Rev.Lett.,78,(1997).[17]W.K.,Wooters,Phys.Rev.Lett.,80,(1998).[18]X.Wang,Phys.Rev.A,66,(2002).[19]D.Gunlycke,V.M.Kendon,and V.Vedral,Phys.Rev.A64,0432302,(2001).[20]A.F.Terzis,E.Paspalakis,Phys.Lett.A,333,(2004).[21]A.M.Childs,D.W.Leung,F.Verstraete,and G.Vidal,Quantum put.,3,97,(2003).[22]X.Xi,W.Chen,S.Hao,and R.Yue,Phys.Lett.A,300,567,(2002).[23]X.Xi and W.M.Liu,arXiv:quant-ph/0609087v1,(2006).[24]X.Wang,Phys.Rev.A,64,(2001).[25]G.L.Kamta and A.F.Starace,Phys.Rev.Lett.,88,(2002).[26]S.D.Hamieh and M.I.Katsnelson,Phys.Rev.A,72,032316,(2005).[27]Y.Sun,Y.Chen,and H.Chen,Phys.Rev.A,68,(2003).[28]X.Wang,Phys.Lett.A,281,101,(2001).[29]Xi,X.Q.,Hao,S.R.,Chen,W.X.and Yue,R.H.,Chin.Phys.Lett.,19,8,(2002).[30]G-F.Zhang,arXiv:quant-ph/0703019v1,(2007).[31]G.Rigolin,arXiv:quant-ph/0311185v2,(2004).[32]L.Zhou,H.S.Song,Y.Q.Guo,and C.Li,Phys.Rev.A,68,024301,(2003).[33]Z.He,Z.Xiong and Y.Zhang,Phys.Rev.A,354,79,(2006).[34]K.V.Kavokin,Phys.Rev.B,64,075305,(2001).[35]K.Maruyama,T.Iitaka,and F.Nori,Phys.Rev.A,75,012325,(2007).。
Correcting Quantum Errors In Higher Spin Systems

H. F. Chau∗
Department of Physics, University of Hong Kong, Pokfulam Road, Hong Kong (February 9, 2008) I consider the theory of quantum error correcting code (QECC) where each quantum particle has more than two possible eigenstates. In this higher spin system, I report an explicit QECC that is ⊗(N −1) ⊗ SN . This QECC, which generalizes Shor’s simple majority related to the symmetry group Z2 vote code, is able to correct errors arising from exactly one quantum particle. I also provide a simple encoding algorithm. PACS numbers: 03.65.Bz, 02.20.Df, 89.70.+c, 89.80.+h
spin-1/2 particle (A) is used as a messenger. It shuttles around other spin-1/2 particles (B) and interacts with them from time to time. Although decoherence between particles (B) may be neglected, decoherence between (A) and (B) can be serious (compare with a similar “gearbox quantum computer” proposal by DiVincenzo [14]). Therefore, it is natural to construct QECC which corrects this kind of “internal” decoherence error between different quantum registers. This can be achieved by constructing QECC that may correct errors involving multiple spins (see, for example, Refs. [5,6,8,10]). Alternatively, we may map this problem to that of correcting single quantum error in a system with higher spin. Suppose the messenger (A) has to interact with a specific spin-1/2 register (C) in (B). We may regard the combination of (A) and (C) as a single quantum particle with spin 3/2. If we encode this spin-3/2 state by an QECC and correct the quantum error immediately after the interaction process, decoherence between (A), (C) and the environment can be greatly suppressed. The advantage of this method is, in general, fewer quantum registers are required. The reason is simple: resources are concentrated on correcting errors in (A) and (C), while extra resources are needed for a general multiple quantum error correcting code in order to take care of the less frequent decoherence error within (B). Another reason to consider QECC for higher spin system is that quantum registers used may consist of more than two possible states. For example, the two bit quantum logic gate experimentally studied by Monroe et al. uses extra states for preparation and measurement [15]. Error correction may be required to prevent the quantum register from going to the unwanted states during the computation. In this paper, I consider QECC for particles with spin higher than 1/2. I study a special kind of QECC that is ⊗(N −1) related to the symmetry group Z2 ⊗ SN where N is the number of states of each spin. An explicit example of an QECC which is able to correct one quantum register∗
化学高中单词中英对照

化学高中单词中英比较foundation chemistry基础化学acid酸apparatus 仪器,装置aqueous solution 水溶液arrangement of electrons 电子摆列assumption 假设atom 原子(化学变化中的最小粒子)atomic mass 原子量atomic number 原子序数atomic radius 原子半径atomic structure 原子构造be composed of 由构成bombardment 撞击boundary 界线cathode rays 阴极射线cathode-ray oscilloscope阴极电子示波器ceramic 陶器制品charge-clouds 电子云charge-to-mass ratio(e/m) 质荷比(质谱剖析时样质量量的丈量以质量与其离子电荷之比表示)chemical behaviour 化学行为chemical property化学性质(物质在化学变化中表现出来的性质)clockwise顺时针方向的compound化合物(由不一样元素构成的纯净物)configuration构型copper铜correspond to相似corrosive腐化d-block elementsd 区元素deflect使倾向,使转向derive from源于deuterium氘diffuse mixture扩散混淆物distance effect 距离效应distil 蒸馏distinguish 差别distribution 分布 doubly charged(2+) ion 正二价离子dye染料effect of electric currentin solutions 电流在溶液里的影响 electrical charge 电荷 electrical field 电场electrically neutral atom 电中性原子electricity 电 electrolysis 电解electron 电子(负电荷粒子,电量等于×10 -10 绝对静电单位)electron shielding 电子障蔽element元素(拥有同样核电荷数即荷内质子数的一类原子的总称)emission spectrum发射光谱(依据发射光源和激发能量方式所产生的特点电磁波谱)energy level能态,能级(稳态能量,有同样主量数的电子壳层)fertiliser 肥料first ionisation energy 一级电离能fluorescent screen 荧光屏fuel 燃料fundamental substance 基础物质fuzzy 模糊的galaxy 星系,银河 gas 气体gaseous state气态gravity 重力GroupⅠ第一族Heisenberg ’s uncertainty principle 海森堡测禁止原理hydrofluoric acid 氢氟酸identical 同一的,相等的 in terms of 依据,在方面innermost 最内的,最深的interaction互相作用internal structure内部构造interpret解说investigate研究 , 检查Orbital轨道ionisation energy 电离能(从原子或分子中移走一个电子至araffin wax 白腊无量远地方需的能量,以电子伏特eV 表示)particle 微粒,粒子ionise 电离Pauli exclusion principle 保里不相容原理(每个原子轨道isotope 同位素(原子里拥有同样的质子数和不一样的中子数的至多只好容纳两个电子;并且,这两个电子自旋方向一定相反)同一元素的原子互称同位素)Periodic Table 周期表. Thomson’s e/m experiment Latin physical property 物理性质(物质不需要发生化学变化就表汤姆森质何比实验拉lepton 轻粒子 liquid 现出来的性质,如颜色、状态、气味、熔沸点、密度等)丁液体magnet 磁铁 magnetic field Maltese plastics 塑料plum-pudding 李子布丁磁场Cross marble positive charge 正电荷(带有质子的物质,用丝绸摩擦玻璃马耳他十字大理石mass number matter metal 棒,在棒上会产生正电荷)质量数物质foil meteorite microbe positive electrode (anode) 阳极金箔陨星微生物,model-building positively charged particle (ion) 离子细菌模型建筑molepotential difference 电位prediction 摩尔(表示一个系统的物质的量的单位,该系统中所包含预知principal quantum的基本单元数与12g 碳 12即 12C的原子数量相等 , 每摩尔物质含有number 主量子数(标示轨道电子的波函数,包含轨道角动量和阿佛加德罗常数个微粒)molecule自旋量子数,电子的能级和距原子核的均匀距离主要取决于主量分子(保持物质的化学性质的最小粒子)narrow beam子数)狭小的光芒negative electrode ( cathode )阴极probe 探测,研究negligibleproton 质子能够忽视的neutronquantum ( pl. quanta )量子(一个电子转移到原子的下一层中子nitrate轨道时发出的有限辐射能单位)quantum mechanics量子力学硝酸盐noble gasQuantum Theory 量子理论罕有气体normal pressuresquark 夸克(构成基本粒子的更小的粒子)常压radioactive source 放射源nuclear charge (原子)核电荷 nuclear model for atoms 原子核模型 nuclear reaction 核反响 nucleus ()核repel 排挤repulsion 斥力respectively分别地rung梯级scattering effect散射作用Schrdinger equation薛定谔(颠簸)方程(一偏微分方程,描绘基本粒子颠簸性)scintillation火花shell电子壳层shielding effect障蔽效应simpler substance单质(指由同种元素构成的纯净物)solid固体sphere球spin自旋stable state稳态sub-atomic particle原子内的粒子subset子集,小集体successive ionisation energy逐级电离能symbol符号symmetry 对称the lowest-energyorbitals最低能量轨道transition elements过渡元素X-ray X射线α - particlesα 粒子,即alpha-particle(带有两个质子和中子的粒子,即氦原子核,对物质的穿透力较强,流速约为光速的1/10 )α- ray α射线β - rayβ 射线β- particlesβ 粒子γ-parti icles γ粒子γ -ray 射线acid酸organic chemistry有机化学inorganic chemistry无机化学derivative衍生物series系列hydrochloric acid盐酸sulphuric acid硫酸nitric acid硝酸fatty acid脂肪酸organic acid有机酸hydrosulphuric acid氢硫酸hydrogen sulfide氢化硫alkali碱, 强碱ammonia氨base碱hydrate水合物hydroxide氢氧化物 , 羟化物hydracid氢酸hydrocarbon碳氢化合物 , 羟anhydride酐alkaloid生物碱aldehyde醛oxide氧化物methane甲烷, 沼气butane丁烷salt盐potassium carbonate碳酸钾soda苏打sodium carbonate碳酸钠caustic potash苛性钾caustic soda苛性钠gel凝胶体analysis分解fractionation分馏endothermic reaction吸热反响exothermic reaction放热反响precipitation积淀to precipitate积淀Bunsen burner本生灯product反响产物flask烧瓶apparatus设施PH indicator PH值指示剂,氢离子(浓度的)负指数指示剂matrass卵形瓶litmus石蕊litmus paper石蕊试纸graduate, graduated flask量筒,量杯reagent试剂test tube试管burette滴定管retort曲颈甑still蒸馏釜cupel烤钵crucible pot, melting pot坩埚pipette吸液管filter滤管stirring rod搅拌棒to distil, to distill蒸馏distillation蒸馏to calcine煅烧to oxidize氧化alkalinization碱化to oxygenate, to oxidize脱氧,氧化to neutralize中和to hydrogenate氢化to hydrate水合,水化to dehydrate脱水fermentation发酵solution溶解combustion焚烧fusion, melting溶化fractionating tower分馏塔alkalinity碱性fractional distillation分馏isomerism, isomery同分异物现象distillation column分裂蒸馏塔hydrolysis水解polymerizing, polymerization聚合electrolysis电解reforming重整electrode电极purification净化anode阳极 , 正极hydrocarbon烃,碳氢化合物cathode阴极 , 负极crude oil, crude原油catalyst催化剂petrol汽油(美作:gasoline)catalysis催化作用LPG, liquefied petroleum gas液化石油气oxidization, oxidation氧化LNG, liquefied natural gas液化天然气reducer复原剂Vaseline凡士林dissolution分解paraffin白腊synthesis合成kerosene, karaffin oil煤油reversible可逆的gas oil柴油refining炼油lubricating oil润滑油refinery炼油厂asphalt沥青cracking裂化benzene苯separation分别fuel燃料natural gas天然filter滤管high-grade petrol, high-octane petrol高级汽油,高辛stirring rod搅拌棒烷值汽油element元素plastic塑料body物体chemical fiber化学纤维compound化合物synthetic rubber合成橡胶atom原子solvent溶剂gram atom克原子Bunsen burner本生灯atomic weight原子量product化学反响产物atomic number原子数flask烧瓶atomic mass原子质量apparatus设施molecule分子PH indicator PH值指示剂,氢离子(浓度的)负指数指示剂electrolyte电解质litmus石蕊ion离子litmus paper石蕊试纸anion阴离子graduate, graduated flask量筒,量杯cation阳离子reagent试剂electron电子test tube试管isotope同位素still蒸馏釜isomer同分异物现象crucible pot, melting pot坩埚polymer聚合物pipette吸液管symbol复合radical基structural formula分子式valence, valency价monovalent单价bivalent二价halogen成盐元素bond原子的聚合mixture混淆combination合成作用compound合成物alloy合金metal金属metalloid非金属Hydrogen(H)氢Iodine(I)碘Iron(Fe)铁Lead(Pb)铅Magnesium(Mg)镁v1.0可编写可改正ExercisesQuestions 1-3 refer to the following aqueous solutions.(A)M HCl(B)M NaCl(C)M HC2H3O2(D)MCH3OH(E)M KOH1.Is weakly acidic2.Has the highest pH3.Reacts with an equal volume of MBa(OH)2 to form a solution with pH = 7KEY:()()()4. If the molar mass of NH 3 is 17g/mol, what isthe density of this compound at STP(标准情况)A. L B.L C.L D.L E.Lv1.0可编写可改正。
TheKlein-Gordonequation:克莱因戈登方程

where the Lagrangian density satisfies the Euler-Lagrange equations of motions
(25)
such that the Euler-Lagrange equations of motion just give the Klein-Gordon equation (12) and its complex conjugate.
as the basic field equation of the scalar field.
The plane waves (10) are basic solutions and the field (9) is constructed by
a general superposition of the basic states.
Quantization
The challenge is to find operator solutions of the Klein-Gordon equation (12) which satisfy eq. (28). In analogy to the Lagrange density (24) , the hamiltonian is
Lecture 8
The Klein-Gordon equation
WS2010/11: ‚Introduction to Nuclear and Particle Physics‘
The bosons in field theory
Bosons with spin 0
scalar (or pseudo-scalar) meson fields
(23)
Singularity of the density of states in the two-dimensional Hubbard model from finite size

a r X i v :c o n d -m a t /9503139v 1 27 M a r 1995Singularity of the density of states in the two-dimensional Hubbard model from finitesize scaling of Yang-Lee zerosE.Abraham 1,I.M.Barbour 2,P.H.Cullen 1,E.G.Klepfish 3,E.R.Pike 3and Sarben Sarkar 31Department of Physics,Heriot-Watt University,Edinburgh EH144AS,UK 2Department of Physics,University of Glasgow,Glasgow G128QQ,UK 3Department of Physics,King’s College London,London WC2R 2LS,UK(February 6,2008)A finite size scaling is applied to the Yang-Lee zeros of the grand canonical partition function for the 2-D Hubbard model in the complex chemical potential plane.The logarithmic scaling of the imaginary part of the zeros with the system size indicates a singular dependence of the carrier density on the chemical potential.Our analysis points to a second-order phase transition with critical exponent 12±1transition controlled by the chemical potential.As in order-disorder transitions,one would expect a symmetry breaking signalled by an order parameter.In this model,the particle-hole symmetry is broken by introducing an “external field”which causes the particle density to be-come non-zero.Furthermore,the possibility of the free energy having a singularity at some finite value of the chemical potential is not excluded:in fact it can be a transition indicated by a divergence of the correlation length.A singularity of the free energy at finite “exter-nal field”was found in finite-temperature lattice QCD by using theYang-Leeanalysisforthechiral phase tran-sition [14].A possible scenario for such a transition at finite chemical potential,is one in which the particle den-sity consists of two components derived from the regular and singular parts of the free energy.Since we are dealing with a grand canonical ensemble,the particle number can be calculated for a given chem-ical potential as opposed to constraining the chemical potential by a fixed particle number.Hence the chem-ical potential can be thought of as an external field for exploring the behaviour of the free energy.From the mi-croscopic point of view,the critical values of the chemical potential are associated with singularities of the density of states.Transitions related to the singularity of the density of states are known as Lifshitz transitions [15].In metals these transitions only take place at zero tem-perature,while at finite temperatures the singularities are rounded.However,for a small ratio of temperature to the deviation from the critical values of the chemical potential,the singularity can be traced even at finite tem-perature.Lifshitz transitions may result from topological changes of the Fermi surface,and may occur inside the Brillouin zone as well as on its boundaries [16].In the case of strongly correlated electron systems the shape of the Fermi surface is indeed affected,which in turn may lead to an extension of the Lifshitz-type singularities into the finite-temperature regime.In relating the macroscopic quantity of the carrier den-sity to the density of quasiparticle states,we assumed the validity of a single particle excitation picture.Whether strong correlations completely distort this description is beyond the scope of the current study.However,the iden-tification of the criticality using the Yang-Lee analysis,remains valid even if collective excitations prevail.The paper is organised as follows.In Section 2we out-line the essentials of the computational technique used to simulate the grand canonical partition function and present its expansion as a polynomial in the fugacity vari-able.In Section 3we present the Yang-Lee zeros of the partition function calculated on 62–102lattices and high-light their qualitative differences from the 42lattice.In Section 4we analyse the finite size scaling of the Yang-Lee zeros and compare it to the real-space renormaliza-tion group prediction for a second-order phase transition.Finally,in Section 5we present a summary of our resultsand an outlook for future work.II.SIMULATION ALGORITHM AND FUGACITY EXPANSION OF THE GRAND CANONICALPARTITION FUNCTIONThe model we are studying in this work is a two-dimensional single-band Hubbard HamiltonianˆH=−t <i,j>,σc †i,σc j,σ+U i n i +−12 −µi(n i ++n i −)(1)where the i,j denote the nearest neighbour spatial lat-tice sites,σis the spin degree of freedom and n iσis theelectron number operator c †iσc iσ.The constants t and U correspond to the hopping parameter and the on-site Coulomb repulsion respectively.The chemical potential µis introduced such that µ=0corresponds to half-filling,i.e.the actual chemical potential is shifted from µto µ−U412.(5)This transformation enables one to integrate out the fermionic degrees of freedom and the resulting partition function is written as an ensemble average of a product of two determinantsZ ={s i,l =±1}˜z = {s i,l =±1}det(M +)det(M −)(6)such thatM ±=I +P ± =I +n τ l =1B ±l(7)where the matrices B ±l are defined asB ±l =e −(±dtV )e −dtK e dtµ(8)with V ij =δij s i,l and K ij =1if i,j are nearestneigh-boursand Kij=0otherwise.The matrices in (7)and (8)are of size (n x n y )×(n x n y ),corresponding to the spatial size of the lattice.The expectation value of a physical observable at chemical potential µ,<O >µ,is given by<O >µ=O ˜z (µ){s i,l =±1}˜z (µ,{s i,l })(9)where the sum over the configurations of Ising fields isdenoted by an integral.Since ˜z (µ)is not positive definite for Re(µ)=0we weight the ensemble of configurations by the absolute value of ˜z (µ)at some µ=µ0.Thus<O >µ= O ˜z (µ)˜z (µ)|˜z (µ0)|µ0|˜z (µ0)|µ0(10)The partition function Z (µ)is given byZ (µ)∝˜z (µ)N c˜z (µ0)|˜z (µ0)|×e µβ+e −µβ−e µ0β−e −µ0βn (16)When the average sign is near unity,it is safe to as-sume that the lattice configurations reflect accurately thequantum degrees of freedom.Following Blankenbecler et al.[1]the diagonal matrix elements of the equal-time Green’s operator G ±=(I +P ±)−1accurately describe the fermion density on a given configuration.In this regime the adiabatic approximation,which is the basis of the finite-temperature algorithm,is valid.The situa-tion differs strongly when the average sign becomes small.We are in this case sampling positive and negative ˜z (µ0)configurations with almost equal probability since the ac-ceptance criterion depends only on the absolute value of ˜z (µ0).In the simulations of the HSfields the situation is dif-ferent from the case of fermions interacting with dynam-ical bosonfields presented in Ref.[1].The auxilary HS fields do not have a kinetic energy term in the bosonic action which would suppress their rapidfluctuations and hence recover the adiabaticity.From the previous sim-ulations on a42lattice[3]we know that avoiding the sign problem,by updating at half-filling,results in high uncontrolledfluctuations of the expansion coefficients for the statistical weight,thus severely limiting the range of validity of the expansion.It is therefore important to obtain the partition function for the widest range ofµ0 and observe the persistence of the hierarchy of the ex-pansion coefficients of Z.An error analysis is required to establish the Gaussian distribution of the simulated observables.We present in the following section results of the bootstrap analysis[17]performed on our data for several values ofµ0.III.TEMPERATURE AND LATTICE-SIZEDEPENDENCE OF THE YANG-LEE ZEROS The simulations were performed in the intermediate on-site repulsion regime U=4t forβ=5,6,7.5on lat-tices42,62,82and forβ=5,6on a102lattice.The ex-pansion coefficients given by eqn.(14)are obtained with relatively small errors and exhibit clear Gaussian distri-bution over the ensemble.This behaviour was recorded for a wide range ofµ0which makes our simulations reli-able in spite of the sign problem.In Fig.1(a-c)we present typical distributions of thefirst coefficients correspond-ing to n=1−7in eqn.(14)(normalized with respect to the zeroth power coefficient)forβ=5−7.5for differ-entµ0.The coefficients are obtained using the bootstrap method on over10000configurations forβ=5increasing to over30000forβ=7.5.In spite of different values of the average sign in these simulations,the coefficients of the expansion(16)indicate good correspondence between coefficients obtained with different values of the update chemical potentialµ0:the normalized coefficients taken from differentµ0values and equal power of the expansion variable correspond within the statistical error estimated using the bootstrap analysis.(To compare these coeffi-cients we had to shift the expansion by2coshµ0β.)We also performed a bootstrap analysis of the zeros in theµplane which shows clear Gaussian distribution of their real and imaginary parts(see Fig.2).In addition, we observe overlapping results(i.e.same zeros)obtained with different values ofµ0.The distribution of Yang-Lee zeros in the complexµ-plane is presented in Fig.3(a-c)for the zeros nearest to the real axis.We observe a gradual decrease of the imaginary part as the lattice size increases.The quantitative analysis of this behaviour is discussed in the next section.The critical domain can be identified by the behaviour of the density of Yang-Lee zeros’in the positive half-plane of the fugacity.We expect tofind that this density is tem-perature and volume dependent as the system approaches the phase transition.If the temperature is much higher than the critical temperature,the zeros stay far from the positive real axis as it happens in the high-temperature limit of the one-dimensional Ising model(T c=0)in which,forβ=0,the points of singularity of the free energy lie at fugacity value−1.As the temperature de-creases we expect the zeros to migrate to the positive half-plane with their density,in this region,increasing with the system’s volume.Figures4(a-c)show the number N(θ)of zeros in the sector(0,θ)as a function of the angleθ.The zeros shown in thesefigures are those presented in Fig.3(a-c)in the chemical potential plane with other zeros lying further from the positive real half-axis added in.We included only the zeros having absolute value less than one which we are able to do because if y i is a zero in the fugacity plane,so is1/y i.The errors are shown where they were estimated using the bootstrap analysis(see Fig.2).Forβ=5,even for the largest simulated lattice102, all the zeros are in the negative half-plane.We notice a gradual movement of the pattern of the zeros towards the smallerθvalues with an increasing density of the zeros nearθ=πIV.FINITE SIZE SCALING AND THESINGULARITY OF THE DENSITY OF STATESAs a starting point for thefinite size analysis of theYang-Lee singularities we recall the scaling hypothesis forthe partition function singularities in the critical domain[11].Following this hypothesis,for a change of scale ofthe linear dimension LLL→−1),˜µ=(1−µT cδ(23)Following the real-space renormalization group treatmentof Ref.[11]and assuming that the change of scaleλisa continuous parameter,the exponentαθis related tothe critical exponentνof the correlation length asαθ=1ξ(θλ)=ξ(θ)αθwe obtain ξ∼|θ|−1|θ|ναµ)(26)where θλhas been scaled to ±1and ˜µλexpressed in terms of ˜µand θ.Differentiating this equation with respect to ˜µyields:<n >sing =(−θ)ν(d −αµ)∂F sing (X,Y )ν(d −αµ)singinto the ar-gument Y =˜µαµ(28)which defines the critical exponent 1αµin terms of the scaling exponent αµof the Yang-Lee zeros.Fig.5presents the scaling of the imaginary part of the µzeros for different values of the temperature.The linear regression slope of the logarithm of the imaginary part of the zeros plotted against the logarithm of the inverse lin-ear dimension of the simulation volume,increases when the temperature decreases from β=5to β=6.The re-sults of β=7.5correspond to αµ=1.3within the errors of the zeros as the simulation volume increases from 62to 82.As it is seen from Fig.3,we can trace zeros with similar real part (Re (µ1)≈0.7which is also consistentwith the critical value of the chemical potential given in Ref.[22])as the lattice size increases,which allows us to examine only the scaling of the imaginary part.Table 1presents the values of αµand 1αµδ0.5±0.0560.5±0.21.3±0.3∂µ,as a function ofthe chemical potential on an 82lattice.The location of the peaks of the susceptibility,rounded by the finite size effects,is in good agreement with the distribution of the real part of the Yang-Lee zeros in the complex µ-plane (see Fig.3)which is particularly evident in the β=7.5simulations (Fig.4(c)).The contribution of each zero to the susceptibility can be singled out by expressing the free energy as:F =2n x n yi =1(y −y i )(29)where y is the fugacity variable and y i is the correspond-ing zero of the partition function.The dotted lines on these plots correspond to the contribution of the nearby zeros while the full polynomial contribution is given by the solid lines.We see that the developing singularities are indeed governed by the zeros closest to the real axis.The sharpening of the singularity as the temperature de-creases is also in accordance with the dependence of the distribution of the zeros on the temperature.The singularities of the free energy and its derivative with respect to the chemical potential,can be related to the quasiparticle density of states.To do this we assume that single particle excitations accurately represent the spectrum of the system.The relationship between the average particle density and the density of states ρ(ω)is given by<n >=∞dω1dµ=ρsing (µ)∝1δ−1(32)and hence the rate of divergence of the density of states.As in the case of Lifshitz transitions the singularity of the particle number is rounded at finite temperature.However,for sufficiently low temperatures,the singular-ity of the density of states remains manifest in the free energy,the average particle density,and particle suscep-tibility [15].The regular part of the density of states does not contribute to the criticality,so we can concentrate on the singular part only.Consider a behaviour of the typedensity of states diverging as the−1ρsing(ω)∝(ω−µc)1δ.(33)with the valueδfor the particle number governed by thedivergence of the density of states(at low temperatures)in spite of thefinite-temperature rounding of the singu-larity itself.This rounding of the singularity is indeedreflected in the difference between the values ofαµatβ=5andβ=6.V.DISCUSSION AND OUTLOOKWe note that in ourfinite size scaling analysis we donot include logarithmic corrections.In particular,thesecorrections may prove significant when taking into ac-count the fact that we are dealing with a two-dimensionalsystem in which the pattern of the phase transition islikely to be of Kosterlitz-Thouless type[23].The loga-rithmic corrections to the scaling laws have been provenessential in a recent work of Kenna and Irving[24].In-clusion of these corrections would allow us to obtain thecritical exponents with higher accuracy.However,suchanalysis would require simulations on even larger lattices.The linearfits for the logarithmic scaling and the criti-cal exponents obtained,are to be viewed as approximatevalues reflecting the general behaviour of the Yang-Leezeros as the temperature and lattice size are varied.Al-though the bootstrap analysis provided us with accurateestimates of the statistical error on the values of the ex-pansion coefficients and the Yang-Lee zeros,the smallnumber of zeros obtained with sufficient accuracy doesnot allow us to claim higher precision for the critical ex-ponents on the basis of more elaboratefittings of the scal-ing behaviour.Thefinite-size effects may still be signifi-cant,especially as the simulation temperature decreases,thus affecting the scaling of the Yang-Lee zeros with thesystem rger lattice simulations will therefore berequired for an accurate evaluation of the critical expo-nent for the particle density and the density of states.Nevertheless,the onset of a singularity atfinite temper-ature,and its persistence as the lattice size increases,areevident.The estimate of the critical exponent for the diver-gence rate of the density of states of the quasiparticleexcitation spectrum is particularly relevant to the highT c superconductivity scenario based on the van Hove sin-gularities[25],[26],[27].It is emphasized in Ref.[25]thatthe logarithmic singularity of a two-dimensional electrongas can,due to electronic correlations,turn into a power-law divergence resulting in an extended saddle point atthe lattice momenta(π,0)and(0,π).In the case of the14.I.M.Barbour,A.J.Bell and E.G.Klepfish,Nucl.Phys.B389,285(1993).15.I.M.Lifshitz,JETP38,1569(1960).16.A.A.Abrikosov,Fundamentals of the Theory ofMetals North-Holland(1988).17.P.Hall,The Bootstrap and Edgeworth expansion,Springer(1992).18.S.R.White et al.,Phys.Rev.B40,506(1989).19.J.E.Hirsch,Phys.Rev.B28,4059(1983).20.M.Suzuki,Prog.Theor.Phys.56,1454(1976).21.A.Moreo, D.Scalapino and E.Dagotto,Phys.Rev.B43,11442(1991).22.N.Furukawa and M.Imada,J.Phys.Soc.Japan61,3331(1992).23.J.Kosterlitz and D.Thouless,J.Phys.C6,1181(1973);J.Kosterlitz,J.Phys.C7,1046(1974).24.R.Kenna and A.C.Irving,unpublished.25.K.Gofron et al.,Phys.Rev.Lett.73,3302(1994).26.D.M.Newns,P.C.Pattnaik and C.C.Tsuei,Phys.Rev.B43,3075(1991);D.M.Newns et al.,Phys.Rev.Lett.24,1264(1992);D.M.Newns et al.,Phys.Rev.Lett.73,1264(1994).27.E.Dagotto,A.Nazarenko and A.Moreo,Phys.Rev.Lett.74,310(1995).28.A.A.Abrikosov,J.C.Campuzano and K.Gofron,Physica(Amsterdam)214C,73(1993).29.D.S.Dessau et al.,Phys.Rev.Lett.71,2781(1993);D.M.King et al.,Phys.Rev.Lett.73,3298(1994);P.Aebi et al.,Phys.Rev.Lett.72,2757(1994).30.E.Dagotto, A.Nazarenko and M.Boninsegni,Phys.Rev.Lett.73,728(1994).31.N.Bulut,D.J.Scalapino and S.R.White,Phys.Rev.Lett.73,748(1994).32.S.R.White,Phys.Rev.B44,4670(1991);M.Veki´c and S.R.White,Phys.Rev.B47,1160 (1993).33.C.E.Creffield,E.G.Klepfish,E.R.Pike and SarbenSarkar,unpublished.Figure CaptionsFigure1Bootstrap distribution of normalized coefficients for ex-pansion(14)at different update chemical potentialµ0for an82lattice.The corresponding power of expansion is indicated in the topfigure.(a)β=5,(b)β=6,(c)β=7.5.Figure2Bootstrap distributions for the Yang-Lee zeros in the complexµplane closest to the real axis.(a)102lat-tice atβ=5,(b)102lattice atβ=6,(c)82lattice at β=7.5.Figure3Yang-Lee zeros in the complexµplane closest to the real axis.(a)β=5,(b)β=6,(c)β=7.5.The correspond-ing lattice size is shown in the top right-hand corner. Figure4Angular distribution of the Yang-Lee zeros in the com-plex fugacity plane Error bars are drawn where esti-mated.(a)β=5,(b)β=6,(c)β=7.5.Figure5Scaling of the imaginary part ofµ1(Re(µ1)≈=0.7)as a function of lattice size.αm u indicates the thefit of the logarithmic scaling.Figure6Electronic susceptibility as a function of chemical poten-tial for an82lattice.The solid line represents the con-tribution of all the2n x n y zeros and the dotted line the contribution of the six zeros nearest to the real-µaxis.(a)β=5,(b)β=6,(c)β=7.5.。
四面体晶格中的多组份纠缠
3
written as Cn = max{0, λ0 −
−1 where {λj }2 j =0 is the spectrum of the operator
n
2n − 1
λj } √
j =1
(4)
ρU ρU −1 in decreasing order.
Multipartite Entanglement of a Tetrahedron Lattice
Rong Zhang and Shiqun Zhu* and Xiang Hao China Center of Advanced Science and Technology (World Laboratory), P. O. Box 8730, Beijing 100080, People’s Republic of China and School of Physical Science and Technology, Suzhou University, Suzhou, Jiangsu 215006, People’s Republic of China**
2
Evaluation of Entanglement
system. For the cases of enIt is necessary to quantify the entanglement in spin- 1 2 systems, the concurrence can be used tanglement between any two qubits in spin- 1 2 to evaluate the entanglement of the system [3]. For many qubits in spin- 1 systems, 2 the multipartite entanglement of more than two qubits can also be calculated through n-concurrence [16, 25-30].
Two-field Models of Dark Energy with Equation of State Across -1
Scattering and Inverse Scattering on ACH Manifolds
dt2 + h(t) t2 ∞ ¯ The function ρ := ψ∗ t is where h(t), t ∈ [0, ǫ) is a C 1-parameter family of C ∞ metrics on ∂ X. ¯ ¯ ¯ Note that a boundary defining function in X near ∂ X, which can be extended smoothly to X. n the boundary represents the geometric infinity of X , as does the sphere S for the hyperbolic space Hn+1 the Laplacian of (X, g ) was studied in [27]; it consists a finite pure point spectrum σpp (∆), which is the set of L2 (X ) eigenvalues, and an absolutely continuous spectrum σac (∆) satisfying The resolvent σac (∆) = n2 /4, ∞ and σpp (∆) ⊂ 0, n2 /4 .
R(λ) = (∆g − λ(n − λ))−1 ,
2000 Mathematics Subject Classification. Primary 58J50, Secondary 35P25. Key words and phrases. scattering, pseudoconvex domains, asymptotically complex hyperbolic manifolds. The first author was partially supported by French ANR grants no. [JC05-52556] and [JC05-46063], and an Australian National University postdoctoral fellowship. Both authors were supported in part by the National Science Foundation Grant DMS 0500788.
Can Short-Range Interactions Mediate a Bose Metal Phase in 2D
a r X i v :c o n d -m a t /0109269v 1 14 S e p 2001Can Short-Range Interactions Mediate a Bose Metal Phase in 2D?Philip Phillips 1and Denis Dalidovich 21Loomis Laboratory of PhysicsUniversity of Illinois at Urbana-Champaign 1100W.Green St.,Urbana,IL,61801-30802National High Magnetic Field LaboratoryFlorida State University,Talahasse,Florida,31301We show here based on a 1-loop scaling analysis that short-range interactions are strongly irrelevant perturbations near the insulator-superconductor (IST)quantum critical point.The lack of any proof that short-range interactions mediate physics which is present only in strong coupling leads us to conclude that short-range interactions are strictly irrelevant near the IST quantum critical point.Hence,we argue that no new physics,such as the formation of a uniform Bose metal phase can arise from an interplay between on-site and nearest-neighbour interactions.The standard model used to study [1–13]the insulator-superconductor transition in thin films is the commensu-rate Bose-Hubbard model or equivalently the charging model for an array of Josephson junctions.The Hamil-tonian for this modelˆH=12dτk˙φ(k )˙φ(−k)no restriction on the range of V ij.To simplify this action, wefirst decouple the charging term by introducing[4]an auxilliary real gaugefield,A0(k),through the identity exp −1V(k)˙φ(−k) = D A0exp −1e−2V(k)−1−12 d d xdτ |(∂τ−ieA0)ψ|2+|∇ψ|2+r|ψ|2+u 2 k,ωA0(k,ω)A0(−k,−ω)2 k,ωkσA0(k,ω)A0(−k,−ω),(7) which is the Fisher and Grinstein[4]result.What about short-range interactions?We simplify to the case considered by Das and Doniach[21]and truncate V(k)at the nearest-neighbour level:V(k)=V0+2V1(cos k x+cos k y).(8) It is crucial in our derivation that V0=0.As has been considered previously,when V0=0but V1=0,the na-ture of the T=0transition changes fundamentally when compared with the V0=0case.In the former case,that is,V0=0but V1=0,the T=0transition is of the Berezinskii-Kosterlitz-Thouless kind[23].In the long wavelength limit,V(k)=V0+2V1−V1k2,which is con-venient to write in the form,e2−V1k2where we have fixed the free parameter,e2=V0+2V1.Consequently, the pure gauge part of the action simplifies toS1=−e2k2.(9) Uponrescaling the gaugefield,A0(k,ω)→i e2A0(k,ω),we arrive at the working form for the action,S=12|ψ|4 +1k2A0(k,ω)(10)where the constant g= V1. Clearly,when V1=0,g=0and the rescaledfields, A0(k,ω),vanish leading to the standard on-site charging model.Hence,the relevance of short range interactions can be deduced entirely from the scaling properties of the coupling constant g.Performing the standard tree-level rescaling with the rescaling parameter b>1,wefind that the momentum and frequency scale as q′=qb andω′=ωb z,with z the dynamical exponent.At the tree level,z=1and the anomalous dimension exponent vanishes,η=0.Hence, theψand A0fields scale asA0=bµA′0,µ=d+z−22.(11) Combining these scaling relations with the rescaling of the momentum and the frequency arising from the inte-grations in the action,we arrive at our key resultg′=gbµ+λWe evaluate these diagrams using the standard frequency-momentum shell RG approach in which we in-tegrate out thefields A0(ω,k)andψ(ω,k)for momenta and frequencies satisfying the constraintΛb <k<Λwith the upper momentum and frequencycutoffsΛω=Λk=Λ=1.Setting b=eℓ,we obtain dgℓ2 gℓ−2Aℓgℓuℓ−Bℓg3ℓ(13) as the differential form for the scaling equation for g.The coefficients,Aℓand Bℓare given byAℓ=2K d(q2+1+rℓ)2 + 10dω(2π)d+1 10dqq d+11+2q2+2rℓ(1+ω2+rℓ)2 ,(15) where K d is the area of a d-dimensional unit sphere. These coefficients are positive and depend on the scal-ing lengthℓthrough the parameter rℓ.Hence,fromthestructureofthescaling equation,for gℓ,Eq.(13),wefindthat the g=0fixed point is stable through one-loop or-der.That is,there is no signature in weak coupling thatfinite g can drive a new critical point.This conclusionis consistent with the standard view that as long as thebroken symmetry state is rotationally and translation-ally invariant,the critical point is of the Wilson-Fishertype where it is well known that short-range interactionscannot lead to a new critical point.Because g∝√[1]S.Doniach,Phys.Rev.B24,5063,(1981).[2]M.P.A.Fisher,Phys.Rev.B36,1917(1987);[3]X.G.Wen and A.Zee,Int.J.Mod.Phys.B4,437(1990).[4]M.P.A.Fisher and G.Grinstein,Phys.Rev.Lett.60,208,(1988).[5]W.Zwerger,J.Low Temp.Phys.72,291(1988);ibid,Physica B152,236(1988).[6]S.Chakravarty,S.Kivelson,G.T.Zimanyi,and B.I.Halperin,Phys.Rev.B37,3283(1988).[7]A.Kampf and G.Sch¨o n,Phys.Rev.B36,3651(1987).[8]V.Ambegoakar,U.Eckern,and G.Sch¨o n,Phys.Rev.Lett.48,1745(1982).[9]K.Wagenblast,A.van Otterlo,G.Sch¨o n,and G.Zi-manyi,Phys.Rev.Lett.79,2730(1997).[10]A.van Otterlo,K.-H Wagenblast,R.Fazio,and G.Sch¨o n,Phys.Rev.B48,3316(1993).[11]M.C.Cha,M.P.A.Fisher,S.M.Girvin,M.Wallin,and A.P.Young,Phys.Rev.B44,6883(1991).[12]E.Frey and L.Balents,Phys.Rev.B55,1050(1997).[13]F.Hebert,G.G.Batrouni,R.T.Scalettar,G.Schmid,M.Troyer,and A.Dorneich,cond-mat/0105450.[14]N.Mason and A.Kapitulnik,Phys.Rev.Lett.82,5341(1999);ibid,cond-mat/0006138.[15]D.Ephron, A.Yazdani, A.Kapitulnik,and M.R.Beasley,Phys.Rev.Lett.76,1529(1996).[16]H.M.Jaeger,D.B.Haviland,B.G.Orr,and A.M.Goldman,Phys.Rev.B40,182(1989).[17]H.S.J.van der Zant,et.al.Phys.Rev.B54,10081,(1996).[18]D.Dalidovich and P.Phillips,Phys.Rev.B64,52507-1(2001).[19]E.Shimshoni,A.Auerbach,and A.Kapitulnik,Phys.Rev.Lett.80,3352(1998).[20]A.Kapitulnik,N.Mason,S. A.Kivelson,and S.Chakravarty,cond-mat/0009201.[21]D.Das and S.Doniach,Phys.Rev.B601261(1999).[22]See Eq.4.11in J.Cardy,Scaling and Renormalization inStatistical Physics,(Cambridge University Press,Cam-bridge,1996)p.71.[23]R.Fazio and G.Sch¨o n,Phys.Rev.43,5307(1991).[24]Jinwu Ye,Phys.Rev.B58,9450(1998).3。
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Physics Department, University of Wuppertal, D-42097 Wuppertal, Germany February 1, 2008
Dedicated to J. Zittartz on the occasion of his 60th birthday. Abstract. We investigate the scaling properties of the excitation energies and transition amplitudes of the one-dimensional spin- 1 2 antiferromagnetic Heisenberg model exposed to an external perturbation. Two types of perturbations are discussed in detail: a staggered field and a dimerized field. PACS. 75.10 -b General theory and models of magnetic ordering
N
(1.5)
(1.2)
S3 (q ) ≡
eilq Sl3 ,
l=1
(1.3)
for the operator S3 (π ) in the one-dimensional antiferromagnetic Heisenberg model in a staggered field of strength h. In section 2 we derive a system of differential equations, which describes the evolution in h for ωmn and Tmn . Section 3 is devoted to a finite-size scaling analysis of the ground state excitations ωm0 and Tm0 in the combined limit h → 0 and N → ∞. It is shown in section 4, that the critical exponents σ and ǫ in the scaling ansatz and the scaling variable as well can be computed by means of the evolution equations. For small values of the scaling variable the scaling function is also determined. In section 5 we analyse in the same way the dimer operator.
m =n
The transition matrix elements Tm0 (N, 0), m = 1, 3, 5, . . . from the ground state |Ψ0 (0) to the excited states |Ψm (0) appear in the definition of the dynamic structure factor S (N, ω, p = π, h = 0) = 1 δ [ω − ωm0 (N, 0)]|Tm0 (N, 0)|2 , N m
1 Introduction
coupled spin chains. Treating the interchain coupling in the mean field approach, reduces the system to a oneThe one-dimensional spin- 1 antiferromagnetic Heisenberg dimensional Heisenberg model in a staggered field [10]. 2 model with nearest neighbour couplings and periodic boundIt is the purpose of this paper to study excitation enary conditions (SN +1 = S1 ): ergies
N
H≡2
l=1
Sl · Sl+1
(1.1)
ωmn (N, h) ≡ Em (N, h) − En (N, h), and transition amplitudes Tmn (N, h) ≡ Ψm (h)|S3 (π )|Ψn (h) ,
(1.4)
has been studied intensively with analytic and numerical methods. Eigenvalues as well as transition matrix elements for the spin operator have been calculated with the Bethe ansatz and quantum group symmetries [1]. These calculations allow to exploit part of the dynamical properties of the model, the two-spinon contributions, at T = 0 [2]. The dynamics of the model in the presence of an external magnetic field, which is periodic in space H(h) ≡ H + hS3 (q ) with
(2.2) (2.3)
(2.11)
where we have used the definitions (1.4) and (1.5). The evolution is governed by the transitiБайду номын сангаасn matrix elements of the operator S3 (π ) [Eq. (1.3)]. The operator S3 (π ) is real hermitian and therefore the matrix (1.5) is symmetric Tmn = Tnm . Remarkably enough, there exists a closed system of differential equations, which describes the h-dependence of the energy eigenvalues En = En (N, h) and the transition matrix elements Tmn = Tmn (N, h): d En = −2 dh2 dTmn =− dh
N →∞
l= n
|Tln | , ωln
2
am0 . N
(2.13)
(2.4)
l=m,n
Tmn dωnm Tml Tln Tml Tln − + . ωlm ωln ωnm dh (2.5)
The Hamiltonian (1.2) behaves under translations T of one lattice spacing as: TH(h)T† = H(−h). Since T is unitary, the eigenvalues En (N, h) = En (N, −h) are symmetric, whereas the eigenstates |Ψ (h) , |Ψ (−h) = T|Ψ (h) , (2.8) are no longer momentum eigenstates, but linear combinations of two momentum eigenstates with momenta p = 0 and p = π , respectively. Of course, in the limit h → 0 translation invariance is recovered and p is again a good quantum number. We use the following notation for the energy eigenstates: T|Ψn (0) = ±|Ψn (0) , n = 0, 1, 2, . . . , (2.9) (2.7) (2.6)
has been studied so far mainly for p = 0 [3,4,5,6,7,8,9]. Since the total spin S3 (0) commutes with H, the eigenvectors of H(h) and H are the same, the eigenvalues change in a trivial manner. For this reason the magnetic properties of the model (1.1) in a constant field – as there are magnetization curves, susceptibilities, static and dynamic structure factors – were accessible by means of the Bethe ansatz as well. The case of a staggered field, i.e. Eq. (1.2) for p = π , in a one-dimensional Heisenberg model has attracted considerable interest as an effective model for