Absence of coexisting phase of quark-antiquark and diquark condensed phases in the extended

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《马斯克传》中逆向思维在文中的原话

《马斯克传》中逆向思维在文中的原话

英文回答:In the literary work entitled 'Elon Musk: Tesla, SpaceX, and the Quest for a Fantastic Future', the concept of reverse thinking is expounded upon in relation to Elon Musk's innovative approach to problem-solving. Musk advocates formencing with the desired oue and systematically working backwards to discern the necessary steps for its attainment. This methodical approach affords him the ability to deconstructplex problems into manageableponents, thereby facilitating the identification of creative solutions that may elude others. Musk's adeptness at reverse thinking has been a pivotal determinant in his capacity as a trailblazing entrepreneur and innovator.文学作品"埃隆·穆斯克:特斯拉"(Elon Musk: Tesla, SpaceX)和"寻找奇妙的未来"(Quest for a Wantific Future)中,结合埃隆·穆斯克解决问题的创新方法,阐述了反向思维的概念。

An Analysis of States in the Phase Space From Quantum Mechanics to General Relativity

An Analysis of States in the Phase Space From Quantum Mechanics to General Relativity

1
ABSTRACT The paper has euristic character. It exploits basic concepts of quantum physics to infer on a selfconsistent basis the properties of the gravitational field. The only assumption of the theoretical model is the quantum uncertainty: the physical properties of quantum systems depends on the delocalization ranges of the constituent particles and not on their local dynamical variables. The conceptual approach follows the same formalism already described in early non-relativistic papers [S. Tosto, Il Nuovo Cimento B, vol. 111, n.2, (1996) and S. Tosto, Il Nuovo Cimento D, vol. 18, n.12, (1996)]. The paper shows that the extended concept of space time uncertainty is inherently consistent with the postulates of special relativity and that the most significant results of general relativity are achieved as straightforward consequence of the space time delocalization of quantum particles.

新事物需要质疑,质疑需要审思作文

新事物需要质疑,质疑需要审思作文

新事物需要质疑,质疑需要审思作文英文回答:In the contemporary world, where advancements are constantly transforming our lives, the importance of questioning new ideas and subjecting them to critical scrutiny cannot be overstated. Questioning is the cornerstone of intellectual progress, allowing us to challenge assumptions, uncover hidden biases, and ultimately arrive at a deeper understanding of the world around us.The first step in questioning is to be open-minded and receptive to new ideas. We must be willing to shed our preconceived notions and biases and approach new information with a fresh perspective. This does not mean accepting everything at face value but rather engaging in thoughtful analysis and evaluation.Critical thinking involves examining the evidence,identifying potential flaws, and evaluating the credibility of sources. It also requires questioning the assumptions underlying an argument and considering alternative viewpoints. By engaging in this process, we can separate facts from opinion, distinguish between strong and weak evidence, and ultimately make more informed decisions.Questioning and critical thinking are not onlyessential for intellectual growth but also for societal progress. In a world where misinformation and propagandaare widespread, the ability to question and critically evaluate information is more important than ever. By questioning authority, challenging conventional wisdom, and holding those in power accountable, we can contribute to a more informed and just society.中文回答:在日新月异的当代世界中,质疑新事物和审慎思考至关重要。

科学发现需要怀疑和坚持 作文

科学发现需要怀疑和坚持 作文

科学发现需要怀疑和坚持作文英文回答:Scientific discovery is a process of ongoing questioning, exploration, and refinement. It requires adeep-seated skepticism and a relentless pursuit of evidence. The scientific method is built upon the foundation of doubt, as it is through challenging existing knowledge and assumptions that new insights can be gained.The ability to question and challenge is essential for scientific progress. It forces scientists to examine their own beliefs and biases, and to consider alternative explanations for their observations. This critical thinking is vital for avoiding confirmation bias, the tendency to seek out evidence that supports one's existing beliefswhile ignoring evidence that contradicts them.Skepticism, however, must be balanced with a strong commitment to empirical evidence. Scientists must bewilling to abandon their cherished theories if the evidence no longer supports them. This requires a degree of intellectual humility and a willingness to admit when one is wrong.The history of science is replete with examples of discoveries that were made as a result of questioning and persistence. The heliocentric model of the solar system,for example, was initially met with great resistance, but eventually prevailed due to the overwhelming evidence inits favor. Similarly, the germ theory of disease wasinitially ridiculed, but eventually became accepted as the basis for modern medicine.These examples demonstrate the transformative power of scientific inquiry. By embracing doubt and relentlessly pursuing evidence, scientists have made countless discoveries that have revolutionized our understanding of the world and improved our lives.中文回答:科学发现是一个持续不断的质疑、探索和完善的过程。

关于小组调查的作文英语

关于小组调查的作文英语

In the realm of academic research and practical problemsolving,group investigations play a pivotal role.These collaborative efforts not only foster a sense of teamwork but also enhance the depth and breadth of the findings.The following narrative illustrates the experience of a group investigation that I,as a seasoned English teacher,have had the privilege to observe and guide.The group consisted of a diverse set of students,each bringing their unique perspectives and skills to the table.The task at hand was to investigate the impact of social media on the mental health of teenagers. This was a topic of significant relevance,given the pervasive nature of social media in the lives of young people today.The initial phase of the investigation involved brainstorming sessions where ideas were freely exchanged.The students were encouraged to voice their opinions without fear of judgment,creating a safe space for open dialogue.This approach was instrumental in generating a wide array of ideas and hypotheses that would guide the subsequent stages of the research.One of the students,a keen observer of social trends,suggested looking into the correlation between the amount of time spent on social media platforms and the levels of reported anxiety and depression among teenagers.Another student,with a background in psychology,proposed examining the role of social comparison and its potential to exacerbate feelings of inadequacy and low selfesteem.As the group delved deeper into the investigation,they divided the work among themselves based on their areas of interest and expertise.Some focused on literature reviews,meticulously sifting through existing research to identify gaps and establish a solid theoretical foundation for their study.Others embarked on designing a survey,ensuring that the questions were clear,unbiased,and relevant to the research objectives.The process was not without its challenges.Disagreements arose over the interpretation of data and the direction the investigation should take. However,these moments served as valuable learning experiences, teaching the students the importance of critical thinking and the art of negotiation.One particularly memorable incident involved a heated debate over the statistical significance of their findings.The group had to revisit their methodology and consider alternative explanations for their results.This exercise not only strengthened their analytical skills but also highlighted the importance of being open to new perspectives and being willing to revise ones initial conclusions.The culmination of the group investigation was the presentation of their findings at a schoolwide seminar.The students had prepared a comprehensive report,complete with visual aids and an engaging narrative that brought their research to life.The audience,comprising fellow students,teachers,and invited guests,was captivated by their insights and the depth of their analysis.The groups investigation revealed that while social media can provide a platform for connection and selfexpression,it can also contribute to feelings of social isolation and selfdoubt,particularly when used excessively or in a manner that encourages comparison with others.The findings underscored the need for a balanced approach to social media usage and the importance of fostering resilience and a healthy selfimage among teenagers.The experience of guiding this group investigation was both rewarding and enlightening.It was a testament to the power of collaboration and the potential for young minds to contribute meaningfully to important societal conversations.As an educator,I was proud to witness the growth and development of these students,not just in terms of their research skills but also in their ability to navigate complex issues with empathy,curiosity,and a commitment to truth and integrity.。

做决定之前思考英文作文

做决定之前思考英文作文

做决定之前思考英文作文Title: The Art of Decision-Making: Unleashing the Imagination。

1. Embrace the Randomness: In the realm of life's choices, don't be a statistician, be a magician. Each decision, like a coin toss, holds the potential for surprise. Don't plan your moves, let the serendipity guide you. 。

2. Question Your Assumptions: The key to bold moves is questioning the norm. Don't let your preconceived notions dictate your path. Instead, ask, "Why not?" and let curiosity be your compass.3. Embrace the Unknown: The path less traveled is often the most rewarding. Don't fear the unknown, embrace it as a stepping stone to personal growth. It's in the uncertainty that we discover hidden treasures.4. Reflect, Don't React: Before you leap, take a moment to ponder. Reflecting allows for deeper understanding, reducing the likelihood of regretful choices. 。

The QCD Coupling Constant

The QCD Coupling Constant
was supported in part by the Director, Office of Science, Office of High Energy
and Nuclear Physics, Division of High Energy Physics of the U.S. Department of Energy under Contracts DE-AC03-76SF00098.
KEYWORDS: QCD,
ABSTRACT: This paper presents a summary of the current status of determinations of the strong coupling constant αs . A detailed description of the definition, scale dependence and inherent theoretical ambiguities is given. The various physical processes that can be used to determine αs are reviewed and attention is given to the uncertainties, both theoretical and experimental.
10 15 15
αs FROM τ DECAY . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . αs FROM LATTICE GAUGE THEORY COMPUTATIONS . . . . . . . . . . . . αs FROM HEAVY QUARK SYSTEMS . . . . . . . . . . . . . . . . . . . . . . . . αs FROM HADRON-HADRON SCATTERING . . . . . . . . . . . . . . . . . . . CONCLUSION . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

Concepts of Heavy-Ion Physics

Concepts of Heavy-Ion Physics
CONCEPTS OF HEAVY-ION PHYSICS∗
Ulrich Heinz Department of Physics, The Ohio State University, Columbus, OH 43210, USA Abstract In these lectures I present the key ideas driving the field of relativistic heavyion physics and develop some of the theoretical tools needed for the description and interpretation of heavy-ion collision experiments. 1 PROLOGUE: THE BIG BANG AND THE EARLY UNIVERSE Matter as we know it, made up from molecules which consist of atoms which consist of electrons circling around a nucleus which consists of protons and neutrons which themselves are bound states of quarks and gluons, has not existed forever. Our universe originated in a “Big Bang” from a state of almost infinite energy density and temperature. During the first few microseconds of its life the energy density in our universe was so high that hadrons (color singlet bound states of quarks, antiquarks and gluons), such as the nucleons inside a nucleus, could not form. Instead, the quarks, antiquarks and gluons were deconfined and permeated the entire universe in a thermalized state known as quark-gluon plasma (QGP). Only when the energy density of the universe dropped below the critical value ecr ≃ 1 GeV/fm3 and its temperature decreased below Tcr ≈ 170 MeV, colored degrees of freedom became confined into color singlet objects of about 1 fm diameter: the first hadrons formed. After the universe hadronized, it took another 200 s or so until its temperature dropped below ∼ 100 keV such that small atomic nuclei could form and survive. This is known as primordial nucleosynthesis. At this point (i.e. after “The First 3 Minutes”) the chemical composition of the early universe was fixed (“chemical freeze-out”). All unstable hadrons had decayed and all antiparticles had annihilated, leaving only a small fraction of excess protons, neutrons and electrons, with all surviving neutrons bound inside small atomic nuclei. The chemical composition of the universe began to change again only several hundred million years later when the cores of the first stars ignited and nuclear fusion processes set in. After primordial nucleosynthesis the universe was still ionized and therefore completely opaque to electromagnetic radiation. About 300 000 years after the Big Bang, when the temperature had reached about 3000 K, electrons and atomic nuclei were finally able to combine into electrically neutral atoms, and the universe became transparant. At this point the electromagnetic radiation decoupled, with a perfectly thermal blackbody spectrum of T ≈ 3000 K (“thermal freeze-out”). Due to the continuing expansion of our universe this thermal photon spectrum has now been redshifted to a temperature of about 2.7 K and turned into the “cosmic microwave background”. The number of photons in this microwave background is huge (about 250 photons in every cm3 of the universe), and they carry the bulk of the entropy of the universe. The entropy-to-baryon ratio of the universe is S/A ≃ 109±1 ; its inverse provides a measure for the tiny baryon-antibaryon asymmetry of our universe when it hadronized – a still incompletely understood small number. The only other surviving feature of the Big Bang is the ongoing Hubble expansion of our universe, and the structure of its density fluctuations, amplified over eons by the action of gravity and reflected in today’s distribution of stars, galaxies, galactic and supergalactic clusters, and dark matter. Using these 3 or 4 observational pillars (today’s expansion rate or “Hubble constant”, the microwave background spectrum and its fluctuations, the primordial nuclear abundances and, most recently, also today’s spectrum
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a r X i v :0801.1937v 1 [h e p -p h ] 13 J a n 20081Absence of coexisting phase of quark-antiquark and diquark condensed phases in the extended Gross-Neveu model in 2+1dimensionsAkira Ni ´e gawaGraduate School of Science,Osaka City University,Sumiyoshi-ku,Osaka 558-8585,JAPANWe show that the coexisting phase of quark-antiquark and diquark condensed phases is absent in the cold quark matter in the 2+1dimensional extended Gross-Neveu model,which is in sharp contrast to the case of 3+1dimensional Nambu–Jona-Lasinio model.§1.IntroductionExtensive studies for last decade on quark matters have disclosed the existence of various phases.Among those are the quark-antiquark (q ¯q )condensed phase,1)different diquark (qq )condensed phases.Furthermore,it has been suggested 2)that the coexisting phase of q ¯q and qq condensations also exists.(For recent reviews,see,e.g.,.3))One of the important theoretical models for studying this issue is the extended Nambu–Jona-Lasinio (NJL)model,which is an low energy effective theory of QCD.3)The Gross-Neveu (GN)model 4)proposed in 1974is the counterpart of the NJL model in 1+1and 2+1dimensional spacetime.Study of the field theoretic models in lower spacetime dimension are interesting in itself as in the solid-state physics.Various works have been devoted to the study of the GN model.(References together with a brief survey of them are given in.5))Recently,the phase structure of the 2+1dimensional (3D)extended GN model has been studied within the mean-field ap-proximation.5)In,5)quarks are assigned to the lowest nontrivial (2-dimensional)representation of the O (2,1)group,which we refer to as the 2d-spinor quarks.The model contains essentially two parameters,the q ¯q coupling constant G S and qq cou-pling constant G D .Through numerical analyses for some sets of values of (G S ,G D ),it has been shown that there appears q ¯q -and qq -condensed phases but no coexisting phase appears,which is in sharp contrast to the case of NJL model.The purpose of this note is to analytically prove the absence of the coexisting phase for any values of G S (>0)and G D .We restrict to the cold “quark matter”with zero temperature (T =0).§2.PreliminaryThe Lagrangian of the extended GN model with 2d-spinor quarks readsL =¯qi∂/+µγ0q +G S (¯q q )2+G D (¯q τ2λ2q c )(¯q c τ2λ2q ),(2.1)typeset using P T P T E X.cls Ver.0.92Akira Ni´e gawawhereµis the quark chemical potential.The quarkfields,q and¯q,are the doublets in theflavor space and the triplets in the color space.q c and¯q c are the charge-conjugatedfields.The Pauli matrixτ2acts on theflavor space,while the Gell-Mann matrix acts on the color space.Employing the mean-field approximation,we get L=¯q i∂/−σ+µγ0 q−12∆∗(¯q cτ2λ2q)−σ24GD.(2.2) Hereσ=−2G S ¯q q ,∆=−2G D ¯q cτ2λ2q ,(2.3) whereσand∆are the order parameters for the q¯q and qq condensations,respectively. Computation of the thermodynamic potential at T=0yields5)Ω=σ24G D−∞σdEE2µ2+σ2|∆|2,E=E2+σ2|∆|2/µ2±µ,theintegrals in(2.4)that contain E±∆may be carried out analytically.We perform renormalization as in,5)and choose,without loss of generality,∆to be real and positive.Then,we introduce following dimensionless quantities:x=σ/µ(≥0),y=˜∆/µ(≥1),A=−2π4G S−3αµ 14,Ω(x,y)=2π∆2+µ2.After all this,we obtainΩ(x,y)=12 (x−1)|x−1|−(x+1)2+2xy−1+|x−y|.(2.7)Note that,for the normal phase,(x,y)=(0,1),Ω(x=0,y=1)=−1.Throughout in this paper,we restrict to the case0<A,the case in which the quark-antiquark condensate can appear.Absence of coexistiong phase in the 3D Gross-Neveu model32.1.Quark-antiquark condensationHere we study the case with y =1(∆=0):Ωx (x )≡Ω(x,y =1)=(3−A )x 2−1.(2.8)Straightforward analysis yieldsΩx ≥−1for A ≤3−A 3/27for 3≤A≡˜Ωx (2.9)2.2.Diquark condensationHere we study the case with x =0(σ=0):Ωy (y )≡Ω(x =0,y )=43,(2.10)where L (y )≡ln[(y +1)/(y −1)].Ωy (y )is minimum at y =y 0:2y 0−L (y 0)=B ,(2.11)Ωy (y 0)=−1dyy =B/2y −BB 2−4y +4BB 2−4y 0−4B2B+22B 2L (B/2).(2.16)Here and in the following,we frequently use the inequality:2(y −1)≤(y 2−1)L (y )≤2y(1≤y ).(2.17)4Akira Ni´e gawaUsing this in(2.16),we obtainy0≥B B2 ≡y′0 .(2.18) Substituting(2.18)into(2.12),we obtainΩy(y0)≤−112−B+53y3−B(y2−1)−2y−(y2−1)L(y)−13y3−B(y2−1)−A+22.(3.5)We next study∆x˜ΩI(y=B/2)≡˜ΩI(y=B/2)−˜Ωx=A312+B−A+2Absence of coexistiong phase in the3D Gross-Neveu model5in the region(3.5).∆x˜ΩI(y=B/2)monotonically decreases with increasing B (for2<B).Then,from(3.5),∆x˜ΩI(y=B/2)≥ ∆x˜ΩI(y=B/2) B=(A+1)/2 (≡H(A)),which is a polynomial in A.It can easily be seen that H(A)increases with increasing A(3≤A)and0≤H(A).Equality holds for A=3and then B=2, where H(A)>Ωy(y0).Note that we have not used the constraint on y that comes from F(y)≤0(see above after(3.2)).§4.Region II((1≤)y≤x)In this region,Ω(x,y)=2x3−Ax2+(y2−1)G(x)(4.1)G(x)=2x−B+(x2−1)L(x).(4.2) For0≤G(x),Ω(x,y)≥Ω(x,y=1)=Ωx(x),and then we restrict to the region G(x)≤0,whereΩ(x,y)≥Ω(x,y=x)=4x3−(A+B)x2−2x+(x2−1)2L(x)+B ≡˜ΩII(x) .(4.3)˜ΩII(x)is minimum at x=x0:5x0+2(x20−1)L(x0)=A+B,(4.4)1˜ΩII(x0)=.(4.7)4Since1≤x,2≤B.In the following,putting aside the equation(4.4),we regard˜ΩII(x0)in(4.5)as a function of x0and show that∆˜ΩII(x0)>0.It can be shown that,in the region of our interest,1≤x0≤(A+B+4)/9,the polynomial˜ΩII(x0)monotonically decreases with increasing x0.6Akira Ni´e gawaWe recall the condition,Eq.(4.7).(A+B+4)/9≤(B+2)/4or A≤(5B+2)/4:In this region,˜ΩII(x0)≥˜ΩII(x0= (B+2)/4).The polynomial∆x˜ΩII(x0=(B+2)/4)(≡∆xˆΩ(A,B))increases mono-tonically with increasing A(in the region of our interest).Since(5B+2)/4≤A,∆xˆΩ(A,B)≥∆xˆΩ(A=(5B+2)/4,B),which is a polynomial in B.This polynomial increases monotonically with increasing(2≤)B and∆xˆΩ(A=(5B+2)/4,B)≥0. The equality holds for B=2and then A=3.At(A,B)=(3,2),ˆΩ−Ωy>0.§5.Region III(1<x<y)In this region,2Ω(x,y)=y3−2y−B(y2−1)−(y2−1)L(y).(5.1)3With respect to x,Ω(x,y)in(5.1)is minimum at x=x0:x0=A−2y−(y2−1)L(y).(5.2) The following four regions should be studied:Region IIIA:(5.2)does not have a solution in the region,1≤x0and1≤y.Region IIIB:x0≤1.Region IIIC:(1≤)y≤x0.region IIID:1<x0<y.Region IIIA and Region IIIBΩ(x,y)in(5.1)monotonically increases with increasing(1≤)x.Then,Ω(x,y)≥Ω(x=1,y),which is the same as(3.3)in the case of Region I above.Then,∆Ω(x,y)>0.Region IIICΩ(x,y)monotonically decreases with increasing x(1<x≤y).Then,Ω(x,y)≥Ω(x=y,y),which is the same as˜ΩII(y)in(4.3)in the case of Region II above,and then we briefly describe.In the present case,from(5.2)with(2.17),the conditiony≤x0yieldsA+2(1≤)y=x≤Absence of coexistiong phase in the3D Gross-Neveu model7 (A+B+4)/9≤(A+2)/5or B≤2(2A−1)/5:In this region,∆y˜ΩII(x0)≥∆y˜ΩII(x0=(A+2)/5)(≡∆yˆΩ(A,B)),which increases monotonically with increas-ing B.Since2(2A−1)/5<B,∆yˆΩ(A,B)≥∆yˆΩ(A,B=2(2A−1)/5),which is a polynomial in A.This polynomial increases with increasing(3≤)A and is positive.5.1.Region IIIDIn this region,Ω(x,y)≥Ω(x0,y)(Eq.(5.1)):Ω(x0,y)=−x203y3−B(y2−1)−A,(5.4)where x0is as in(5.2).Using(2.17),the condition1<x0<y yieldMax 1,A4,(5.5) from which we can restrict to the region A≤3because1≤y.Ignoring the explicit form of x0,we analyze the functionΩ(x0,y).SinceΩ(x0,y) monotonically decreases with increasing(1≤)x0,Ω(x0,y)>Ω(x0=y,y)=y3−B(y−1)+y−A≡˜Ω(A,B;y).(5.6) For B≤2,˜Ωmonotonically increases with increasing(1≤)y,and then˜Ω(A,B;y)≥˜Ω(A,B;y=1)=2−A≥˜Ωx.For2≤B,˜Ω(A,B;y)is minimum aty0=1B2−3 ,˜Ω(A,B;y0)=−2B2−3 +108(A+1) 3(A+1)2+3(A+1)+16 ,(5.8) which is an increasing function of(3<)A.Then,For B≤B0(A),y0≤(A+1)/4,For B0(A)<B,(A+1)/4<y0,(5.9)8Akira Ni´e gawaRegion:2≤B ≤B 0(A )(3≤A )We first analyze ∆x ˜Ω≥A 3/27+˜Ω(A,B 0;y 0(B 0)).Numerical computation shows that A 3/27+˜Ω(A,B 0;y 0(B 0))≤0for A <4.173....Then,we analyze ∆y ˜Ωfor A ≤4.18:∆y ˜Ω(A,B ;y 0)≥∆y ˜Ω(A =4.18,B ;y 0)=B 39B −43−4.18.(5.10)It can easily be seen that this polynomial is positive for A ≤3≤4.18.Region:B 0(A )≤B (3≤A )In this case,˜Ω(A,B ;y )≥˜Ω(A,B ;y =(A +1)/4)=(A +1)34(A +1)+1−110891(A +1)−192+352108[91(A +1)−192](≡B 1(A )).(5.12)Numerical computation shows that,for A ≤A 0=4.396...[A 0<A ],B 1≤B 0[B 0<B 1].Then,the region of our interest is as follows:For A ≤A 0,B 0(A )≤B ,For A 0<A ,B 1(A )<B.(5.13)Now,we analyze ∆y ˜Ωfor B 1(A )≤B and B 0(A )≤B ,which is polynomial in A and B .For A +1≤√32<A +1,this polynomial takes minimum at B =B 2(A ):B 2(A )=1(A +1)2−32.(5.14)√:Numerical computation shows that,For A ≤A 2=9.84...,B 2≤B 0,For A 2<A ,B 0<B 2.(5.15)On the other hand,one can analytically show that B 2<B 1.After all of this,we learnthat the region (of A and B )that should be analyzed is (A 0,B 1)≤(A,B ).In thisregion,∆y ˜Ω(A,B )>∆y ˜Ω(A,B 1),which is polynomial in A .It is straightforward to show that this polynomial ∆y ˜Ω(A,B 1)is positive for A 0≤A .A +1<√:From the above analysis,we see that,for A 0≤A ≤√Absence of coexistiong phase in the3D Gross-Neveu model9 A and is positive.In the latter case,∆y˜Ω≥∆y˜Ω(B=B0)≥∆y˜Ω(B=B′0),(5.16)whereB′0(A)=14.4+1 (<B0(A)),(5.17)which holds in the region under study.One can see that he last expression in(5.16), which is polynomial in A,is positive in the region of interest.§6.Concluding remarkWe have studied the phase structure of the extended3D Gross-Neveu model with2d-spinor quarks.The following results are obtained.(I)There does not appear the region where the quark-antiquark and diquark con-densations coexist.(II)The diquark condensed state is always energetically favored over the normal vacuum(see after(2.13)).(III)From(I)and(II),we see that,for a given q¯q coupling constant A,there is the critical value,B c for the qq coupling constant B:For B≤B c,q¯q-condensed state is realized,while,for B c<B,the qq-condensed state is realized.AcknowledgementI would like to thank M.Inui and H.Kohyama for useful discussions.References1)T.Hatsuda and T.Kunihiro,Phys.Rep.247(1994),221.Earlier works are quoted therein.2)T.M.Schwarz,S.P.Klevansky and G.Papp,Phys.Rev.C60(1999),055205;B.Vander-heyden and A.D.Jackson,Phys.Rev.D62(2000),094010.3)M.Huang,Int.J.Mod.Phys.E14(2005),675;M.Buballa,Phys.Rep.407(2005),205.4) D.J.Gross and A.Neveu,Phys.Rev.D10(1974),3235.5)H.Kohyama,hep-ph/0706.1153,to be published in Phys.Rev.D.。

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