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1.
[1]J.H. Hamilton,A. VRamayya, W.T. Pinkston, et al.,Phys. Rev. Lett. 32 (1974) 239. [2]R. Julin, K. Helariutta, and M. Muikku, J. Phys. G 27(2001) R109. [3]J.H. Hamilton, Nukleonika 24 (1979) 561. [4]W.C. Ma, et al., Phys. Lett. B 139 (1984) 276. [5]R. Bengtsson, et al., Phys. Lett. B 183 (1987) 1. [6]S. Yoshida and N. Takigawa, Phys. Rev. C 55 (1996)1255. [7]T. Niksic, D. Vretenar, P. Ring, et al., Phys. Rev. C 65(2002) 054320. [8]F.G. Condev, M.P. Carpenter, R.V.F. Janssens, et al.,Phys. Lett. B 528 (2002) 221. [9]D.G. Jenkins, A.N. Andreyev, R.D. Page, et al., Phys.Rev. C 66 (2002) 011301(R). [10]B.D. Serot and J.D. Walecka, Adv. Nuc]. Phys. 16 (1986)1. [11]P. Ring, Prog. Part. Nucl. Phys. 37 (1996) 193. [12]J. Meng and P. Ring, Phys. Rev. Lett. 77 (1996) 3963. [13]J. Meng and P. Ring, Phys. Rev. Lett. 80 (1998) 460. [14]S.K. Patra, S. Yoshida, N. Takigawa, and C.R. Praharaj,Phys. Rev. C 50 (1994) 1924. [15]S. Yoshida, S.K. Patra, N. Takigawa, and C.R. Praharaj,Phys. Rev. C 50 (1994) 1938. [16]G.A. Lalazissis and P. Ring, Phys. Lett. B 427 (1998)225. [17]Jun-Qing Li, Zhong-Yu Ma, Bao-Qiu Chen, and Yong Zhou, Phys. Rev. C 65 (2002) 064305. [18]G. Audi and A.H. Wapstra, Nucl. Phys. A 565 (1993) 1. [19]G. Audi and A.H. Wapstra, Nucl. Phys. A 595 (1995)409. [20]G. Audi and A.H. Wapstra, Nucl. Phys. A 624 (1997) 1. [21]P. MOller and J.R. Nix, Atom. Data and Nucl. Data Table 59 (1995) 307.  相似文献   

2.
[1]R. Casalbuoani, A. Deandrea, and M. Oertel, JHEP 032(2004) 0402. [2]G. Hooft, In Search of the Ultimate Building Blocks, Cambridge University Press, Cambridge (1997). [3]J. Belazey, Searches for New Physics at Hadron Coliders,Northern Illinois University (2005). [4]N. Arkani-hamed, A.G. Cohen, and H. Georgi, Phys. Lett.B 513 (2001) 232 [hep-ph/0105239]. [5]I. Low, W. Skiba, and D. Smith, Phys. Rev. D 66 (2002)072001 [hep-ph/0207243]. [6]N. Arkani-hamed, A.G. Cohen, E. Katz, and A.E. Nelson,JHEP 0207 (2002) 304 [hep-ph/0206021]. [7]N. Arkani-hamed, A.G. Cohen, E. Katz, A.E. Nelson, T.Gregoire, and J. G. Wacker, JHEP 0208 (2002) 021 [hepph/0206020]. [8]T. Gregoire and J.G. Wacker, JHEP 0208 (2002) 019[hep-ph/0206023]. [9]For a recent review, see e.g., M. Schmaltz, Nucl. Phys. B (Proc. Suppl.) 117 (2003) 40. [10]N. Arkani-hamed, A.G. Cohen, T. Gregoire, and J.G.Jacker, JHEP 0208 (2002) 020 [hep-ph/0202089]. [11]or a recent review, see e.g., M. Schmaltz, Nucl. Phys.Proc. Suppl. 117 (2003) 40 [hep-ph/0210415]. [12]E. Katz, J. Lee, A.E. Nelson, and D.G. Walker, hepph/0312287. [13]M. Beneke, I. Efthymiopoulos, M.L. Mangano, et al., hepph/0003033. [14]D.O. Carlson and C.-P. Yuan, hep-ph/9211289. [15]R. Frey, D. Gerdes, and J. Jaros, hep-ph/9704243. [16]G. Eilam, J.L. Hewett, and A. Soni, Phys. Rev. D 44(1991) 1473; W.S. Hou, Phys. Lett. B 296 (1992) 179; K.Agashe and M. Graesser, Phys. Rev. D 54 (1996) 4445;M. Hosch, K. Whisnant, and B.L. Young, Phys. Rev. D56 (1997) 5725. [17]C.S. Li, R.J. Oakes, and J.M. Yang, Phys. Rev. D 49(1994) 293, Erratum-ibid. D 56 (1997) 3156; G. Couture,C. Hamzaoui, and H. Koenig, Phys. Rev. D 52 (1995)1713; G. Couture, M. Frank, and H. Koenig, Phys. Rev.D 56 (1997) 4213; G.M. de Divitiis, et al., Nucl. Phys. B 504 (1997) 45. [18]B. Mele, S. Petrarca, and A. Soddu, Phys. Lett. B 435(1998) 401. [19]B. Mele, hep-ph/0003064. [20]J.M. Yang and C.S. Li, Phys. Rev. D 49 (1994) 3412,Erratum, ibid. D 51 (1995) 3974; J.G. Inglada, hepph/9906517. [21]L.R. Xing, W.G. Ma, R.Y. Zhang, Y.B. Sun, and H.S.Hou, Commun. Theor. Phys. (Beijing, China) 41 (2004)241. [22]L.R. Xing, W.G. Ma, R.Y. Zhang, Y.B. Sun, and H.S.Hou, Commun. Theor. Phys. (Beijing, China) 40 (2003)171. [23]T. Han, H.E. Logan, B. McElrath, and L.T. Wang, Phys.Rev. D 67 (2003) 095004. [24]I. Low, W. Skiba, and D. Smith, Phys. Rev. D 66 (2002)072001. [25]T. Han, H.E. Logan, B. McElrath, and L.T. Wang, hepph/0302188. [26]A.J. Buras, A. Poschenrieder, and S. Uhlig, hepph/0410309. [27]S. Eidelman, et al., Phys. Lett. B 592 (2004) 1. [28]F. Legerlehner, DESY 01-029, hep-ph/0105283.  相似文献   

3.
《Physics letters. [Part B]》1999,446(2):170-174
We consider the propagation of light in the QED vacuum between an unusual pair of parallel plates, namely: a perfectly conducting one (ϵ→∞) and an infinitely permeable one (μ→∞). For weak fields and in the soft photon approximation we show that the speed of light for propagation normal to the plates is smaller than its value in unbounded space (in contrast to the original Scharnhorst effect [K. Scharnhorst, Phys. Lett. B 236 (1990) 354, G. Barton, Phys. Lett. B 237 (1990) 559, G. Barton, K. Scharnhorst, J. Phys. A 26 (1993) 2037]).  相似文献   

4.
《中国物理 B》2021,30(6):67505-067505
Recent experiments [Guo et al., Phys. Rev. Lett. 124 206602(2020)] on thermodynamic properties of the frustrated layered quantum magnet SrCu_2(BO_3)_2-the Shastry–Sutherland material-have provided strong evidence for a lowtemperature phase transition between plaquette-singlet and antiferromagnetic order as a function of pressure. Further motivated by the recently discovered unusual first-order quantum phase transition with an apparent emergent O(4) symmetry of the antiferromagnetic and plaquette-singlet order parameters in a two-dimensional "checkerboard J-Q" quantum spin model[Zhao et al., Nat. Phys. 15 678(2019)], we here study the same model in the presence of weak inter-layer couplings. Our focus is on the evolution of the emergent symmetry as the system crosses over from two to three dimensions and the phase transition extends from strictly zero temperature in two dimensions up to finite temperature as expected in SrCu_2(BO_3)_2.Using quantum Monte Carlo simulations, we map out the phase boundaries of the plaquette-singlet and antiferromagnetic phases, with particular focus on the triple point where these two ordered phases meet the paramagnetic phase for given strength of the inter-layer coupling. All transitions are first-order in the neighborhood of the triple point. We show that the emergent O(4) symmetry of the coexistence state breaks down clearly when the interlayer coupling becomes sufficiently large, but for a weak coupling, of the magnitude expected experimentally, the enlarged symmetry can still be observed at the triple point up to significant length scales. Thus, it is likely that the plaquette-singlet to antiferromagnetic transition in SrCu_2(BO_3)_2 exhibits remnants of emergent O(4) symmetry, which should be observable due to additional weakly gapped Goldstone modes.  相似文献   

5.
[1]V.D.Burkert,Phys.Lett.B 72 (1997) 109. [2]S.Capstick and W.Roberts,Prog.Part.Nucl.Phys.45 (2000) S241,and references therein. [3]B.S.Zou,Nucl.Phys.A 675 (2000) 167c; B.S.Zou,Nucl.Phys.A 684 (2001) 330; BES Collaboration (J.Z.Bai,et al.) Phys.Lett.B 510 (2001) 75; BES Collaboration (M.Ablikim,et al.),hep-ex/0405030. [4]R.Sinha and Susumu Okubo,Phys.Rev.D 30 (1984)2333. [5]W.H.Liang,P.N.Shen,B.S.Zou,and A.Faessler,Euro.Phys.J A 21 (2004) 487. [6]Particle Data Group,Euro.Phys.J.C 15 (2000) 1. [7]K.Tsushima,A.Sibrtsev,and A.W.Thomas,Phys.Lett.B 390 (1997) 29. [8]J.Kogut,Rev.Mod.Phys.51 (1979) 659; Rev.Mod.Phys.55 (1983) 775. [9]Q.Haider and L.C.Liu,J.Phys.G 22 (1996) 1187; L.C.Liu and W.X.Ma,J.Phys.G 26 (2000) L59. [10]V.G.J.Stoks,R.A.M.Klomp,C.P.F.Terheggen,and J.J.de Swart,Phys.Rev.C 49 (1994) 2950. [11]H.Haberzettl,C.Bennhold,T.Mart,and T.Feuster,Phys.Rev.C 58 (1998) R40. [12]Y.Oh,A.I.Titov,and T.-S.H.Lee,Phys.Rev.C 63(2001) 25201.  相似文献   

6.
Strange stars (ReSS) calculated from a realistic equation of state (EOS), that incorporate chiral symmetry restoration as well as deconfinement at high density [Phys. Lett. B 438 (1998) 123; Phys. Lett. B 447 (1999) 352, Addendum; Phys. Lett. B 467 (1999) 303, Erratum; Indian J. Phys. B 73 (1999) 377] show compact objects in the mass radius curve. We compare our calculations of incompressibility for this EOS with that of nuclear matter. One of the nuclear matter EOS has a continuous transition to ud-matter at about five times normal density. Another nuclear matter EOS incorporates density dependent coupling constants. From a look at the consequent velocity of sound, it is found that the transition to ud-matter seems necessary.  相似文献   

7.
[1]J.Gasser,H.Leutwyler,and M.E.Sainio,Phys.Lett.B 253 (1991) 252. [2]John Ellis,Eur.Phys.J.A 24S2 (2005) 3,[arXive:hepph/0411369]. [3]T.Inoue,V.E.Lyubovitskij,Th.Gutsche,and Amand Faessler,Phys.Rev.C 69 (2004) 035207,[arXive:hepph/0311275]. [4]M.M.Pavan,I.I.Strakovsky,R.L.Workman,and R.A.Arndt,PiN Newslett.16 (2002) 110,[arXive:hepph/0111066]. [5]V.E.Lyubovitskij,Th.Gutsche,Amand Faessler,and E.G.Drukarev,Phys.Rev.D 63 (2001) 054026,[arXive:hep-ph/0009341]. [6]S.D.Bass,Phys.Lett.B 329 (1994) 358,[arXive:hepph/9404294]. [7]Marc Knecht,PiN Newslett.15 (1999) 108,[arXive:hepph/9912443]. [8]P.Schweitzer,Phys.Rev.D 69 (2004) 034003. [9]B.C.Lehnhart,J.Gegelia,and S.Scherer,J.Phys.G 31(2005) 89,[arXive:hep-ph/0412092]. [10]P.J.Ellis and K.Torikoshi,Phys.Rev.C 61 (1999)015205. [11]Gerald E.Hite,William B.Kaufmann,and Richard J.Jacob,Phys.Rev.C 71 (2005) 065201. [12]S.Weinberg,Physica A 96 (1979) 327. [13]J.Gasser and H.Leutwyler,Nucl.Phys.B 250 (1985)465. [14]J.Gasser,M.E.Sainio,and A.Svarc,Nucl.Phys.B 307(1988) 779. [15]P.Papazoglou,D.Zschiesche,S.Schramm,J.SchaffnerBielich,H.St(o)cker,and W.Greiner,Phys.Rev.C 59(1999) 411. [16]T.Fuchs and J.Gegelia,Phys.Rev.D 68 (2003) 056005.  相似文献   

8.
[1]M.Alford,K.Rajagopal,and F.Wilczek,Phys.Lett.B 422 (1998) 247; Nucl.Phys.B 537 (1999) 443. [2]M.Gyulassy and L.McLerran,arXiv:nucl-th/0405013;E.V.Shuryak,arXiv:hep-ph/0405066. [3]K.Rajagopal and F.Wilczek,hep-ph/0011333. [4]M.Alford,Chris Kouvaris,and K.Rajagopal,hepph/0406137. [5]Y.Nambu and G.Jona-Lasinio,Phys.Rev.122 (1961)345. [6]R.T.Cahill and C.D.Roberts,Phys.Rev.D 32 (1985)2419. [7]R.T.Cahill and Susan M.Ganner,hep-ph/9812491. [8]A.W.Steiner,S.Reddy,and M.Prakash,Phys.Rev.D 66 (2002) 094007. [9]P.Amore,M.C.Birse,J.A.McGovern,and N.R.Walet,Phys.Rev.D 65 (2002) 074005. [10]M.Alford and K.Rajagopal,JHEP 0206 (2002) 031. [11]Xiao-Fu Li,Yu-Xin Liu,Hong-Shi Zong,and En-GuangZhao,Phys.Rev.C 58 (1998) 1195. [12]H.Reinhardt,Phys.Lett.B 244 (1990) 2. [13]Steven Weinberg,The Quantum Theory of Fields,Vol.2,Cambridge University Press,Cambridge (1996) p.348.  相似文献   

9.
D. V. Antonov 《JETP Letters》1997,65(9):701-707
The correction to the Hamiltonian of a quark-antiquark system due to the rigidity term in the action of the gluodynamics string is found using the action obtained by D. V. Antonov et al., Mod. Phys. Lett. A 11, 1905 (1996) with the Hamiltonian obtained by A. Yu. Dubin et al., Phys. At. Nucl. 56, 1745 (1993); Phys. Lett. B 323, 41 (1994) and E. L. Gubankova and A. Yu. Dubin, Phys. Lett. B 334, 180 (1994); preprint ITEP 62-94. This correction contains additional contributions to the orbital momentum of the system and several higher derivative operators. The resulting Hamiltonian is used to evaluate the rigid-string-induced term in the Hamiltonian of the relativistic quark model for the case of large masses of the quark and antiquark. Pis’ma Zh. éksp. Teor. Fiz. 65, No. 9, 673–678 (10 May 1997) Published in English in the original Russian journal. Edited by Steve Torstveit.  相似文献   

10.
[1]J. Nagamatsu, N. Nakagava, T. Muranaka, Y. Zenitani,and J. Akimitsu, Nature 410 (2001) 63. [2]C. Buzea and T. Yamashita, Supercond. Sci. Techn. 14(2001) R115. [3]S. Budko, G. Lapertot, C. Petrovic, C.E. Gunningham, N.Anderson, and P.C. Canfield, Phys. Rev. Lett. 86 (2001)1877. [4]H. Kotegawa, K. Ishida, Y. Kitaoka, T. Muranaka, and J. Akimitsu, Phys. Rev. Lett. 87 (2001) 127001. [5]J. Kortus, I.I. Mazin, K.D. Belashchenko, V.P. Antropov,and L.L. Boyer, Phys. Rev. Lett. 87 (2001) 4656. [6]A. Liu, I.I. Mazin, and J. Kortus, Phys. Rev. Lett. 87(2001) 087005. [7]X.K. Chen, M.J. Konstantinovich, J.C. Irwin, D.D.Lawrie, and J.P. Frank, Phys. Rev. Lett. 87 (2001)157002. [8]H. Giublio, D. Roditchev, W. Sacks, R. Lamy, D.X.Thanh, J. Kleins, S. Miraglia, D. Fruchart, J. Markus,and P. Monod, Phys. Rev. Lett. 87 (2001) 177008. [9]F. Bouquet, R.A. Fisher, N.E. Phillips, D.G. Hinks, and J.D. Jorgensen, Phys. Rev. Lett. 87 (2001) 04700. [10]S.V. Shulga, S.-L. Drechsler, H. Echrig, H. Rosner, and W. Pickett, Cond-mat/0103154 (2001). [11]A.A. Golubov, J. Kortus, O.V. Dolgov, O. Jepsen, Y.Kong, O.K. Andersen, B.J. Gibson, K. Ahn, and R.K.Kremer, J. Phys. Condens. Matter 14 (2002) 1353. [12]H. Doh, M. Sigrist, B.K. Chao, and Sung-Ik Lee, Phys.Rev. Lett. 85 (1999) 5350. [13]I.N. Askerzade, N. Guclu, and A. Gencer, Supercond. Sci.Techn. 15 (2002) L13. [14]I.N. Askerzade, N. Guclu, A. Gencer, and A. Kiliq, Supercond. Sci. Techn. 15 (2002) L17. [15]I.N. Askerzade and A. Gencer, J. Phys. Soc. Jpn. 71(2002) 1637. [16]I.N. Askerzade, Physica C 397 (2003) 99. [17]V.V. Anshukova, B.M. Bulychev, A.I. Golovashkin, L.I.Ivanova, A.A. Minakov, and A.P. Rusakov, Phys. Solid State 45 (2003) 1207. [18]A.A. Abrikosov, Fundamentals of the Theory of Metals,North-Holland, Amsterdam (1988). [19]M.N. Kunchur, S.I. Lee, and W.N. Kang, Phys. Rev. B 68 (2003) 064516.  相似文献   

11.
We study certain mild degenerations of algebraic varieties which appear in the analysis of a large class of supersymmetric theories, including superstring theory. We analyze Witten’s σ-model [Nucl. Phys. B 403 (1993) 159] and find that the non-transversality of the superpotential induces additional singularities and a stratification of the ground state variety. This stratified variety admits certain homology groups such that ⊕qH2q satisfies the “Kähler package” of requirements [Ann. Math. Studies 102 (1982) 303]. Also, this ⊕qH2q extends the “flopped” pair of small resolutions [Nucl. Phys. B 416 (1994) 414; Nucl. Phys. B 330 (1990) 49; Commun. Math. Phys. 119 (1988) 431] to an “(exo)flopped” triple, and is compatible with both mirror symmetry [S.-T. Yau (Ed.), Mirror Manifolds, International Press, Hong Kong, 1990; B. Greene, S.-T. Yau (Eds.), Mirror Manifolds II, International Press, Hong Kong, 1996] and string theory [Mod. Phys. Lett. A 12 (1997) 521; Nucl. Phys. B 451 (1995) 96] results. Finally, we revisit the conifold transition [Nucl. Phys. B 330 (1990) 49] as it applies in our formalism.  相似文献   

12.
[1]C.O.Weiss and R.Vilaseca,Dynamics of Lasers,VCH,Weinheim (1991); Instabilities and Chaos in Quantum Optics,eds.F.T.Arecchi and R.G.Harrison,Springer-Verlag,Berlin (1987). [2]H.Haken,Phys.Lett.A 53 (1975) 77. [3]Ju Rui,Huang Hong-Bin,Yang Peng,Xie Xia,and Zhao Huan,Commun.Theor.Phys.(Beijing,China) 44 (2005) 65; Ju Rui,Zhang Ya-Jun,Huang Hong-Bin,and Zhao Huan,Acta Phys.Sin.53 (2004) 2191 (in Chinese). [4]C.Z.Ning and H.Haken,Z.Phys.B 77 (1989) 247; B 77 (1989) 157; B 77 (1989) 163; J.Zakrenwski and M.Lewenstein,Phys.Rev.A 45 (1992) 2057. [5]G.J.deValearcel,E.Roldan,and R.Vilaseca,Phys.Rev.A 45 (1992) R2674; Phys.Rev.A 49 (1994) 1243. [6]X.Xie,H.B.Huang,F.Qian,Y.J.Zhang,P.Yang,and G.X.Qi,Commun.Theor.Phys.(Beijing,China) 46 (2006) 1042. [7]X.L.Deng,H.Q.Ma,B.D.Chen,and H.B.Huang,Phys.Lett.A 290 (2001) 77. [8]C.Benkert,and M.O.Scully,Phys.Rev.A 42 (1990) 2817. [9]M.O.Scully and M.S.Zubairy,Quantum Optics,Cambridge University Press,Cambridge (1997).  相似文献   

13.
Magnetic phases in PrCo2Si2 have been studied by measurements of magnetization, neutron diffraction and electrical resistivity. For <9 K, the magnetic structure with a propagation vector k = (0,0,1) [2π/c] is stable. Incommensurate structures k = (0,0,0.926) and (0,0,0.777) appear for 9 K < T <17 K and 17 K < T <30 K, respectively.  相似文献   

14.
A long-standing puzzle about the heterotic string has been what happens when an instanton shrinks to zero size. It is argued here that the answer at the quantum level is that an extra SU(2) gauge symmetry appears that is supported in the core of the instanton. Thus in particular the quantum heterotic string has vacua with higher rank than is possible in conformal field theory. When k instantons collapse at the same point, the enhanced gauge symmetry is Sp(k). These results, which can be tested by comparison to Dirichlet five-branes of Type I superstrings and to the ADHM construction of instantons, give the first example for the heterotic string of a non-perturbative phenomenon that cannot be turned off by making the coupling smaller. They have applications to several interesting puzzles about string duality.  相似文献   

15.
李静辉  黄祖洽 《中国物理》1997,6(5):341-347
We report a new model for infinite interacting noise driven subsystems which are coupled by a mean field and study its nonequilibrium phase transitions. In this model, under some circumstances the phase transition is between the state with zero mean field and the state with non zero mean field, and has a breaking of symmetry, which is similar to that reported by Van den Broeck, Parrondo, Toral, and Armcro [Phys. Rev. Lett.,73(1994),3395; Phys. Rev., E49(1994),2639], by Pikovsky, Rateitschak, and Kurths [Z.Phys.,B95(1994),541], and by other authors. We style this nonequi librium phase transition the symmetry breaking mean field. However, under other circumstances, the nonequilibrium phase transition of our model is not of the symme try breaking mean field type, which is a new phenomenon that has not been reported before.  相似文献   

16.
[1]G.T.Bodwin,E.Braaten,and G.P.Lepage,Phys.Rev.D 51 (1995) 1125;[Erratum-ibid.D 55 (1997) 5853][arXiv:hep-ph/9407339]; J.Boltz,P.Kroll,and G.A.Schulre,Phys.Lett.B 392 (1997) 198; J.Boltz,P.Kroll,and G.A.Schulre,Phys.J.C 2 (1998) 705. [2]S.M.Wong,Nucl.Phys.A 674 (2000) 185; S.M.Wong,Eur.Phys.J.C 14 (2000) 643. [3]J.Z.Bai,Y.Ban,J.G.Bian,et al.,Phys.Rev.D 67 (2003)112001. [4]M.Jacob and G.C.Wick,Ann.Phys.7 (1959) 404. [5]S.U.Chung,Phys.Rev.D 48 (1993) 1225; S.U.Chung,Phys.Rev.D 57 (1998) 431; B.S.Zou and D.V.Bugg,Eur.Phys.J.A 16 (2003) 537. [6]Particle Data Group,Phys.Lett.B 592 (2004) pp.924-966. [7]M.A.Doncheski,et al.,Phys.Rev.D 42 (1990) 2293; E.Eichten,et al.,Phys.Rev.D 21 (1980) 203; K.J.Sebastian,Phys.Rev.D 26 (1982) 2295; G.Hardekopf and J.Sucher,Phys.Rev.D 25 (1982) 2938; R.McClary and N.Byers,Phys.Rev.D 28 (1983) 1692; P.Moxhay and J.L.Rosner,Phys.Rev.D 28 (1983) 1132. [8]B.S.Zou and F.Hussain,Phys.Rev.C 67 (2003) 015204.  相似文献   

17.
We show that there is no contradiction between the results presented by Pan [Opt. Lett. 25, 369 (2000)] and the 1/L(2) dependence of the radiative energy flux between two half-spaces separated by a small vacuum gap of width L obtained by Polder and Van Hove [Phys. Rev. B 4, 3303 (1971)] and by Loomis and Maris [Phys. Rev. B 50, 18517 (1994)].  相似文献   

18.
If G is any finite product of compact orthogonal, unitary and symplectic matrix groups, then Wilson loops generate a dense subalgebra of continuous observables on the configuration space of lattice gauge theory with structure group G. If G is orthogonal, unitary or symplectic, then Wilson loops associated to the natural representation of G are enough.

This extends a result of Sengupta [Proc. Am. Math. Soc. 1221 (3) (1994) 897] and earlier work by Durhuus [Lett. Math. Phys. 4 (6) (1980) 515]. In particular, our approach includes the cases of even orthogonal and symplectic groups.  相似文献   


19.
Equilibrium and nonequilibrium properties of a chain of colliding harmonic oscillators (ding-dong model) are investigated. Our chain is modeled as harmonically bounded particles that can only interact with neighboring particles by hard-core interaction. Between the collisions, particles are just independent harmonic oscillators. We are especially interested in the stationary nonequilibrium state of the ding-dong model coupled with two stochastic heat reservoirs (not thermostated) at the ends, whose temperature is different. We check the Gallavotti-Cohen fluctuation theorem [G. Gallavoti and E. G. D. Cohen, Phys. Rev. Lett. 74, 2694 (1995)] and also the Evans-Searles identity [D. Evans and D. Searles, Phys. Rev. E. 50, 1994 (1994)] numerically. It is verified that the former theorem is satisfied for this system, although the system is not a thermostated system.  相似文献   

20.
通过介绍六粒子纠缠态的新应用研究,提出了一个二粒子任意态的信息分离方案.在这个方案中,发送者Alice、控制者Charlie和接受者Bob共享一个六粒子纠缠态,发送者先执行两次Bell基测量|然后控制者执行一次Bell基测量|最后接受者根据发送者和控制者的测量结果,对自己拥有的粒子做适当的幺正变换,从而能够重建要发送的二粒子任意态.这个信息分离方案是决定性的,即成功概率为100%.与使用相同的量子信道进行二粒子任意态的信息分离方案相比,本文提出的方案只需要进行Bell基测量而不需要执行多粒子的联合测量,从而使得这个方案更简单、更容易,并且在目前的实验室技术条件下是能够实现的.  相似文献   

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